pax_global_header 0000666 0000000 0000000 00000000064 12567135624 0014525 g ustar 00root root 0000000 0000000 52 comment=a2aa5e10f70f4cc8218050e43a961755c37e4d44
pyorbital-1.0.0/ 0000775 0000000 0000000 00000000000 12567135624 0013530 5 ustar 00root root 0000000 0000000 pyorbital-1.0.0/.gitignore 0000664 0000000 0000000 00000000534 12567135624 0015522 0 ustar 00root root 0000000 0000000 *.py[~cod]
# emacs
*~
# C extensions
*.so
# Packages
*.egg
*.egg-info
dist
build
eggs
parts
bin
var
sdist
develop-eggs
.installed.cfg
lib
lib64
__pycache__
# Installer logs
pip-log.txt
# Unit test / coverage reports
.coverage
.tox
nosetests.xml
# Translations
*.mo
# Mr Developer
.mr.developer.cfg
.project
.pydevproject
# rope
.ropeproject pyorbital-1.0.0/.travis.yml 0000664 0000000 0000000 00000000720 12567135624 0015640 0 ustar 00root root 0000000 0000000 language: python
python:
- '2.6'
- '2.7'
install:
- pip install .
- pip install coveralls
script: coverage run --source=pyorbital setup.py test
after_success: coveralls
deploy:
provider: pypi
user: Martin.Raspaud
password:
secure: P3WiHVzDAJyZmiIfSF3PhY7Xqp3P3pSHhogla8u3KOw4Sy5Ye6IWwMX1+pupAyhdXgo8ZgGT4+wOn9dBejaLEA0RGIRLMHXd1QxP9BbPD5te/k5aTpzHILx786g5R6G4yw/8s/sftQC6lJT+0jJd2OJjQJsnNUJJTG8OC2uwq3Y=
on:
tags: true
repo: mraspaud/pyorbital
pyorbital-1.0.0/LICENSE.txt 0000664 0000000 0000000 00000104513 12567135624 0015357 0 ustar 00root root 0000000 0000000 GNU GENERAL PUBLIC LICENSE
Version 3, 29 June 2007
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This program is distributed in the hope that it will be useful,
but WITHOUT ANY WARRANTY; without even the implied warranty of
MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
GNU General Public License for more details.
You should have received a copy of the GNU General Public License
along with this program. If not, see .
Also add information on how to contact you by electronic and paper mail.
If the program does terminal interaction, make it output a short
notice like this when it starts in an interactive mode:
Copyright (C)
This program comes with ABSOLUTELY NO WARRANTY; for details type `show w'.
This is free software, and you are welcome to redistribute it
under certain conditions; type `show c' for details.
The hypothetical commands `show w' and `show c' should show the appropriate
parts of the General Public License. Of course, your program's commands
might be different; for a GUI interface, you would use an "about box".
You should also get your employer (if you work as a programmer) or school,
if any, to sign a "copyright disclaimer" for the program, if necessary.
For more information on this, and how to apply and follow the GNU GPL, see
.
The GNU General Public License does not permit incorporating your program
into proprietary programs. If your program is a subroutine library, you
may consider it more useful to permit linking proprietary applications with
the library. If this is what you want to do, use the GNU Lesser General
Public License instead of this License. But first, please read
.
pyorbital-1.0.0/MANIFEST.in 0000664 0000000 0000000 00000000153 12567135624 0015265 0 ustar 00root root 0000000 0000000 include doc/Makefile
recursive-include doc/source *
include LICENSE.txt
include MANIFEST.in
include README
pyorbital-1.0.0/README 0000664 0000000 0000000 00000000267 12567135624 0014415 0 ustar 00root root 0000000 0000000 This is pyorbital, python package for computing orbital parameters from tle
files, and making diverse astronomical computations.
It is part of the pytroll project:
http://pytroll.org pyorbital-1.0.0/changelog.rst 0000664 0000000 0000000 00000027354 12567135624 0016224 0 ustar 00root root 0000000 0000000 Changelog
=========
v1.0.0 (2015-08-25)
-------------------
- Update changelog. [Martin Raspaud]
- Bump version: 0.3.2 → 1.0.0. [Martin Raspaud]
- Cleanup. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Fix version number. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Cosmetics. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge pull request #2 from pnuu/feature_tle_lookup. [Martin Raspaud]
Use NORAD catalog numbers for TLE reading
- Example file for mapping OSCAR platform names and NORAD catalog
numbers. [Panu Lahtinen]
- Add setup.cfg for easy rpm generation. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge branch 'develop' of github.com:mraspaud/pyorbital into develop.
[Martin Raspaud]
- Merge pull request #1 from spareeth/develop. [Martin Raspaud]
changes to avhrr_gacfunction and read_tle_decimal
- Added '+' as a condition in the read_tle function. [Sajid Pareeth]
- Renaming the variable scans_nb to scan_times in offset in avhrr_gac
function. [Sajid Pareeth]
- Bugfix: eccentricity too low message formatting. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Allow reading TLE from the most recent file described by the TLES env.
[Martin Raspaud]
Signed-off-by: Martin Raspaud
- Change decimate to frequency in avhrr instruments. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Add the avhrr instrument, gac version. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Accept missing zeros in TLE (old noaa compatibility). [Martin Raspaud]
- Add the horizon parameter to get_next_passes to get the
risetime/falltime at given angle. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge branch 'master' into develop. [Martin Raspaud]
- Fix backwards numpy compatibility. [Martin Raspaud]
Signed-off-by: Martin Raspaud
v0.3.2 (2014-04-10)
-------------------
- Merge branch 'develop' [Martin Raspaud]
- Bump up version number. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge branch 'feature-no-scipy' into develop. [Martin Raspaud]
- Remove scipy dependencies. [Martin Raspaud]
Was depending on scipy.optimize, brent and brentq function.
Replaced by secant method root finding and successive parabolic
interpolation local minimum finding.
Signed-off-by: Martin Raspaud
- Correcting the travis file. [Martin Raspaud]
Signed-off-by: Martin Raspaud
v0.3.1 (2014-02-24)
-------------------
- Bugfix in travis file. [Martin Raspaud]
- Bump up version number. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Fixed documentation. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Cleanup. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- New nadir computations for geoloc. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- More unit tests. [Martin Raspaud]
Signed-off-by: Martin Raspaud
v0.3.0 (2014-01-07)
-------------------
- Auto update version number in documentation. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Change to version file and bump up to v0.3.0. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Cleanup the testfiles. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Add a test to read tle from file. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Fix doc path in MANIFEST.in. [Martin Raspaud]
Signed-off-by: Martin Raspaud
v0.2.4 (2014-01-07)
-------------------
- Merge branch 'feature-travis' into pre-master. [Martin Raspaud]
- Add test for tle reading, cleanup and make ready for travis. [Martin
Raspaud]
Signed-off-by: Martin Raspaud
- Cleanup. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Add function to fetch the tle files from internet manually. [Martin
Raspaud]
Signed-off-by: Martin Raspaud
- Adding the viirs instrument. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Change sphinx theme. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Fix doc for readthedocs. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Remove unused old file. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge branch 'geoloc' into pre-master. [Martin Raspaud]
- Work on geolocation. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Numpyze the orbital computation. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Add some logging in tle file fetching. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Fix syntax error in doc/conf.py. [Martin Raspaud]
- Make the scan angle of avhrr an argument. [Martin Raspaud]
- Factorize avhrr code (geoloc definition) [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Add Mikhail's definition of AMSU-A. [Martin Raspaud]
- Add instrument examples for geoloc. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge branch 'geoloc' of github.com:mraspaud/pyorbital into geoloc.
[Martin Raspaud]
- Try fixing nadir. [Martin Raspaud]
- Fix attitude. [Martin Raspaud]
- Updated doc and copyright. [Martin Raspaud]
- Add geoloc example. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Merge branch 'feature-vectorize' into geoloc. [Martin Raspaud]
- Vectorize the days function. [Martin Raspaud]
- Merge branch 'master' into geoloc. [Martin Raspaud]
- Merge branch 'pre-master' into geoloc. [Martin Raspaud]
- Cosmetics. [Martin Raspaud]
- Computations for true nadir. [Martin Raspaud]
- Bugfix in the example and added attitude correction (roll and pitch
for now). [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Cosmetic, be consistent in name og time argument as 'utc_time' [Lars
Orum Rasmussen]
- Get_zenith_overpass replaced by Martin's get_next_passes. [Lars Orum
Rasmussen]
- Add sun_earth_distance_correction function. [Martin Raspaud]
v0.2.3 (2013-03-07)
-------------------
- Merge branch 'release-0.2.3' [Martin Raspaud]
- Merge branch 'pre-master' into release-0.2.3. [Martin Raspaud]
- Bumped up version number. [Martin Raspaud]
- Corrected search for previous an_time with a substracted 10 min. dt.
[Esben S. Nielsen]
- Merge branch 'release-0.2.2' [Martin Raspaud]
- Import with_statement in test_aiaa.py for python 2.5 compliance.
[Esben S. Nielsen]
- Made unit tests python 2.5 and 2.6 compliant. [Esben S. Nielsen]
- Removed download URL from setup.py. [Esben S. Nielsen]
- Bumped version number and marked as stable. [Esben S. Nielsen]
- Better handling of time deltas in test_aiaa.py. [Esben S. Nielsen]
- Updated equator test with position check. [Esben S. Nielsen]
- Now uses nodal period for orbit number calculation instead of revs/day
for mean motion. [Esben S. Nielsen]
- Orbit number now handles epoch AN mis-match. Made AIAA unit test path
agnostic. [Esben S. Nielsen]
- Better __main__ [Lars Orum Rasmussen]
- Adding risetime and falltime functions, and improving the
get_zenith_overpass function. [Adam Dybbroe]
- Editorial. [Adam Dybbroe]
- Cleanup. [Martin Raspaud]
Signed-off-by: Martin Raspaud
- Feature: Correcting/adding test cases from the aiaa. [Martin Raspaud]
- Style: raises NotImplementedErrors instead of just Exceptions. [Martin
Raspaud]
- Merge branch 'pre-master' of github.com:mraspaud/pyorbital into pre-
master. [Martin Raspaud]
- Adding new function get_zenith_overpass to get the time when the
satellite passes over zenith relative to an observer on ground. [Adam
Dybbroe]
- Feature: Added checksum for tle lines. [Martin Raspaud]
v0.2.1 (2012-06-01)
-------------------
- Updated version number. [Martin Raspaud]
- Added pyorbital path to doc/source/conf.py. [Esben S. Nielsen]
- Updated docs and added license and manifest. [Esben S. Nielsen]
- Merge branch 'pre-master' of https://github.com/mraspaud/pyorbital
into pre-master. [Adam Dybbroe]
- Merge branch 'pre-master' of https://github.com/mraspaud/pyorbital
into pre-master. [Lars Orum Rasmussen]
- Added access to line1 and line2 in a Tle instance. [Lars Orum
Rasmussen]
Change satellite to platform
- Spelling error. [Adam Dybbroe]
v0.2.0 (2012-05-14)
-------------------
- Prepared for pypi. [Martin Raspaud]
- Merge branch 'geoloc' into pre-master. [Martin Raspaud]
- Added now compute pixels on the ellipsoid, not on the sphere anymore.
[Martin Raspaud]
- Merge branch 'master' into geoloc. [Martin Raspaud]
- Updated the geoloc todo list. [Martin Raspaud]
- Added the geoloc module. [Martin Raspaud]
- Merge branch 'master' into pre-master. [Martin Raspaud]
Conflicts:
pyorbital/tlefile.py
- Corrected handling of mean motion and orbitnumber fields in
tlefiles.py. [Esben S. Nielsen]
- Testing getting the orbit number from the TLEs. [Adam.Dybbroe]
- Fixing bug in tle file reading, so that also NPP and other satellites
with orbit numbers less than 9999 can be handled. [Adam.Dybbroe]
- Typo. [Adam.Dybbroe]
- Merge branch 'master' into pre-master. [Martin Raspaud]
- Removed html submodule. [Martin Raspaud]
- Fixing bug in function sun_zenith_angle. Changing interfaces so that
all public functions expects lon,lat in degrees. All internal
functions us radians. Made the lsmt and local_hour_angle functions
private. [Adam.Dybbroe]
- Adding main. [Adam.Dybbroe]
- Gathering unit tests to the tests-directory. [Adam.Dybbroe]
- Added separate test-script for astronomy.py. [Adam.Dybbroe]
- Collected all unit test scripts under the tests directory.
[Adam.Dybbroe]
- Merge branch 'release-0.2.0' [Martin Raspaud]
Conflicts:
doc/build
setup.py
- Bumped version number to 0.2.0. [Martin Raspaud]
- Added html documentation. [Martin Raspaud]
- Corrected sgp4's propagate in the case of array as input, and cleaned
up. [Martin Raspaud]
- Fixed calling test_aiaa from another directory. [Martin Raspaud]
- Vectorize merge. [Martin Raspaud]
- Merging master branch. [Martin Raspaud]
- Remove html submodule. [Martin Raspaud]
- Remove html submodule. [Martin Raspaud]
- Added Esben in the author field. [Martin Raspaud]
- Removed unneded .pyc file. [Martin Raspaud]
- Added unittests. [Esben S. Nielsen]
- Corrected observer_look function and added first unittest. [Esben S.
Nielsen]
- Corrected observer_pos in astronomy. [Esben S. Nielsen]
- Setting up documentation. [Martin Raspaud]
v0.1.0 (2011-10-03)
-------------------
- Merge branch 'release-0.1.0' [Martin Raspaud]
- Bumped version number to 0.1.0. [Martin Raspaud]
- Merge branch 'dundee_port' into pre-master. [Martin Raspaud]
- Cleanup and documentation. [Martin Raspaud]
- Now using unittest module for aiaa test cases. [Martin Raspaud]
- Added licences, and removed prints. [Martin Raspaud]
- Added basic tests to pyorbital. [Martin Raspaud]
- Ported SGP4 code to Dundee implementation. [Esben S. Nielsen]
- Ported sgp4 init. [Esben S. Nielsen]
- Added the first unit test :) [Martin Raspaud]
- New gmst function (from AIAA paper). Cleaning. [Martin Raspaud]
- Merged DMI and SMHI versions. [Esben S. Nielsen]
- Made the package more package-like. [Martin Raspaud]
- Cleanup of astronomy file. [Martin Raspaud]
- Added a readme file. [Martin Raspaud]
- Added astronomy.py file. [Martin Raspaud]
pyorbital-1.0.0/doc/ 0000775 0000000 0000000 00000000000 12567135624 0014275 5 ustar 00root root 0000000 0000000 pyorbital-1.0.0/doc/Makefile 0000664 0000000 0000000 00000010776 12567135624 0015750 0 ustar 00root root 0000000 0000000 # Makefile for Sphinx documentation
#
# You can set these variables from the command line.
SPHINXOPTS =
SPHINXBUILD = sphinx-build
PAPER =
BUILDDIR = build
# Internal variables.
PAPEROPT_a4 = -D latex_paper_size=a4
PAPEROPT_letter = -D latex_paper_size=letter
ALLSPHINXOPTS = -d $(BUILDDIR)/doctrees $(PAPEROPT_$(PAPER)) $(SPHINXOPTS) source
.PHONY: help clean html dirhtml singlehtml pickle json htmlhelp qthelp devhelp epub latex latexpdf text man changes linkcheck doctest
help:
@echo "Please use \`make ' where is one of"
@echo " html to make standalone HTML files"
@echo " dirhtml to make HTML files named index.html in directories"
@echo " singlehtml to make a single large HTML file"
@echo " pickle to make pickle files"
@echo " json to make JSON files"
@echo " htmlhelp to make HTML files and a HTML help project"
@echo " qthelp to make HTML files and a qthelp project"
@echo " devhelp to make HTML files and a Devhelp project"
@echo " epub to make an epub"
@echo " latex to make LaTeX files, you can set PAPER=a4 or PAPER=letter"
@echo " latexpdf to make LaTeX files and run them through pdflatex"
@echo " text to make text files"
@echo " man to make manual pages"
@echo " changes to make an overview of all changed/added/deprecated items"
@echo " linkcheck to check all external links for integrity"
@echo " doctest to run all doctests embedded in the documentation (if enabled)"
clean:
-rm -rf $(BUILDDIR)/*
html:
$(SPHINXBUILD) -b html $(ALLSPHINXOPTS) $(BUILDDIR)/html
@echo
@echo "Build finished. The HTML pages are in $(BUILDDIR)/html."
dirhtml:
$(SPHINXBUILD) -b dirhtml $(ALLSPHINXOPTS) $(BUILDDIR)/dirhtml
@echo
@echo "Build finished. The HTML pages are in $(BUILDDIR)/dirhtml."
singlehtml:
$(SPHINXBUILD) -b singlehtml $(ALLSPHINXOPTS) $(BUILDDIR)/singlehtml
@echo
@echo "Build finished. The HTML page is in $(BUILDDIR)/singlehtml."
pickle:
$(SPHINXBUILD) -b pickle $(ALLSPHINXOPTS) $(BUILDDIR)/pickle
@echo
@echo "Build finished; now you can process the pickle files."
json:
$(SPHINXBUILD) -b json $(ALLSPHINXOPTS) $(BUILDDIR)/json
@echo
@echo "Build finished; now you can process the JSON files."
htmlhelp:
$(SPHINXBUILD) -b htmlhelp $(ALLSPHINXOPTS) $(BUILDDIR)/htmlhelp
@echo
@echo "Build finished; now you can run HTML Help Workshop with the" \
".hhp project file in $(BUILDDIR)/htmlhelp."
qthelp:
$(SPHINXBUILD) -b qthelp $(ALLSPHINXOPTS) $(BUILDDIR)/qthelp
@echo
@echo "Build finished; now you can run "qcollectiongenerator" with the" \
".qhcp project file in $(BUILDDIR)/qthelp, like this:"
@echo "# qcollectiongenerator $(BUILDDIR)/qthelp/pyorbital.qhcp"
@echo "To view the help file:"
@echo "# assistant -collectionFile $(BUILDDIR)/qthelp/pyorbital.qhc"
devhelp:
$(SPHINXBUILD) -b devhelp $(ALLSPHINXOPTS) $(BUILDDIR)/devhelp
@echo
@echo "Build finished."
@echo "To view the help file:"
@echo "# mkdir -p $$HOME/.local/share/devhelp/pyorbital"
@echo "# ln -s $(BUILDDIR)/devhelp $$HOME/.local/share/devhelp/pyorbital"
@echo "# devhelp"
epub:
$(SPHINXBUILD) -b epub $(ALLSPHINXOPTS) $(BUILDDIR)/epub
@echo
@echo "Build finished. The epub file is in $(BUILDDIR)/epub."
latex:
$(SPHINXBUILD) -b latex $(ALLSPHINXOPTS) $(BUILDDIR)/latex
@echo
@echo "Build finished; the LaTeX files are in $(BUILDDIR)/latex."
@echo "Run \`make' in that directory to run these through (pdf)latex" \
"(use \`make latexpdf' here to do that automatically)."
latexpdf:
$(SPHINXBUILD) -b latex $(ALLSPHINXOPTS) $(BUILDDIR)/latex
@echo "Running LaTeX files through pdflatex..."
make -C $(BUILDDIR)/latex all-pdf
@echo "pdflatex finished; the PDF files are in $(BUILDDIR)/latex."
text:
$(SPHINXBUILD) -b text $(ALLSPHINXOPTS) $(BUILDDIR)/text
@echo
@echo "Build finished. The text files are in $(BUILDDIR)/text."
man:
$(SPHINXBUILD) -b man $(ALLSPHINXOPTS) $(BUILDDIR)/man
@echo
@echo "Build finished. The manual pages are in $(BUILDDIR)/man."
changes:
$(SPHINXBUILD) -b changes $(ALLSPHINXOPTS) $(BUILDDIR)/changes
@echo
@echo "The overview file is in $(BUILDDIR)/changes."
linkcheck:
$(SPHINXBUILD) -b linkcheck $(ALLSPHINXOPTS) $(BUILDDIR)/linkcheck
@echo
@echo "Link check complete; look for any errors in the above output " \
"or in $(BUILDDIR)/linkcheck/output.txt."
doctest:
$(SPHINXBUILD) -b doctest $(ALLSPHINXOPTS) $(BUILDDIR)/doctest
@echo "Testing of doctests in the sources finished, look at the " \
"results in $(BUILDDIR)/doctest/output.txt."
pyorbital-1.0.0/doc/source/ 0000775 0000000 0000000 00000000000 12567135624 0015575 5 ustar 00root root 0000000 0000000 pyorbital-1.0.0/doc/source/conf.py 0000664 0000000 0000000 00000016117 12567135624 0017102 0 ustar 00root root 0000000 0000000 # -*- coding: utf-8 -*-
#
# pyorbital documentation build configuration file, created by
# sphinx-quickstart on Mon Oct 3 08:48:29 2011.
#
# This file is execfile()d with the current directory set to its containing dir.
#
# Note that not all possible configuration values are present in this
# autogenerated file.
#
# All configuration values have a default; values that are commented out
# serve to show the default.
import sys
import os
# If extensions (or modules to document with autodoc) are in another directory,
# add these directories to sys.path here. If the directory is relative to the
# documentation root, use os.path.abspath to make it absolute, like shown here.
#sys.path.insert(0, os.path.abspath('.'))
sys.path.insert(0, os.path.abspath('../../'))
sys.path.insert(0, os.path.abspath('../../pyorbital'))
from pyorbital.version import __version__
# -- General configuration -----------------------------------------------------
# If your documentation needs a minimal Sphinx version, state it here.
#needs_sphinx = '1.0'
# Add any Sphinx extension module names here, as strings. They can be extensions
# coming with Sphinx (named 'sphinx.ext.*') or your custom ones.
extensions = ['sphinx.ext.autodoc', 'sphinx.ext.doctest', 'sphinx.ext.coverage']
# Add any paths that contain templates here, relative to this directory.
templates_path = ['.templates']
# The suffix of source filenames.
source_suffix = '.rst'
# The encoding of source files.
#source_encoding = 'utf-8-sig'
# The master toctree document.
master_doc = 'index'
# General information about the project.
project = u'pyorbital'
copyright = u'2012-2015, The Pytroll crew'
# The version info for the project you're documenting, acts as replacement for
# |version| and |release|, also used in various other places throughout the
# built documents.
#
# The full version, including alpha/beta/rc tags.
release = __version__
# The short X.Y version.
version = ".".join(release.split(".")[:2])
# The language for content autogenerated by Sphinx. Refer to documentation
# for a list of supported languages.
#language = None
# There are two options for replacing |today|: either, you set today to some
# non-false value, then it is used:
#today = ''
# Else, today_fmt is used as the format for a strftime call.
#today_fmt = '%B %d, %Y'
# List of patterns, relative to source directory, that match files and
# directories to ignore when looking for source files.
exclude_patterns = []
# The reST default role (used for this markup: `text`) to use for all documents.
#default_role = None
# If true, '()' will be appended to :func: etc. cross-reference text.
#add_function_parentheses = True
# If true, the current module name will be prepended to all description
# unit titles (such as .. function::).
#add_module_names = True
# If true, sectionauthor and moduleauthor directives will be shown in the
# output. They are ignored by default.
#show_authors = False
# The name of the Pygments (syntax highlighting) style to use.
pygments_style = 'sphinx'
# A list of ignored prefixes for module index sorting.
#modindex_common_prefix = []
# -- Options for HTML output ---------------------------------------------------
# The theme to use for HTML and HTML Help pages. See the documentation for
# a list of builtin themes.
html_theme = 'default'
# Theme options are theme-specific and customize the look and feel of a theme
# further. For a list of options available for each theme, see the
# documentation.
#html_theme_options = {}
# Add any paths that contain custom themes here, relative to this directory.
#html_theme_path = []
# The name for this set of Sphinx documents. If None, it defaults to
# " v documentation".
#html_title = None
# A shorter title for the navigation bar. Default is the same as html_title.
#html_short_title = None
# The name of an image file (relative to this directory) to place at the top
# of the sidebar.
#html_logo = None
# The name of an image file (within the static path) to use as favicon of the
# docs. This file should be a Windows icon file (.ico) being 16x16 or 32x32
# pixels large.
#html_favicon = None
# Add any paths that contain custom static files (such as style sheets) here,
# relative to this directory. They are copied after the builtin static files,
# so a file named "default.css" will overwrite the builtin "default.css".
html_static_path = ['.static']
# If not '', a 'Last updated on:' timestamp is inserted at every page bottom,
# using the given strftime format.
#html_last_updated_fmt = '%b %d, %Y'
# If true, SmartyPants will be used to convert quotes and dashes to
# typographically correct entities.
#html_use_smartypants = True
# Custom sidebar templates, maps document names to template names.
#html_sidebars = {}
# Additional templates that should be rendered to pages, maps page names to
# template names.
#html_additional_pages = {}
# If false, no module index is generated.
#html_domain_indices = True
# If false, no index is generated.
#html_use_index = True
# If true, the index is split into individual pages for each letter.
#html_split_index = False
# If true, links to the reST sources are added to the pages.
#html_show_sourcelink = True
# If true, "Created using Sphinx" is shown in the HTML footer. Default is True.
#html_show_sphinx = True
# If true, "(C) Copyright ..." is shown in the HTML footer. Default is True.
#html_show_copyright = True
# If true, an OpenSearch description file will be output, and all pages will
# contain a tag referring to it. The value of this option must be the
# base URL from which the finished HTML is served.
#html_use_opensearch = ''
# This is the file name suffix for HTML files (e.g. ".xhtml").
#html_file_suffix = None
# Output file base name for HTML help builder.
htmlhelp_basename = 'pyorbitaldoc'
# -- Options for LaTeX output --------------------------------------------------
# The paper size ('letter' or 'a4').
#latex_paper_size = 'letter'
# The font size ('10pt', '11pt' or '12pt').
#latex_font_size = '10pt'
# Grouping the document tree into LaTeX files. List of tuples
# (source start file, target name, title, author, documentclass [howto/manual]).
latex_documents = [
('index', 'pyorbital.tex', u'pyorbital Documentation',
u'The Pytroll crew', 'manual'),
]
# The name of an image file (relative to this directory) to place at the top of
# the title page.
#latex_logo = None
# For "manual" documents, if this is true, then toplevel headings are parts,
# not chapters.
#latex_use_parts = False
# If true, show page references after internal links.
#latex_show_pagerefs = False
# If true, show URL addresses after external links.
#latex_show_urls = False
# Additional stuff for the LaTeX preamble.
#latex_preamble = ''
# Documents to append as an appendix to all manuals.
#latex_appendices = []
# If false, no module index is generated.
#latex_domain_indices = True
# -- Options for manual page output --------------------------------------------
# One entry per manual page. List of tuples
# (source start file, name, description, authors, manual section).
man_pages = [
('index', 'pyorbital', u'pyorbital Documentation',
[u'The Pytroll crew'], 1)
]
pyorbital-1.0.0/doc/source/index.rst 0000664 0000000 0000000 00000004572 12567135624 0017446 0 ustar 00root root 0000000 0000000 .. pyorbital documentation master file, created by
sphinx-quickstart on Mon Oct 3 08:48:29 2011.
You can adapt this file completely to your liking, but it should at least
contain the root `toctree` directive.
Pyorbital
=========
Pyorbital is a python package to compute orbital parameters for satellites from
TLE files as well as astronomical parameters of interest for satellite remote sensing.
Currently pyorbital only supports low earth orbit satellites.
TLE files
---------
Pyorbital has a module for parsing NORAD TLE-files
>>> from pyorbital import tlefile
>>> tle = tlefile.read('noaa 18', '/path/to/my/tle_file.txt')
>>> tle.inclination
99.043499999999995
If no path is given pyorbital tries to read the earth observation TLE-files from celestrak.com
Computing satellite postion
---------------------------
The orbital module enables computation of satellite position and velocity at a specific time:
>>> from pyorbital.orbital import Orbital
>>> from datetime import datetime
>>> orb = Orbital("noaa 18")
>>> now = datetime.utcnow()
>>> # Get normalized position and velocity of the satellite:
>>> orb.get_position(now)
([0.57529384846822862, 0.77384005228105424, 0.59301408257897559],
[0.031846489698768146, 0.021287993461926374, -0.05854106186659274])
>>> # Get longitude, latitude and altitude of the satellite:
>>> orb.get_lonlatalt(now)
(-1.1625895579622014, 0.55402132517640568, 847.89381184656702)
Computing astronomical parameters
---------------------------------
The astronomy module enables computation of certain parameters of interest for satellite remote sensing for instance the Sun-zenith angle:
>>> from pyorbital import astronomy
>>> from datetime import datetime
>>> utc_time = datetime(2012, 5, 15, 15, 45)
>>> lon, lat = 12, 56
>>> astronomy.sun_zenith_angle(utc_time, lon, lat)
62.685986438071602
API
---
Orbital computations
~~~~~~~~~~~~~~~~~~~~
.. automodule:: pyorbital.orbital
:members:
:undoc-members:
TLE handling
~~~~~~~~~~~~
.. automodule:: pyorbital.tlefile
:members:
:undoc-members:
Astronomical computations
~~~~~~~~~~~~~~~~~~~~~~~~~
.. automodule:: pyorbital.astronomy
:members:
:undoc-members:
.. Contents:
.. toctree::
:maxdepth: 2
Indices and tables
==================
* :ref:`genindex`
* :ref:`modindex`
* :ref:`search`
pyorbital-1.0.0/etc/ 0000775 0000000 0000000 00000000000 12567135624 0014303 5 ustar 00root root 0000000 0000000 pyorbital-1.0.0/etc/platforms.txt 0000664 0000000 0000000 00000002004 12567135624 0017047 0 ustar 00root root 0000000 0000000 # The platform numbers are given in a file $PPP_CONFIG_DIR/platforms.txt
# in the following format. Copy this file to $PPP_CONFIG_DIR
#
# Mappings between satellite catalogue numbers and corresponding
# platform names from OSCAR.
ALOS-2 39766
CloudSat 29107
CryoSat-2 36508
CSK-1 31598
CSK-2 32376
CSK-3 33412
CSK-4 37216
DMSP-F15 25991
DMSP-F16 28054
DMSP-F17 29522
DMSP-F18 35951
DMSP-F19 39630
EOS-Aqua 27424
EOS-Aura 28376
EOS-Terra 25994
FY-2D 29640
FY-2E 33463
FY-2F 38049
FY-2G 40367
FY-3A 32958
FY-3B 37214
FY-3C 39260
GOES-13 29155
GOES-14 35491
GOES-15 36411
Himawari-6 28622
Himawari-7 28937
Himawari-8 40267
INSAT-3A 27714
INSAT-3C 27298
INSAT-3D 39216
JASON-2 33105
Kalpana-1 27525
Landsat-7 25682
Landsat-8 39084
Meteosat-7 24932
Meteosat-8 27509
Meteosat-9 28912
Meteosat-10 38552
Metop-A 29499
Metop-B 38771
NOAA-15 25338
NOAA-16 26536
NOAA-17 27453
NOAA-18 28654
NOAA-19 33591
RadarSat-2 32382
Sentinel-1A 39634
SMOS 36036
SPOT-5 27421
SPOT-6 38755
SPOT-7 40053
Suomi-NPP 37849
TanDEM-X 36605
TerraSAR-X 31698
pyorbital-1.0.0/pyorbital/ 0000775 0000000 0000000 00000000000 12567135624 0015535 5 ustar 00root root 0000000 0000000 pyorbital-1.0.0/pyorbital/__init__.py 0000664 0000000 0000000 00000000000 12567135624 0017634 0 ustar 00root root 0000000 0000000 pyorbital-1.0.0/pyorbital/astronomy.py 0000664 0000000 0000000 00000014036 12567135624 0020146 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2011, 2013
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Astronomy module.
Parts taken from http://www.geoastro.de/elevaz/basics/index.htm
"""
import datetime
import numpy as np
F = 1 / 298.257223563 # Earth flattening WGS-84
A = 6378.137 # WGS84 Equatorial radius
MFACTOR = 7.292115E-5
def jdays2000(utc_time):
"""Get the days since year 2000.
"""
return _days(utc_time - datetime.datetime(2000, 1, 1, 12, 0))
def jdays(utc_time):
"""Get the julian day of *utc_time*.
"""
return jdays2000(utc_time) + 2451545
def _fdays(dt):
"""Get the days (floating point) from *d_t*.
"""
return (dt.days +
(dt.seconds +
dt.microseconds / (1000000.0)) / (24 * 3600.0))
_vdays = np.vectorize(_fdays)
def _days(dt):
"""Get the days (floating point) from *d_t*.
"""
try:
return _fdays(dt)
except AttributeError:
return _vdays(dt)
def gmst(utc_time):
"""Greenwich mean sidereal utc_time, in radians.
As defined in the AIAA 2006 implementation:
http://www.celestrak.com/publications/AIAA/2006-6753/
"""
ut1 = jdays2000(utc_time) / 36525.0
theta = 67310.54841 + ut1 * (876600 * 3600 + 8640184.812866 + ut1 *
(0.093104 - ut1 * 6.2 * 10e-6))
return np.deg2rad(theta / 240.0) % (2 * np.pi)
def _lmst(utc_time, longitude):
"""Local mean sidereal time, computed from *utc_time* and *longitude*.
In radians.
"""
return gmst(utc_time) + longitude
def sun_ecliptic_longitude(utc_time):
"""Ecliptic longitude of the sun at *utc_time*.
"""
jdate = jdays2000(utc_time) / 36525.0
# mean anomaly, rad
m_a = np.deg2rad(357.52910 +
35999.05030*jdate -
0.0001559*jdate*jdate -
0.00000048*jdate*jdate*jdate)
# mean longitude, deg
l_0 = 280.46645 + 36000.76983*jdate + 0.0003032*jdate*jdate
d_l = ((1.914600 - 0.004817*jdate - 0.000014*jdate*jdate)*np.sin(m_a) +
(0.019993 - 0.000101*jdate)*np.sin(2*m_a) + 0.000290*np.sin(3*m_a))
# true longitude, deg
l__ = l_0 + d_l
return np.deg2rad(l__)
def sun_ra_dec(utc_time):
"""Right ascension and declination of the sun at *utc_time*.
"""
jdate = jdays2000(utc_time) / 36525.0
eps = np.deg2rad(23.0 + 26.0/60.0 + 21.448/3600.0 -
(46.8150*jdate + 0.00059*jdate*jdate -
0.001813*jdate*jdate*jdate) / 3600)
eclon = sun_ecliptic_longitude(utc_time)
x__ = np.cos(eclon)
y__ = np.cos(eps) * np.sin(eclon)
z__ = np.sin(eps) * np.sin(eclon)
r__ = np.sqrt(1.0 - z__ * z__)
# sun declination
declination = np.arctan2(z__, r__)
# right ascension
right_ascension = 2 * np.arctan2(y__, (x__ + r__))
return right_ascension, declination
def _local_hour_angle(utc_time, longitude, right_ascension):
"""Hour angle at *utc_time* for the given *longitude* and
*right_ascension*
longitude in radians
"""
return _lmst(utc_time, longitude) - right_ascension
def get_alt_az(utc_time, lon, lat):
"""Return sun altitude and azimuth from *utc_time*, *lon*, and *lat*.
lon,lat in degrees
What is the unit of the returned angles and heights!? FIXME!
"""
lon = np.deg2rad(lon)
lat = np.deg2rad(lat)
ra_, dec = sun_ra_dec(utc_time)
h__ = _local_hour_angle(utc_time, lon, ra_)
return (np.arcsin(np.sin(lat)*np.sin(dec) +
np.cos(lat) * np.cos(dec) * np.cos(h__)),
np.arctan2(-np.sin(h__), (np.cos(lat)*np.tan(dec) -
np.sin(lat)*np.cos(h__))))
def cos_zen(utc_time, lon, lat):
"""Cosine of the sun-zenith angle for *lon*, *lat* at *utc_time*.
utc_time: datetime.datetime instance of the UTC time
lon and lat in degrees.
"""
lon = np.deg2rad(lon)
lat = np.deg2rad(lat)
r_a, dec = sun_ra_dec(utc_time)
h__ = _local_hour_angle(utc_time, lon, r_a)
return (np.sin(lat)*np.sin(dec) + np.cos(lat) * np.cos(dec) * np.cos(h__))
def sun_zenith_angle(utc_time, lon, lat):
"""Sun-zenith angle for *lon*, *lat* at *utc_time*.
lon,lat in degrees.
The angle returned is given in degrees
"""
return np.rad2deg(np.arccos(cos_zen(utc_time, lon, lat)))
def sun_earth_distance_correction(utc_time):
"""Calculate the sun earth distance correction, relative to 1 AU.
"""
year = 365.256363004
# This is computed from
# http://curious.astro.cornell.edu/question.php?number=582
# AU = 149597870700.0
# a = 149598261000.0
# theta = (jdays2000(utc_time) - 2) * (2 * np.pi) / year
# e = 0.01671123
# r = a*(1-e*e)/(1+e * np.cos(theta))
# corr_me = (r / AU) ** 2
# from known software.
corr = 1 - 0.0334 * np.cos(2 * np.pi * (jdays2000(utc_time) - 2) / year)
return corr
def observer_position(time, lon, lat, alt):
"""Calculate observer ECI position.
http://celestrak.com/columns/v02n03/
"""
lon = np.deg2rad(lon)
lat = np.deg2rad(lat)
theta = (gmst(time) + lon) % (2 * np.pi)
c = 1 / np.sqrt(1 + F * (F - 2) * np.sin(lat)**2)
sq = c * (1 - F)**2
achcp = (A * c + alt) * np.cos(lat)
x = achcp * np.cos(theta) # kilometers
y = achcp * np.sin(theta)
z = (A * sq + alt) * np.sin(lat)
vx = -MFACTOR*y # kilometers/second
vy = MFACTOR*x
vz = 0
return (x, y, z), (vx, vy, vz)
pyorbital-1.0.0/pyorbital/geoloc.py 0000664 0000000 0000000 00000022320 12567135624 0017356 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2011, 2012, 2013, 2014, 2015.
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Module to compute geolocalization of a satellite scene.
"""
# TODO:
# - Attitude correction
# - project on an ellipsoid instead of a sphere
# - optimize !!!
# - test !!!
import numpy as np
from numpy import cos, sin, sqrt
from datetime import timedelta
from pyorbital.orbital import Orbital
a = 6378.137 # km
b = 6356.75231414 # km, GRS80
# b = 6356.752314245 # km, WGS84
def geodetic_lat(point, a=a, b=b):
x, y, z = point
r = np.sqrt(x * x + y * y)
geoc_lat = np.arctan2(z, r)
geod_lat = geoc_lat
e2 = (a * a - b * b) / (a * a)
while True:
phi = geod_lat
C = 1 / sqrt(1 - e2 * sin(phi)**2)
geod_lat = np.arctan2(z + a * C * e2 * sin(phi), r)
if np.allclose(geod_lat, phi):
return geod_lat
def subpoint(query_point, a=a, b=b):
"""Get the point on the ellipsoid under the *query_point*.
"""
x, y, z = query_point
r = sqrt(x * x + y * y)
lat = geodetic_lat(query_point)
lon = np.arctan2(y, x)
e2_ = (a * a - b * b) / (a * a)
n__ = a / sqrt(1 - e2_ * sin(lat)**2)
nx_ = n__ * cos(lat) * cos(lon)
ny_ = n__ * cos(lat) * sin(lon)
nz_ = (1 - e2_) * n__ * sin(lat)
return np.vstack([nx_, ny_, nz_])
class ScanGeometry(object):
"""Description of the geometry of an instrument.
*fovs* is the x and y viewing angles of the instrument. y is zero if the we
talk about scanlines of course. *times* is the time of viewing of each
angle relative to the start of the scanning, so it should have the same
size as the *fovs*. *attitude* is the attitude correction to apply.
"""
def __init__(self,
fovs,
times,
attitude=(0, 0, 0)):
self.fovs = np.array(fovs)
self._times = np.array(times)
self.attitude = attitude
def vectors(self, pos, vel, roll=0.0, pitch=0.0, yaw=0.0):
"""Get unit vectors pointing to the different pixels.
*pos* and *vel* are column vectors, or matrices of column
vectors. Returns vectors as stacked rows.
"""
# TODO: yaw steering mode !
# Fake nadir: This is the intersection point between the satellite
# looking down at the centre of the ellipsoid and the surface of the
# ellipsoid. Nadir on the other hand is the point which vertical goes
# through the satellite...
#nadir = -pos / vnorm(pos)
nadir = subpoint(-pos)
nadir /= vnorm(nadir)
# x is along track (roll)
x = vel / vnorm(vel)
# y is cross track (pitch)
y = np.cross(nadir, vel, 0, 0, 0)
y /= vnorm(y)
# rotate first around x
x_rotated = qrotate(nadir, x, self.fovs[:, 0] + roll)
# then around y
xy_rotated = qrotate(x_rotated, y, self.fovs[:, 1] + pitch)
# then around z
return qrotate(xy_rotated, nadir, yaw)
def times(self, start_of_scan):
tds = [timedelta(seconds=i) for i in self._times]
return np.array(tds) + start_of_scan
class Quaternion(object):
def __init__(self, scalar, vector):
self.__x, self.__y, self.__z = vector
self.__w = scalar
def rotation_matrix(self):
x, y, z, w = self.__x, self.__y, self.__z, self.__w
zero = np.zeros_like(x)
return np.array(
((w**2 + x**2 - y**2 - z**2,
2 * x * y + 2 * z * w,
2 * x * z - 2 * y * w,
zero),
(2 * x * y - 2 * z * w,
w**2 - x**2 + y**2 - z**2,
2 * y * z + 2 * x * w,
zero),
(2 * x * z + 2 * y * w,
2 * y * z - 2 * x * w,
w**2 - x**2 - y**2 + z**2,
zero),
(zero, zero, zero, w**2 + x**2 + y**2 + z**2)))
def qrotate(vector, axis, angle):
"""Rotate *vector* around *axis* by *angle* (in radians).
*vector* is a matrix of column vectors, as is *axis*.
This function uses quaternion rotation.
"""
n_axis = axis / vnorm(axis)
sin_angle = np.expand_dims(sin(angle / 2), 0)
if np.rank(n_axis) == 1:
n_axis = np.expand_dims(n_axis, 1)
p__ = np.dot(n_axis, sin_angle)[:, np.newaxis]
else:
p__ = n_axis * sin_angle
q__ = Quaternion(cos(angle / 2), p__)
return np.einsum("kj, ikj->ij",
vector,
q__.rotation_matrix()[:3, :3])
# DIRTY STUFF. Needed the get_lonlatalt function to work on pos directly if
# we want to print out lonlats in the end.
from pyorbital import astronomy
from pyorbital.orbital import *
def get_lonlatalt(pos, utc_time):
"""Calculate sublon, sublat and altitude of satellite, considering the
earth an ellipsoid.
http://celestrak.com/columns/v02n03/
"""
(pos_x, pos_y, pos_z) = pos / XKMPER
lon = ((np.arctan2(pos_y * XKMPER, pos_x * XKMPER) - astronomy.gmst(utc_time))
% (2 * np.pi))
lon = np.where(lon > np.pi, lon - np.pi * 2, lon)
lon = np.where(lon <= -np.pi, lon + np.pi * 2, lon)
r = np.sqrt(pos_x ** 2 + pos_y ** 2)
lat = np.arctan2(pos_z, r)
e2 = F * (2 - F)
while True:
lat2 = lat
c = 1 / (np.sqrt(1 - e2 * (np.sin(lat2) ** 2)))
lat = np.arctan2(pos_z + c * e2 * np.sin(lat2), r)
if np.all(abs(lat - lat2) < 1e-10):
break
alt = r / np.cos(lat) - c
alt *= A
return np.rad2deg(lon), np.rad2deg(lat), alt
# END OF DIRTY STUFF
def compute_pixels((tle1, tle2), sgeom, times, rpy=(0.0, 0.0, 0.0)):
"""Compute cartesian coordinates of the pixels in instrument scan.
"""
orb = Orbital("mysatellite", line1=tle1, line2=tle2)
# get position and velocity for each time of each pixel
pos, vel = orb.get_position(times, normalize=False)
# now, get the vectors pointing to each pixel
vectors = sgeom.vectors(pos, vel, *rpy)
# compute intersection of lines (directed by vectors and passing through
# (0, 0, 0)) and ellipsoid. Derived from:
# http://en.wikipedia.org/wiki/Line%E2%80%93sphere_intersection
# do the computation between line and ellipsoid (WGS 84)
# NB: AAPP uses GRS 80...
centre = -pos
a__ = 6378.137 # km
# b__ = 6356.75231414 # km, GRS80
b__ = 6356.752314245 # km, WGS84
radius = np.array([[1 / a__, 1 / a__, 1 / b__]]).T
xr_ = vectors * radius
cr_ = centre * radius
ldotc = np.einsum("ij,ij->j", xr_, cr_)
lsq = np.einsum("ij,ij->j", xr_, xr_)
csq = np.einsum("ij,ij->j", cr_, cr_)
d1_ = (ldotc - np.sqrt(ldotc ** 2 - csq * lsq + lsq)) / lsq
# return the actual pixel positions
return vectors * d1_ - centre
def norm(v):
return np.sqrt(np.dot(v, v.conj()))
def mnorm(m, axis=None):
"""norm of a matrix of vectors stacked along the *axis* dimension.
"""
if axis is None:
axis = np.rank(m) - 1
return np.sqrt((m**2).sum(axis))
def vnorm(m):
"""norms of a matrix of column vectors.
"""
return np.sqrt((m**2).sum(0))
def hnorm(m):
"""norms of a matrix of row vectors.
"""
return np.sqrt((m**2).sum(1))
if __name__ == '__main__':
# NOAA 18 (from the 2011-10-12, 16:55 utc)
# 1 28654U 05018A 11284.35271227 .00000478 00000-0 28778-3 0 9246
# 2 28654 99.0096 235.8581 0014859 135.4286 224.8087 14.11526826329313
noaa18_tle1 = "1 28654U 05018A 11284.35271227 .00000478 00000-0 28778-3 0 9246"
noaa18_tle2 = "2 28654 99.0096 235.8581 0014859 135.4286 224.8087 14.11526826329313"
from datetime import datetime
t = datetime(2011, 10, 12, 13, 45)
# edge and centre of an avhrr scanline
# sgeom = ScanGeometry([(-0.9664123687741623, 0),
# (0, 0)],
# [0, 0.0, ])
# print compute_pixels((noaa18_tle1, noaa18_tle2), sgeom, t)
# avhrr swath
scanline_nb = 1
# building the avhrr angles, 2048 pixels from +55.37 to -55.37 degrees
avhrr = np.vstack(((np.arange(2048) - 1023.5) / 1024 * np.deg2rad(-55.37),
np.zeros((2048,)))).transpose()
avhrr = np.tile(avhrr, [scanline_nb, 1])
# building the corresponding times array
offset = np.arange(scanline_nb) * 0.1667
times = (np.tile(np.arange(2048) * 0.000025 + 0.0025415, [scanline_nb, 1])
+ np.expand_dims(offset, 1))
# build the scan geometry object
sgeom = ScanGeometry(avhrr, times.ravel())
# print the lonlats for the pixel positions
s_times = sgeom.times(t)
pixels_pos = compute_pixels((noaa18_tle1, noaa18_tle2), sgeom, s_times)
print get_lonlatalt(pixels_pos, s_times)
pyorbital-1.0.0/pyorbital/geoloc_example.py 0000664 0000000 0000000 00000005264 12567135624 0021101 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2013 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Simple usage for geoloc.
"""
import numpy as np
from datetime import datetime
from pyorbital.geoloc import ScanGeometry, compute_pixels, get_lonlatalt
tle1 = "1 33591U 09005A 12345.45213434 .00000391 00000-0 24004-3 0 6113"
tle2 = "2 33591 098.8821 283.2036 0013384 242.4835 117.4960 14.11432063197875"
t = datetime(2012, 12, 12, 4, 16, 1, 575000)
scanline_nb = 351
# we take only every 40th point for plotting clarity
scan_points = np.arange(24, 2048, 40)
# build the avhrr instrument (scan angles)
avhrr = np.vstack(((scan_points - 1023.5) / 1024 * np.deg2rad(-55.37),
np.zeros((len(scan_points),)))).transpose()
avhrr = np.tile(avhrr, [scanline_nb, 1])
# building the corresponding times array
offset = np.arange(scanline_nb) * 0.1666667
times = (np.tile(scan_points * 0.000025 + 0.0025415, [scanline_nb, 1])
+ np.expand_dims(offset, 1))
# build the scan geometry object
sgeom = ScanGeometry(avhrr, times.ravel())
# roll, pitch, yaw in radians
rpy = (0, 0, 0)
# print the lonlats for the pixel positions
s_times = sgeom.times(t)
pixels_pos = compute_pixels((tle1, tle2), sgeom, s_times, rpy)
pos_time = get_lonlatalt(pixels_pos, s_times)
print pos_time
# Plot the result
from mpl_toolkits.basemap import Basemap
import matplotlib.pyplot as plt
m = Basemap(projection='stere', llcrnrlat=24, urcrnrlat=70, llcrnrlon=-25, urcrnrlon=120, lat_ts=58, lat_0=58, lon_0=14, resolution='l')
# convert and plot the predicted pixels in red
x, y = m(pos_time[0], pos_time[1])
p1 = m.plot(x,y, marker='+', color='red', markerfacecolor='red', markeredgecolor='red', markersize=1, markevery=1, zorder=4, linewidth=0.0)
m.fillcontinents(color='0.85', lake_color=None, zorder=3)
m.drawparallels(np.arange(-90.,90.,5.), labels=[1,0,1,0],fontsize=10, dashes=[1, 0], color=[0.8,0.8,0.8], zorder=1)
m.drawmeridians(np.arange(-180.,180.,5.), labels=[0,1,0,1],fontsize=10, dashes=[1, 0], color=[0.8,0.8,0.8], zorder=2)
plt.show()
pyorbital-1.0.0/pyorbital/geoloc_instrument_definitions.py 0000664 0000000 0000000 00000016347 12567135624 0024255 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2013, 2014, 2015 Martin Raspaud
# Author(s):
# Martin Raspaud
# Mikhail Itkin
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Some instrument definitions to use with geoloc.
To define an instrument, one must first define the scan angles (in radians)
around x (along-track vector) and y (cross-track vector). the y scan angles are
just 0 in the case of scanline based instruments (like avhrr), but can be
different if the instrument is forward and/or backward scanning (e.g. viirs or
modis).
For the instrument to be defined completely, one must also provide the
observation times (in seconds, respective to the nominal scan time) for the
different pixels.
Both scan angles and scan times are then combined into a ScanGeometry object.
"""
import numpy as np
from pyorbital.geoloc import ScanGeometry
################################################################
#
# AVHRR
#
################################################################
def avhrr(scans_nb, scan_points,
scan_angle=55.37, frequency=1 / 6.0):
"""Definition of the avhrr instrument.
Source: NOAA KLM User's Guide, Appendix J
http://www.ncdc.noaa.gov/oa/pod-guide/ncdc/docs/klm/html/j/app-j.htm
"""
# build the avhrr instrument (scan angles)
avhrr_inst = np.vstack(((scan_points / 1023.5 - 1)
* np.deg2rad(-scan_angle),
np.zeros((len(scan_points),)))).transpose()
avhrr_inst = np.tile(avhrr_inst, [scans_nb, 1])
# building the corresponding times array
offset = np.arange(scans_nb) * frequency
# times = (np.tile(scan_points * 0.000025 + 0.0025415, [scans_nb, 1])
# + np.expand_dims(offset, 1))
times = (np.tile(scan_points * 0.000025, [scans_nb, 1])
+ np.expand_dims(offset, 1))
return ScanGeometry(avhrr_inst, times.ravel())
def avhrr_gac(scan_times, scan_points,
scan_angle=55.37, frequency=0.5):
"""Definition of the avhrr instrument, gac version
Source: NOAA KLM User's Guide, Appendix J
http://www.ncdc.noaa.gov/oa/pod-guide/ncdc/docs/klm/html/j/app-j.htm
"""
try:
offset = np.array([(t - scan_times[0]).seconds +
(t - scan_times[0]).microseconds / 1000000.0 for t in scan_times])
except TypeError:
offset = np.arange(scan_times) * frequency
scans_nb = len(offset)
# build the avhrr instrument (scan angles)
avhrr_inst = np.vstack(((scan_points / 1023.5 - 1)
* np.deg2rad(-scan_angle),
np.zeros((len(scan_points),)))).transpose()
avhrr_inst = np.tile(avhrr_inst, [scans_nb, 1])
# building the corresponding times array
times = (np.tile(scan_points * 0.000025, [scans_nb, 1])
+ np.expand_dims(offset, 1))
return ScanGeometry(avhrr_inst, times.ravel())
################################################################
# avhrr, all pixels
# build the scan geometry object
def avhrr_all_geom(scans_nb):
# we take all pixels
scan_points = np.arange(2048)
return avhrr(scans_nb, scan_points)
################################################################
# avhrr, edge pixels
# build the scan geometry object
def avhrr_edge_geom(scans_nb):
# we take only edge pixels
scan_points = np.array([0, 2047])
return avhrr(scans_nb, scan_points)
################################################################
# avhrr, every 40th pixel from the 24th (aapp style)
# build the scan geometry object
def avhrr_40_geom(scans_nb):
# we take only every 40th pixel
scan_points = np.arange(24, 2048, 40)
return avhrr(scans_nb, scan_points)
################################################################
#
# VIIRS
#
################################################################
def viirs(scans_nb, scan_indices=slice(0, None)):
"""Describe VIIRS instrument geometry, I-band.
"""
entire_width = np.arange(6400)
scan_points = entire_width[scan_indices]
across_track = (scan_points / 3199.5 - 1) * np.deg2rad(-55.84)
y_max_angle = np.arctan2(11.87 / 2, 824.0)
along_track = np.array([-y_max_angle, 0, y_max_angle])
scan_pixels = len(scan_points)
scan = np.vstack((np.tile(across_track, scan_pixels),
np.repeat(along_track, 6400))).T
npp = np.tile(scan, [scans_nb, 1])
# from the timestamp in the filenames, a granule takes 1:25.400 to record
# (85.4 seconds) so 1.779166667 would be the duration of 1 scanline
# dividing the duration of a single scan by a width of 6400 pixels results
# in 0.0002779947917 seconds for each column of 32 pixels in the scanline
# the individual times per pixel are probably wrong, unless the scanning
# behaves the same as for AVHRR, The VIIRS sensor rotates to allow internal
# calibration before each scanline. This would imply that the scanline
# always moves in the same direction. more info @
# http://www.eoportal.org/directory/pres_NPOESSNationalPolarorbitingOperationalEnvironmentalSatelliteSystem.html
offset = np.arange(scans_nb) * 1.779166667
times = (np.tile(scan_points * 0.0002779947917, [scans_nb, scan_pixels])
+ np.expand_dims(offset, 1))
# build the scan geometry object
return ScanGeometry(npp, times.ravel())
################################################################
#
# AMSU-A
#
################################################################
def amsua(scans_nb, edges_only=False):
""" Describe AMSU-A instrument geometry
Parameters:
scans_nb | int - number of scan lines
Keywords:
* edges_only - use only edge pixels
Returns:
pyorbital.geoloc.ScanGeometry object
"""
scan_len = 30 # 30 samples per scan
scan_rate = 8 # single scan, seconds
scan_angle = -48.3 # swath, degrees
sampling_interval = 0.2 # single view, seconds
sync_time = 0.00355 # delay before the actual scan starts
if edges_only:
scan_points = np.array([0, scan_len - 1])
else:
scan_points = np.arange(0, scan_len)
# build the instrument (scan angles)
samples = np.vstack(((scan_points / (scan_len * 0.5 - 0.5) - 1)
* np.deg2rad(scan_angle),
np.zeros((len(scan_points),)))).transpose()
samples = np.tile(samples, [scans_nb, 1])
# building the corresponding times array
offset = np.arange(scans_nb) * scan_rate
times = (np.tile(scan_points * sampling_interval + sync_time, [scans_nb, 1])
+ np.expand_dims(offset, 1))
# build the scan geometry object
return ScanGeometry(samples, times.ravel())
pyorbital-1.0.0/pyorbital/orbital.py 0000664 0000000 0000000 00000070123 12567135624 0017546 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2011, 2012, 2013, 2014.
# Author(s):
# Esben S. Nielsen
# Adam Dybbroe
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Module for computing the orbital parameters of satellites.
"""
from datetime import datetime, timedelta
import numpy as np
from pyorbital import tlefile
from pyorbital import astronomy
import warnings
ECC_EPS = 1.0e-6 # Too low for computing further drops.
ECC_LIMIT_LOW = -1.0e-3
ECC_LIMIT_HIGH = 1.0 - ECC_EPS # Too close to 1
ECC_ALL = 1.0e-4
EPS_COS = 1.5e-12
NR_EPS = 1.0e-12
CK2 = 5.413080e-4
CK4 = 0.62098875e-6
E6A = 1.0e-6
QOMS2T = 1.88027916e-9
S = 1.01222928
S0 = 78.0
XJ3 = -0.253881e-5
XKE = 0.743669161e-1
XKMPER = 6378.135
XMNPDA = 1440.0
#MFACTOR = 7.292115E-5
AE = 1.0
SECDAY = 8.6400E4
F = 1 / 298.257223563 # Earth flattening WGS-84
A = 6378.137 # WGS84 Equatorial radius
SGDP4_ZERO_ECC = 0
SGDP4_DEEP_NORM = 1
SGDP4_NEAR_SIMP = 2
SGDP4_NEAR_NORM = 3
KS = AE * (1.0 + S0 / XKMPER)
A3OVK2 = (-XJ3 / CK2) * AE**3
class OrbitalError(Exception):
pass
class Orbital(object):
"""Class for orbital computations.
The *satellite* parameter is the name of the satellite to work on and is
used to retreive the right TLE data for internet or from *tle_file* in case
it is provided.
"""
def __init__(self, satellite, tle_file=None, line1=None, line2=None):
satellite = satellite.upper()
self.satellite_name = satellite
self.tle = tlefile.read(satellite, tle_file=tle_file,
line1=line1, line2=line2)
self.orbit_elements = OrbitElements(self.tle)
self._sgdp4 = _SGDP4(self.orbit_elements)
def __str__(self):
return self.satellite_name + " " + str(self.tle)
def get_last_an_time(self, utc_time):
"""Calculate time of last ascending node relative to the
specified time
"""
# Propagate backwards to ascending node
dt = timedelta(minutes=10)
t_old = utc_time
t_new = t_old - dt
pos0, vel0 = self.get_position(t_old, normalize=False)
pos1, vel1 = self.get_position(t_new, normalize=False)
while not (pos0[2] > 0 and pos1[2] < 0):
pos0, vel0 = pos1, vel1
t_old = t_new
t_new = t_old - dt
pos1, vel1 = self.get_position(t_new, normalize=False)
# Return if z within 1 km of an
if np.abs(pos0[2]) < 1:
return t_old
elif np.abs(pos1[2]) < 1:
return t_new
# Bisect to z within 1 km
while np.abs(pos1[2]) > 1:
pos0, vel0 = pos1, vel1
dt = (t_old - t_new) / 2
t_mid = t_old - dt
pos1, vel1 = self.get_position(t_mid, normalize=False)
if pos1[2] > 0:
t_old = t_mid
else:
t_new = t_mid
return t_mid
def get_position(self, utc_time, normalize=True):
"""Get the cartesian position and velocity from the satellite.
"""
kep = self._sgdp4.propagate(utc_time)
pos, vel = kep2xyz(kep)
if normalize:
pos /= XKMPER
vel /= XKMPER * XMNPDA / SECDAY
return pos, vel
def get_lonlatalt(self, utc_time):
"""Calculate sublon, sublat and altitude of satellite.
http://celestrak.com/columns/v02n03/
"""
(pos_x, pos_y, pos_z), (vel_x, vel_y, vel_z) = self.get_position(
utc_time, normalize=True)
lon = ((np.arctan2(pos_y * XKMPER, pos_x * XKMPER) - astronomy.gmst(utc_time))
% (2 * np.pi))
lon = np.where(lon > np.pi, lon - np.pi * 2, lon)
lon = np.where(lon <= -np.pi, lon + np.pi * 2, lon)
r = np.sqrt(pos_x ** 2 + pos_y ** 2)
lat = np.arctan2(pos_z, r)
e2 = F * (2 - F)
while True:
lat2 = lat
c = 1 / (np.sqrt(1 - e2 * (np.sin(lat2) ** 2)))
lat = np.arctan2(pos_z + c * e2 * np.sin(lat2), r)
if np.all(abs(lat - lat2) < 1e-10):
break
alt = r / np.cos(lat) - c
alt *= A
return np.rad2deg(lon), np.rad2deg(lat), alt
def find_aos(self, utc_time, lon, lat):
pass
def find_aol(self, utc_time, lon, lat):
pass
def get_observer_look(self, utc_time, lon, lat, alt):
"""Calculate observers look angle to a satellite.
http://celestrak.com/columns/v02n02/
utc_time: Observation time (datetime object)
lon: Longitude of observer position on ground
lat: Latitude of observer position on ground
alt: Altitude above sea-level (geoid) of observer position on ground
Return: (Azimuth, Elevation)
"""
(pos_x, pos_y, pos_z), (vel_x, vel_y, vel_z) = self.get_position(
utc_time, normalize=False)
(opos_x, opos_y, opos_z), (ovel_x, ovel_y, ovel_z) = \
astronomy.observer_position(utc_time, lon, lat, alt)
lon = np.deg2rad(lon)
lat = np.deg2rad(lat)
theta = (astronomy.gmst(utc_time) + lon) % (2 * np.pi)
rx = pos_x - opos_x
ry = pos_y - opos_y
rz = pos_z - opos_z
sin_lat = np.sin(lat)
cos_lat = np.cos(lat)
sin_theta = np.sin(theta)
cos_theta = np.cos(theta)
top_s = sin_lat * cos_theta * rx + \
sin_lat * sin_theta * ry - cos_lat * rz
top_e = -sin_theta * rx + cos_theta * ry
top_z = cos_lat * cos_theta * rx + \
cos_lat * sin_theta * ry + sin_lat * rz
az_ = np.arctan(-top_e / top_s)
az_ = np.where(top_s > 0, az_ + np.pi, az_)
az_ = np.where(az_ < 0, az_ + 2 * np.pi, az_)
rg_ = np.sqrt(rx * rx + ry * ry + rz * rz)
el_ = np.arcsin(top_z / rg_)
return np.rad2deg(az_), np.rad2deg(el_)
def get_orbit_number(self, utc_time, tbus_style=False):
"""Calculate orbit number at specified time.
Optionally use TBUS-style orbit numbering (TLE orbit number + 1)
"""
try:
dt = astronomy._days(utc_time - self.orbit_elements.an_time)
orbit_period = astronomy._days(self.orbit_elements.an_period)
except AttributeError:
pos_epoch, vel_epoch = self.get_position(self.tle.epoch,
normalize=False)
if np.abs(pos_epoch[2]) > 1 or not vel_epoch[2] > 0:
# Epoch not at ascending node
self.orbit_elements.an_time = self.get_last_an_time(
self.tle.epoch)
else:
# Epoch at ascending node (z < 1 km) and positive v_z
self.orbit_elements.an_time = self.tle.epoch
self.orbit_elements.an_period = self.orbit_elements.an_time - \
self.get_last_an_time(self.orbit_elements.an_time
- timedelta(minutes=10))
dt = astronomy._days(utc_time - self.orbit_elements.an_time)
orbit_period = astronomy._days(self.orbit_elements.an_period)
orbit = int(self.tle.orbit + dt / orbit_period +
self.tle.mean_motion_derivative * dt**2 +
self.tle.mean_motion_sec_derivative * dt**3)
if tbus_style:
orbit += 1
return orbit
def get_next_passes(self, utc_time, length, lon, lat, alt, tol=0.001, horizon=0):
"""Calculate passes for the next hours for a given start time and a
given observer.
Original by Martin.
utc_time: Observation time (datetime object)
length: Number of hours to find passes (int)
lon: Longitude of observer position on ground (float)
lat: Latitude of observer position on ground (float)
alt: Altitude above sea-level (geoid) of observer position on ground (float)
tol: precision of the result in seconds
horizon: the elevation of horizon to compute risetime and falltime.
Return: [(rise-time, fall-time, max-elevation-time), ...]
"""
def elevation(minutes):
"""elevation
"""
return self.get_observer_look(utc_time +
timedelta(
minutes=np.float64(minutes)),
lon, lat, alt)[1] - horizon
def elevation_inv(minutes):
"""inverse of elevation
"""
return -elevation(minutes)
def get_root_secant(fun, start, end, tol=0.01):
"""Secant method
"""
x_0 = end
x_1 = start
fx_0 = fun(end)
fx_1 = fun(start)
if abs(fx_0) < abs(fx_1):
fx_0, fx_1 = fx_1, fx_0
x_0, x_1 = x_1, x_0
while abs(x_0 - x_1) > tol:
x_n = x_1 - fx_1 * ((x_1 - x_0) / (fx_1 - fx_0))
x_0, x_1 = x_1, x_n
fx_0, fx_1 = fx_1, fun(x_n)
return x_1
def get_max_parab(fun, start, end, tol=0.01):
"""Successive parabolic interpolation
"""
a = start
c = end
b = (a + c) / 2.0
x = b
f_a = fun(a)
f_b = fun(b)
f_c = fun(c)
while abs(c - a) > tol:
x = b - 0.5 * (((b - a) ** 2 * (f_b - f_c)
- (b - c) ** 2 * (f_b - f_a)) /
((b - a) * (f_b - f_c) - (b - c) * (f_b - f_a)))
f_x = fun(x)
if x > b:
a, b, c = b, x, c
f_a, f_b, f_c = f_b, f_x, f_c
else:
a, b, c = a, x, b
f_a, f_b, f_c = f_a, f_x, f_b
return x
times = utc_time + np.array([timedelta(minutes=minutes)
for minutes in range(length * 60)])
elev = self.get_observer_look(times, lon, lat, alt)[1] - horizon
zcs = np.where(np.diff(np.sign(elev)))[0]
res = []
risetime = None
falltime = None
for guess in zcs:
horizon_mins = get_root_secant(
elevation, guess, guess + 1.0, tol=tol / 60.0)
horizon_time = utc_time + timedelta(minutes=horizon_mins)
if elev[guess] < 0:
risetime = horizon_time
risemins = horizon_mins
falltime = None
else:
falltime = horizon_time
fallmins = horizon_mins
if risetime:
middle = (risemins + fallmins) / 2.0
highest = utc_time + \
timedelta(minutes=get_max_parab(
elevation_inv,
middle - 0.1, middle + 0.1,
tol=tol / 60.0
))
res += [(risetime, falltime, highest)]
risetime = None
return res
def _get_time_at_horizon(self, utc_time, obslon, obslat, **kwargs):
"""Get the time closest in time to *utc_time* when the
satellite is at the horizon relative to the position of an observer on
ground (altitude = 0)
Note: This is considered deprecated and it's functionality is currently
replaced by 'get_next_passes'.
"""
warnings.warn("_get_time_at_horizon is replaced with get_next_passes",
DeprecationWarning)
if "precision" in kwargs:
precision = kwargs['precision']
else:
precision = timedelta(seconds=0.001)
if "max_iterations" in kwargs:
nmax_iter = kwargs["max_iterations"]
else:
nmax_iter = 100
sec_step = 0.5
t_step = timedelta(seconds=sec_step / 2.0)
# Local derivative:
def fprime(timex):
el0 = self.get_observer_look(timex - t_step,
obslon, obslat, 0.0)[1]
el1 = self.get_observer_look(timex + t_step,
obslon, obslat, 0.0)[1]
return el0, (abs(el1) - abs(el0)) / sec_step
tx0 = utc_time - timedelta(seconds=1.0)
tx1 = utc_time
idx = 0
#eps = 500.
eps = 100.
while abs(tx1 - tx0) > precision and idx < nmax_iter:
tx0 = tx1
fpr = fprime(tx0)
# When the elevation is high the scale is high, and when
# the elevation is low the scale is low
#var_scale = np.abs(np.sin(fpr[0] * np.pi/180.))
#var_scale = np.sqrt(var_scale)
var_scale = np.abs(fpr[0])
tx1 = tx0 - timedelta(seconds=(eps * var_scale * fpr[1]))
idx = idx + 1
# print idx, tx0, tx1, var_scale, fpr
if abs(tx1 - utc_time) < precision and idx < 2:
tx1 = tx1 + timedelta(seconds=1.0)
if abs(tx1 - tx0) <= precision and idx < nmax_iter:
return tx1
else:
return None
class OrbitElements(object):
"""Class holding the orbital elements.
"""
def __init__(self, tle):
self.epoch = tle.epoch
self.excentricity = tle.excentricity
self.inclination = np.deg2rad(tle.inclination)
self.right_ascension = np.deg2rad(tle.right_ascension)
self.arg_perigee = np.deg2rad(tle.arg_perigee)
self.mean_anomaly = np.deg2rad(tle.mean_anomaly)
self.mean_motion = tle.mean_motion * (np.pi * 2 / XMNPDA)
self.mean_motion_derivative = tle.mean_motion_derivative * \
np.pi * 2 / XMNPDA ** 2
self.mean_motion_sec_derivative = tle.mean_motion_sec_derivative * \
np.pi * 2 / XMNPDA ** 3
self.bstar = tle.bstar * AE
n_0 = self.mean_motion
k_e = XKE
k_2 = CK2
i_0 = self.inclination
e_0 = self.excentricity
a_1 = (k_e / n_0) ** (2.0 / 3)
delta_1 = ((3 / 2.0) * (k_2 / a_1**2) * ((3 * np.cos(i_0)**2 - 1) /
(1 - e_0**2)**(2.0 / 3)))
a_0 = a_1 * (1 - delta_1 / 3 - delta_1**2 - (134.0 / 81) * delta_1**3)
delta_0 = ((3 / 2.0) * (k_2 / a_0**2) * ((3 * np.cos(i_0)**2 - 1) /
(1 - e_0**2)**(2.0 / 3)))
# original mean motion
n_0pp = n_0 / (1 + delta_0)
self.original_mean_motion = n_0pp
# semi major axis
a_0pp = a_0 / (1 - delta_0)
self.semi_major_axis = a_0pp
self.period = np.pi * 2 / n_0pp
self.perigee = (a_0pp * (1 - e_0) / AE - AE) * XKMPER
self.right_ascension_lon = (self.right_ascension
- astronomy.gmst(self.epoch))
if self.right_ascension_lon > np.pi:
self.right_ascension_lon -= 2 * np.pi
class _SGDP4(object):
"""Class for the SGDP4 computations.
"""
def __init__(self, orbit_elements):
self.mode = None
perigee = orbit_elements.perigee
self.eo = orbit_elements.excentricity
self.xincl = orbit_elements.inclination
self.xno = orbit_elements.original_mean_motion
k_2 = CK2
k_4 = CK4
k_e = XKE
self.bstar = orbit_elements.bstar
self.omegao = orbit_elements.arg_perigee
self.xmo = orbit_elements.mean_anomaly
self.xnodeo = orbit_elements.right_ascension
self.t_0 = orbit_elements.epoch
self.xn_0 = orbit_elements.mean_motion
A30 = -XJ3 * AE**3
if not(0 < self.eo < ECC_LIMIT_HIGH):
raise OrbitalError('Eccentricity out of range: %e' % self.eo)
elif not((0.0035 * 2 * np.pi / XMNPDA) < self.xn_0 < (18 * 2 * np.pi / XMNPDA)):
raise OrbitalError('Mean motion out of range: %e' % self.xn_0)
elif not(0 < self.xincl < np.pi):
raise OrbitalError('Inclination out of range: %e' % self.xincl)
if self.eo < 0:
self.mode = self.SGDP4_ZERO_ECC
return
self.cosIO = np.cos(self.xincl)
self.sinIO = np.sin(self.xincl)
theta2 = self.cosIO**2
theta4 = theta2 ** 2
self.x3thm1 = 3.0 * theta2 - 1.0
self.x1mth2 = 1.0 - theta2
self.x7thm1 = 7.0 * theta2 - 1.0
a1 = (XKE / self.xn_0) ** (2. / 3)
betao2 = 1.0 - self.eo**2
betao = np.sqrt(betao2)
temp0 = 1.5 * CK2 * self.x3thm1 / (betao * betao2)
del1 = temp0 / (a1**2)
a0 = a1 * \
(1.0 - del1 * (1.0 / 3.0 + del1 * (1.0 + del1 * 134.0 / 81.0)))
del0 = temp0 / (a0**2)
self.xnodp = self.xn_0 / (1.0 + del0)
self.aodp = (a0 / (1.0 - del0))
self.perigee = (self.aodp * (1.0 - self.eo) - AE) * XKMPER
self.apogee = (self.aodp * (1.0 + self.eo) - AE) * XKMPER
self.period = (2 * np.pi * 1440.0 / XMNPDA) / self.xnodp
if self.period >= 225:
# Deep-Space model
self.mode = SGDP4_DEEP_NORM
elif self.perigee < 220:
# Near-space, simplified equations
self.mode = SGDP4_NEAR_SIMP
else:
# Near-space, normal equations
self.mode = SGDP4_NEAR_NORM
if self.perigee < 156:
s4 = self.perigee - 78
if s4 < 20:
s4 = 20
qoms24 = ((120 - s4) * (AE / XKMPER))**4
s4 = (s4 / XKMPER + AE)
else:
s4 = KS
qoms24 = QOMS2T
pinvsq = 1.0 / (self.aodp**2 * betao2**2)
tsi = 1.0 / (self.aodp - s4)
self.eta = self.aodp * self.eo * tsi
etasq = self.eta**2
eeta = self.eo * self.eta
psisq = np.abs(1.0 - etasq)
coef = qoms24 * tsi**4
coef_1 = coef / psisq**3.5
self.c2 = (coef_1 * self.xnodp * (self.aodp *
(1.0 + 1.5 * etasq + eeta * (4.0 + etasq)) +
(0.75 * CK2) * tsi / psisq * self.x3thm1 *
(8.0 + 3.0 * etasq * (8.0 + etasq))))
self.c1 = self.bstar * self.c2
self.c4 = (2.0 * self.xnodp * coef_1 * self.aodp * betao2 * (self.eta *
(2.0 + 0.5 * etasq) + self.eo * (0.5 + 2.0 *
etasq) - (2.0 * CK2) * tsi / (self.aodp * psisq) * (-3.0 *
self.x3thm1 * (1.0 - 2.0 * eeta + etasq *
(1.5 - 0.5 * eeta)) + 0.75 * self.x1mth2 * (2.0 *
etasq - eeta * (1.0 + etasq)) * np.cos(2.0 * self.omegao))))
self.c5, self.c3, self.omgcof = 0.0, 0.0, 0.0
if self.mode == SGDP4_NEAR_NORM:
self.c5 = (2.0 * coef_1 * self.aodp * betao2 *
(1.0 + 2.75 * (etasq + eeta) + eeta * etasq))
if self.eo > ECC_ALL:
self.c3 = coef * tsi * A3OVK2 * \
self.xnodp * AE * self.sinIO / self.eo
self.omgcof = self.bstar * self.c3 * np.cos(self.omegao)
temp1 = 3.0 * CK2 * pinvsq * self.xnodp
temp2 = temp1 * CK2 * pinvsq
temp3 = 1.25 * CK4 * pinvsq**2 * self.xnodp
self.xmdot = (self.xnodp + (0.5 * temp1 * betao * self.x3thm1 + 0.0625 *
temp2 * betao * (13.0 - 78.0 * theta2 +
137.0 * theta4)))
x1m5th = 1.0 - 5.0 * theta2
self.omgdot = (-0.5 * temp1 * x1m5th + 0.0625 * temp2 *
(7.0 - 114.0 * theta2 + 395.0 * theta4) +
temp3 * (3.0 - 36.0 * theta2 + 49.0 * theta4))
xhdot1 = -temp1 * self.cosIO
self.xnodot = (xhdot1 + (0.5 * temp2 * (4.0 - 19.0 * theta2) +
2.0 * temp3 * (3.0 - 7.0 * theta2)) * self.cosIO)
if self.eo > ECC_ALL:
self.xmcof = (-(2. / 3) * AE) * coef * self.bstar / eeta
else:
self.xmcof = 0.0
self.xnodcf = 3.5 * betao2 * xhdot1 * self.c1
self.t2cof = 1.5 * self.c1
# Check for possible divide-by-zero for X/(1+cos(xincl)) when
# calculating xlcof */
temp0 = 1.0 + self.cosIO
if np.abs(temp0) < EPS_COS:
temp0 = np.sign(temp0) * EPS_COS
self.xlcof = 0.125 * A3OVK2 * self.sinIO * \
(3.0 + 5.0 * self.cosIO) / temp0
self.aycof = 0.25 * A3OVK2 * self.sinIO
self.cosXMO = np.cos(self.xmo)
self.sinXMO = np.sin(self.xmo)
self.delmo = (1.0 + self.eta * self.cosXMO)**3
if self.mode == SGDP4_NEAR_NORM:
c1sq = self.c1**2
self.d2 = 4.0 * self.aodp * tsi * c1sq
temp0 = self.d2 * tsi * self.c1 / 3.0
self.d3 = (17.0 * self.aodp + s4) * temp0
self.d4 = 0.5 * temp0 * self.aodp * tsi * \
(221.0 * self.aodp + 31.0 * s4) * self.c1
self.t3cof = self.d2 + 2.0 * c1sq
self.t4cof = 0.25 * \
(3.0 * self.d3 + self.c1 * (12.0 * self.d2 + 10.0 * c1sq))
self.t5cof = (0.2 * (3.0 * self.d4 + 12.0 * self.c1 * self.d3 + 6.0 * self.d2**2 +
15.0 * c1sq * (2.0 * self.d2 + c1sq)))
elif self.mode == SGDP4_DEEP_NORM:
raise NotImplementedError('Deep space calculations not supported')
def propagate(self, utc_time):
kep = {}
ts = astronomy._days(utc_time - self.t_0) * XMNPDA
em = self.eo
xinc = self.xincl
xmp = self.xmo + self.xmdot * ts
xnode = self.xnodeo + ts * (self.xnodot + ts * self.xnodcf)
omega = self.omegao + self.omgdot * ts
if self.mode == SGDP4_ZERO_ECC:
raise NotImplementedError('Mode SGDP4_ZERO_ECC not implemented')
elif self.mode == SGDP4_NEAR_SIMP:
raise NotImplementedError('Mode "Near-space, simplified equations"'
' not implemented')
elif self.mode == SGDP4_NEAR_NORM:
delm = self.xmcof * \
((1.0 + self.eta * np.cos(xmp))**3 - self.delmo)
temp0 = ts * self.omgcof + delm
xmp += temp0
omega -= temp0
tempa = 1.0 - \
(ts *
(self.c1 + ts * (self.d2 + ts * (self.d3 + ts * self.d4))))
tempe = self.bstar * \
(self.c4 * ts + self.c5 * (np.sin(xmp) - self.sinXMO))
templ = ts * ts * \
(self.t2cof + ts *
(self.t3cof + ts * (self.t4cof + ts * self.t5cof)))
a = self.aodp * tempa**2
e = em - tempe
xl = xmp + omega + xnode + self.xnodp * templ
else:
raise NotImplementedError('Deep space calculations not supported')
if np.any(a < 1):
raise Exception('Satellite crased at time %s', utc_time)
elif np.any(e < ECC_LIMIT_LOW):
raise ValueError('Satellite modified eccentricity to low: %s < %e'
% (str(e[e < ECC_LIMIT_LOW]), ECC_LIMIT_LOW))
e = np.where(e < ECC_EPS, ECC_EPS, e)
e = np.where(e > ECC_LIMIT_HIGH, ECC_LIMIT_HIGH, e)
beta2 = 1.0 - e**2
# Long period periodics
sinOMG = np.sin(omega)
cosOMG = np.cos(omega)
temp0 = 1.0 / (a * beta2)
axn = e * cosOMG
ayn = e * sinOMG + temp0 * self.aycof
xlt = xl + temp0 * self.xlcof * axn
elsq = axn**2 + ayn**2
if np.any(elsq >= 1):
raise Exception('e**2 >= 1 at %s', utc_time)
kep['ecc'] = np.sqrt(elsq)
epw = np.fmod(xlt - xnode, 2 * np.pi)
# needs a copy in case of an array
capu = np.array(epw)
maxnr = kep['ecc']
for i in range(10):
sinEPW = np.sin(epw)
cosEPW = np.cos(epw)
ecosE = axn * cosEPW + ayn * sinEPW
esinE = axn * sinEPW - ayn * cosEPW
f = capu - epw + esinE
if np.all(np.abs(f) < NR_EPS):
break
df = 1.0 - ecosE
# 1st order Newton-Raphson correction.
nr = f / df
# 2nd order Newton-Raphson correction.
nr = np.where(np.logical_and(i == 0, np.abs(nr) > 1.25 * maxnr),
np.sign(nr) * maxnr,
f / (df + 0.5 * esinE * nr))
epw += nr
# Short period preliminary quantities
temp0 = 1.0 - elsq
betal = np.sqrt(temp0)
pl = a * temp0
r = a * (1.0 - ecosE)
invR = 1.0 / r
temp2 = a * invR
temp3 = 1.0 / (1.0 + betal)
cosu = temp2 * (cosEPW - axn + ayn * esinE * temp3)
sinu = temp2 * (sinEPW - ayn - axn * esinE * temp3)
u = np.arctan2(sinu, cosu)
sin2u = 2.0 * sinu * cosu
cos2u = 2.0 * cosu**2 - 1.0
temp0 = 1.0 / pl
temp1 = CK2 * temp0
temp2 = temp1 * temp0
# Update for short term periodics to position terms.
rk = r * (1.0 - 1.5 * temp2 * betal * self.x3thm1) + \
0.5 * temp1 * self.x1mth2 * cos2u
uk = u - 0.25 * temp2 * self.x7thm1 * sin2u
xnodek = xnode + 1.5 * temp2 * self.cosIO * sin2u
xinck = xinc + 1.5 * temp2 * self.cosIO * self.sinIO * cos2u
if np.any(rk < 1):
raise Exception('Satellite crased at time %s', utc_time)
temp0 = np.sqrt(a)
temp2 = XKE / (a * temp0)
rdotk = ((XKE * temp0 * esinE * invR - temp2 * temp1 * self.x1mth2 * sin2u) *
(XKMPER / AE * XMNPDA / 86400.0))
rfdotk = ((XKE * np.sqrt(pl) * invR + temp2 * temp1 *
(self.x1mth2 * cos2u + 1.5 * self.x3thm1)) *
(XKMPER / AE * XMNPDA / 86400.0))
kep['radius'] = rk * XKMPER / AE
kep['theta'] = uk
kep['eqinc'] = xinck
kep['ascn'] = xnodek
kep['argp'] = omega
kep['smjaxs'] = a * XKMPER / AE
kep['rdotk'] = rdotk
kep['rfdotk'] = rfdotk
return kep
def kep2xyz(kep):
sinT = np.sin(kep['theta'])
cosT = np.cos(kep['theta'])
sinI = np.sin(kep['eqinc'])
cosI = np.cos(kep['eqinc'])
sinS = np.sin(kep['ascn'])
cosS = np.cos(kep['ascn'])
xmx = -sinS * cosI
xmy = cosS * cosI
ux = xmx * sinT + cosS * cosT
uy = xmy * sinT + sinS * cosT
uz = sinI * sinT
x = kep['radius'] * ux
y = kep['radius'] * uy
z = kep['radius'] * uz
vx = xmx * cosT - cosS * sinT
vy = xmy * cosT - sinS * sinT
vz = sinI * cosT
v_x = kep['rdotk'] * ux + kep['rfdotk'] * vx
v_y = kep['rdotk'] * uy + kep['rfdotk'] * vy
v_z = kep['rdotk'] * uz + kep['rfdotk'] * vz
return np.array((x, y, z)), np.array((v_x, v_y, v_z))
if __name__ == "__main__":
obs_lon, obs_lat = np.deg2rad((12.4143, 55.9065))
obs_alt = 0.02
o = Orbital(satellite="METOP-B")
t_start = datetime.now()
t_stop = t_start + timedelta(minutes=20)
t = t_start
while t < t_stop:
t += timedelta(seconds=15)
lon, lat, alt = o.get_lonlatalt(t)
lon, lat = np.rad2deg((lon, lat))
az, el = o.get_observer_look(t, obs_lon, obs_lat, obs_alt)
ob = o.get_orbit_number(t, tbus_style=True)
print az, el, ob
pyorbital-1.0.0/pyorbital/tests/ 0000775 0000000 0000000 00000000000 12567135624 0016677 5 ustar 00root root 0000000 0000000 pyorbital-1.0.0/pyorbital/tests/SGP4-VER.TLE 0000664 0000000 0000000 00000020650 12567135624 0020417 0 ustar 00root root 0000000 0000000 # ------------------ Verification test cases ----------------------
# # TEME example
1 00005U 58002B 00179.78495062 .00000023 00000-0 28098-4 0 4753
2 00005 34.2682 348.7242 1859667 331.7664 19.3264 10.82419157413667 0.00 4320.0 360.00
# ## fig show lyddane fix error with gsfc ver
1 04632U 70093B 04031.91070959 -.00000084 00000-0 10000-3 0 9955
2 04632 11.4628 273.1101 1450506 207.6000 143.9350 1.20231981 44145 -5184.0 -4896.0 120.00
# DELTA 1 DEB # near earth normal drag equation
# # perigee = 377.26km, so moderate drag case
1 06251U 62025E 06176.82412014 .00008885 00000-0 12808-3 0 3985
2 06251 58.0579 54.0425 0030035 139.1568 221.1854 15.56387291 6774 0.0 2880.0 120.00
# MOLNIYA 2-14 # 12h resonant ecc in 0.65 to 0.7 range
1 08195U 75081A 06176.33215444 .00000099 00000-0 11873-3 0 813
2 08195 64.1586 279.0717 6877146 264.7651 20.2257 2.00491383225656 0.0 2880.0 120.00
# MOLNIYA 1-36 ## fig 12h resonant ecc in 0.7 to 0.715 range
1 09880U 77021A 06176.56157475 .00000421 00000-0 10000-3 0 9814
2 09880 64.5968 349.3786 7069051 270.0229 16.3320 2.00813614112380 0.0 2880.0 120.00
# SMS 1 AKM # show the integrator problem with gsfc ver
1 09998U 74033F 05148.79417928 -.00000112 00000-0 00000+0 0 4480
2 09998 9.4958 313.1750 0270971 327.5225 30.8097 1.16186785 45878 -1440.0 -720.00 60.0
# # Original STR#3 SDP4 test
1 11801U 80230.29629788 .01431103 00000-0 14311-1 13
2 11801 46.7916 230.4354 7318036 47.4722 10.4117 2.28537848 13 0.0 1440.0 360.00
# EUTELSAT 1-F1 (ECS1)## fig lyddane choice in GSFC at 2080 min
1 14128U 83058A 06176.02844893 -.00000158 00000-0 10000-3 0 9627
2 14128 11.4384 35.2134 0011562 26.4582 333.5652 0.98870114 46093 0.0 2880.0 120.00
# SL-6 R/B(2) # Deep space, perigee = 82.48 (<98) for
# # s4 > 20 mod
1 16925U 86065D 06151.67415771 .02550794 -30915-6 18784-3 0 4486
2 16925 62.0906 295.0239 5596327 245.1593 47.9690 4.88511875148616 0.0 1440.0 120.00
# SL-12 R/B # Shows Lyddane choice at 1860 and 4700 min
1 20413U 83020D 05363.79166667 .00000000 00000-0 00000+0 0 7041
2 20413 12.3514 187.4253 7864447 196.3027 356.5478 0.24690082 7978 1440.0 4320.0 120.00
# MOLNIYA 1-83 # 12h resonant, ecc > 0.715 (negative BSTAR)
1 21897U 92011A 06176.02341244 -.00001273 00000-0 -13525-3 0 3044
2 21897 62.1749 198.0096 7421690 253.0462 20.1561 2.01269994104880 0.0 2880.0 120.00
# SL-6 R/B(2) # last tle given, decayed 2006-04-04, day 94
1 22312U 93002D 06094.46235912 .99999999 81888-5 49949-3 0 3953
2 22312 62.1486 77.4698 0308723 267.9229 88.7392 15.95744531 98783 54.2028672 1440.0 20.00
# SL-6 R/B(2) # 12h resonant ecc in the > 0.715 range
1 22674U 93035D 06176.55909107 .00002121 00000-0 29868-3 0 6569
2 22674 63.5035 354.4452 7541712 253.3264 18.7754 1.96679808 93877 0.0 2880.0 120.00
# ARIANE 44L+ R/B # Lyddane bug at <= 70 min for atan2(),
# # no quadrant fix
1 23177U 94040C 06175.45752052 .00000386 00000-0 76590-3 0 95
2 23177 7.0496 179.8238 7258491 296.0482 8.3061 2.25906668 97438 0.0 1440.0 120.00
# WIND # STR#3 Kepler failes past about 200 min
1 23333U 94071A 94305.49999999 -.00172956 26967-3 10000-3 0 15
2 23333 28.7490 2.3720 9728298 30.4360 1.3500 0.07309491 70 0.0 1600.0 120.00
# ARIANE 42P+3 R/B ## fig Lyddane bug at > 280.5 min for AcTan()
1 23599U 95029B 06171.76535463 .00085586 12891-6 12956-2 0 2905
2 23599 6.9327 0.2849 5782022 274.4436 25.2425 4.47796565123555 0.0 720.0 20.00
# ITALSAT 2 # 24h resonant GEO, inclination > 3 deg
1 24208U 96044A 06177.04061740 -.00000094 00000-0 10000-3 0 1600
2 24208 3.8536 80.0121 0026640 311.0977 48.3000 1.00778054 36119 0.0 1440.0 120.00
# AMC-4 ## fig low incl, show incl shift with
# ## gsfc version from 240 to 1440 min
1 25954U 99060A 04039.68057285 -.00000108 00000-0 00000-0 0 6847
2 25954 0.0004 243.8136 0001765 15.5294 22.7134 1.00271289 15615 -1440.0 1440.0 120.00
# INTELSAT 902 # negative incl at 9313 min then
# # 270 deg Lyddane bug at 37606 min
1 26900U 01039A 06106.74503247 .00000045 00000-0 10000-3 0 8290
2 26900 0.0164 266.5378 0003319 86.1794 182.2590 1.00273847 16981 9300.00 9400.00 60.00
# COSMOS 1024 DEB # 12h resonant ecc in 0.5 to 0.65 range
1 26975U 78066F 06174.85818871 .00000620 00000-0 10000-3 0 6809
2 26975 68.4714 236.1303 5602877 123.7484 302.5767 2.05657553 67521 0.0 2880.0 120.00
# CBERS 2 # Near Earth, ecc = 8.84E-5 (< 1.0e-4)
# # drop certain normal drag terms
1 28057U 03049A 06177.78615833 .00000060 00000-0 35940-4 0 1836
2 28057 98.4283 247.6961 0000884 88.1964 271.9322 14.35478080140550 0.0 2880.0 120.00
# NAVSTAR 53 (USA 175)# 12h non-resonant GPS (ecc < 0.5 ecc)
1 28129U 03058A 06175.57071136 -.00000104 00000-0 10000-3 0 459
2 28129 54.7298 324.8098 0048506 266.2640 93.1663 2.00562768 18443 0.0 1440.0 120.00
# COSMOS 2405 # Near Earth, perigee = 127.20 (< 156) s4 mod
1 28350U 04020A 06167.21788666 .16154492 76267-5 18678-3 0 8894
2 28350 64.9977 345.6130 0024870 260.7578 99.9590 16.47856722116490 0.0 2880.0 120.00
# H-2 R/B # Deep space, perigee = 135.75 (<156) s4 mod
1 28623U 05006B 06177.81079184 .00637644 69054-6 96390-3 0 6000
2 28623 28.5200 114.9834 6249053 170.2550 212.8965 3.79477162 12753 0.0 1440.0 120.00
# XM-3 # 24h resonant geo, incl < 3 deg goes
# # negative around 1130 min
1 28626U 05008A 06176.46683397 -.00000205 00000-0 10000-3 0 2190
2 28626 0.0019 286.9433 0000335 13.7918 55.6504 1.00270176 4891 0.0 1440.0 120.00
# MINOTAUR R/B # Sub-orbital case - Decayed 2005-11-29
# #(perigee = -51km), lost in 50 minutes
1 28872U 05037B 05333.02012661 .25992681 00000-0 24476-3 0 1534
2 28872 96.4736 157.9986 0303955 244.0492 110.6523 16.46015938 10708 0.0 60.0 5.00
# SL-14 DEB # Last stage of decay - lost in under 420 min
1 29141U 85108AA 06170.26783845 .99999999 00000-0 13519-0 0 718
2 29141 82.4288 273.4882 0015848 277.2124 83.9133 15.93343074 6828 0.0 440.0 20.00
# SL-12 DEB # Near Earth, perigee = 212.24 < 220
# # simplified drag eq
1 29238U 06022G 06177.28732010 .00766286 10823-4 13334-2 0 101
2 29238 51.5595 213.7903 0202579 95.2503 267.9010 15.73823839 1061 0.0 1440.0 120.00
# # Original STR#3 SGP4 test
1 88888U 80275.98708465 .00073094 13844-3 66816-4 0 87
2 88888 72.8435 115.9689 0086731 52.6988 110.5714 16.05824518 1058 0.0 1440.0 120.00
#
# # check error code 4
1 33333U 05037B 05333.02012661 .25992681 00000-0 24476-3 0 1534
2 33333 96.4736 157.9986 9950000 244.0492 110.6523 4.00004038 10708 0.0 150.0 5.00
# # try and check error code 2 but this
1 33334U 78066F 06174.85818871 .00000620 00000-0 10000-3 0 6809
2 33334 68.4714 236.1303 5602877 123.7484 302.5767 0.00001000 67521 0.0 1440.0 1.00
# # try to check error code 3 looks like ep never goes below zero, tied close to ecc
1 33335U 05008A 06176.46683397 -.00000205 00000-0 10000-3 0 2190
2 33335 0.0019 286.9433 0000004 13.7918 55.6504 1.00270176 4891 0.0 1440.0 20.00
# SL-12 R/B # Shows Lyddane choice at 1860 and 4700 min
1 20413U 83020D 05363.79166667 .00000000 00000-0 00000+0 0 7041
2 20413 12.3514 187.4253 7864447 196.3027 356.5478 0.24690082 7978 1844000 1845100 5.00
pyorbital-1.0.0/pyorbital/tests/__init__.py 0000664 0000000 0000000 00000002674 12567135624 0021021 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2014 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""The tests package.
"""
from pyorbital.tests import (test_aiaa, test_tlefile, test_orbital,
test_astronomy, test_geoloc)
import unittest
def suite():
"""The global test suite.
"""
mysuite = unittest.TestSuite()
# Test the documentation strings
#mysuite.addTests(doctest.DocTestSuite(image))
# Use the unittests also
mysuite.addTests(test_aiaa.suite())
mysuite.addTests(test_tlefile.suite())
mysuite.addTests(test_orbital.suite())
mysuite.addTests(test_astronomy.suite())
mysuite.addTests(test_geoloc.suite())
return mysuite
if __name__ == '__main__':
unittest.TextTestRunner(verbosity=2).run(suite())
pyorbital-1.0.0/pyorbital/tests/aiaa_results 0000664 0000000 0000000 00000171044 12567135624 0021305 0 ustar 00root root 0000000 0000000 # Min from epoch position x km position y km position z km vel km/s vel km/s vel km/s year mon day hr min sec
5 xx
0.00000000 7022.46529266 -1400.08296755 0.03995155 1.893841015 6.405893759 4.534807250
360.00000000 -7154.03120202 -3783.17682504 -3536.19412294 4.741887409 -4.151817765 -2.093935425 2000 6 28 0:50:19.733571
720.00000000 -7134.59340119 6531.68641334 3260.27186483 -4.113793027 -2.911922039 -2.557327851 2000 6 28 6:50:19.733571
1080.00000000 5568.53901181 4492.06992591 3863.87641983 -4.209106476 5.159719888 2.744852980 2000 6 28 12:50:19.733571
1440.00000000 -938.55923943 -6268.18748831 -4294.02924751 7.536105209 -0.427127707 0.989878080 2000 6 28 18:50:19.733571
1800.00000000 -9680.56121728 2802.47771354 124.10688038 -0.905874102 -4.659467970 -3.227347517 2000 6 29 0:50:19.733571
2160.00000000 190.19796988 7746.96653614 5110.00675412 -6.112325142 1.527008184 -0.139152358 2000 6 29 6:50:19.733571
2520.00000000 5579.55640116 -3995.61396789 -1518.82108966 4.767927483 5.123185301 4.276837355 2000 6 29 12:50:19.733571
2880.00000000 -8650.73082219 -1914.93811525 -3007.03603443 3.067165127 -4.828384068 -2.515322836 2000 6 29 18:50:19.733571
3240.00000000 -5429.79204164 7574.36493792 3747.39305236 -4.999442110 -1.800561422 -2.229392830 2000 6 30 0:50:19.733571
3600.00000000 6759.04583722 2001.58198220 2783.55192533 -2.180993947 6.402085603 3.644723952 2000 6 30 6:50:19.733571
3960.00000000 -3791.44531559 -5712.95617894 -4533.48630714 6.668817493 -2.516382327 -0.082384354 2000 6 30 12:50:19.733571
4320.00000000 -9060.47373569 4658.70952502 813.68673153 -2.232832783 -4.110453490 -3.157345433 2000 6 30 18:50:19.733571
4632 xx
0.00000000 2334.11450085 -41920.44035349 -0.03867437 2.826321032 -0.065091664 0.570936053
-5184.00000000 -29020.02587128 13819.84419063 -5713.33679183 -1.768068390 -3.235371192 -0.395206135 2004 1 28 7:27:25.308584
-5064.00000000 -32982.56870101 -11125.54996609 -6803.28472771 0.617446996 -3.379240041 0.085954707 2004 1 28 9:27:25.308597
-4944.00000000 -22097.68730513 -31583.13829284 -4836.34329328 2.230597499 -2.166594667 0.426443070 2004 1 28 11:27:25.308611
-4896.00000000 -15129.94694545 -36907.74526221 -3487.56256701 2.581167187 -1.524204737 0.504805763 2004 1 28 12:15:25.308600
6251 xx
0.00000000 3988.31022699 5498.96657235 0.90055879 -3.290032738 2.357652820 6.496623475
120.00000000 -3935.69800083 409.10980837 5471.33577327 -3.374784183 -6.635211043 -1.942056221 2006 6 25 21:46:43.980124
240.00000000 -1675.12766915 -5683.30432352 -3286.21510937 5.282496925 1.508674259 -5.354872978 2006 6 25 23:46:43.980097
360.00000000 4993.62642836 2890.54969900 -3600.40145627 0.347333429 5.707031557 5.070699638 2006 6 26 1:46:43.980111
480.00000000 -1115.07959514 4015.11691491 5326.99727718 -5.524279443 -4.765738774 2.402255961 2006 6 26 3:46:43.980124
600.00000000 -4329.10008198 -5176.70287935 409.65313857 2.858408303 -2.933091792 -6.509690397 2006 6 26 5:46:43.980097
720.00000000 3692.60030028 -976.24265255 -5623.36447493 3.897257243 6.415554948 1.429112190 2006 6 26 7:46:43.980111
840.00000000 2301.83510037 5723.92394553 2814.61514580 -5.110924966 -0.764510559 5.662120145 2006 6 26 9:46:43.980124
960.00000000 -4990.91637950 -2303.42547880 3920.86335598 -0.993439372 -5.967458360 -4.759110856 2006 6 26 11:46:43.980097
1080.00000000 642.27769977 -4332.89821901 -5183.31523910 5.720542579 4.216573838 -2.846576139 2006 6 26 13:46:43.980111
1200.00000000 4719.78335752 4798.06938996 -943.58851062 -2.294860662 3.492499389 6.408334723 2006 6 26 15:46:43.980124
1320.00000000 -3299.16993602 1576.83168320 5678.67840638 -4.460347074 -6.202025196 -0.885874586 2006 6 26 17:46:43.980097
1440.00000000 -2777.14682335 -5663.16031708 -2462.54889123 4.915493146 0.123328992 -5.896495091 2006 6 26 19:46:43.980111
1560.00000000 4992.31573893 1716.62356770 -4287.86065581 1.640717189 6.071570434 4.338797931 2006 6 26 21:46:43.980124
1680.00000000 -8.22384755 4662.21521668 4905.66411857 -5.891011274 -3.593173872 3.365100460 2006 6 26 23:46:43.980097
1800.00000000 -4966.20137963 -4379.59155037 1349.33347502 1.763172581 -3.981456387 -6.343279443 2006 6 27 1:46:43.980111
1920.00000000 2954.49390331 -2080.65984650 -5754.75038057 4.895893306 5.858184322 0.375474825 2006 6 27 3:46:43.980124
2040.00000000 3363.28794321 5559.55841180 1956.05542266 -4.587378863 0.591943403 6.107838605 2006 6 27 5:46:43.980097
2160.00000000 -4856.66780070 -1107.03450192 4557.21258241 -2.304158557 -6.186437070 -3.956549542 2006 6 27 7:46:43.980111
2280.00000000 -497.84480071 -4863.46005312 -4700.81211217 5.960065407 2.996683369 -3.767123329 2006 6 27 9:46:43.980124
2400.00000000 5241.61936096 3910.75960683 -1857.93473952 -1.124834806 4.406213160 6.148161299 2006 6 27 11:46:43.980097
2520.00000000 -2451.38045953 2610.60463261 5729.79022069 -5.366560525 -5.500855666 0.187958716 2006 6 27 13:46:43.980111
2640.00000000 -3791.87520638 -5378.82851382 -1575.82737930 4.266273592 -1.199162551 -6.276154080 2006 6 27 15:46:43.980124
2760.00000000 4730.53958356 524.05006433 -4857.29369725 2.918056288 6.135412849 3.495115636 2006 6 27 17:46:43.980097
2880.00000000 1159.27802897 5056.60175495 4353.49418579 -5.968060341 -2.314790406 4.230722669 2006 6 27 19:46:43.980111
8195 xx
0.00000000 2349.89483350 -14785.93811562 0.02119378 2.721488096 -3.256811655 4.498416672
120.00000000 15223.91713658 -17852.95881713 25280.39558224 1.079041732 0.875187372 2.485682813 2006 6 25 9:58:18.143649
240.00000000 19752.78050009 -8600.07130962 37522.72921090 0.238105279 1.546110924 0.986410447 2006 6 25 11:58:18.143622
360.00000000 19089.29762968 3107.89495018 39958.14661370 -0.410308034 1.640332277 -0.306873818 2006 6 25 13:58:18.143636
480.00000000 13829.66070574 13977.39999817 32736.32082508 -1.065096849 1.279983299 -1.760166075 2006 6 25 15:58:18.143649
600.00000000 3333.05838525 18395.31728674 12738.25031238 -1.882432221 -0.611623333 -4.039586549 2006 6 25 17:58:18.143622
720.00000000 2622.13222207 -15125.15464924 474.51048398 2.688287199 -3.078426664 4.494979530 2006 6 25 19:58:18.143636
840.00000000 15320.56770017 -17777.32564586 25539.53198382 1.064346229 0.892184771 2.459822414 2006 6 25 21:58:18.143649
960.00000000 19769.70267785 -8458.65104454 37624.20130236 0.229304396 1.550363884 0.966993056 2006 6 25 23:58:18.143622
1080.00000000 19048.56201523 3260.43223119 39923.39143967 -0.418015536 1.639346953 -0.326094840 2006 6 26 1:58:18.143636
1200.00000000 13729.19205837 14097.70014810 32547.52799890 -1.074511043 1.270505211 -1.785099927 2006 6 26 3:58:18.143649
1320.00000000 3148.86165643 18323.19841703 12305.75195578 -1.895271701 -0.678343847 -4.086577951 2006 6 26 5:58:18.143622
1440.00000000 2890.80638268 -15446.43952300 948.77010176 2.654407490 -2.909344895 4.486437362 2006 6 26 7:58:18.143636
1560.00000000 15415.98410712 -17699.90714437 25796.19644689 1.049818334 0.908822332 2.434107329 2006 6 26 9:58:18.143649
1680.00000000 19786.00618538 -8316.74570581 37723.74539119 0.220539813 1.554518900 0.947601047 2006 6 26 11:58:18.143622
1800.00000000 19007.28688729 3412.85948715 39886.66579255 -0.425733568 1.638276809 -0.345353807 2006 6 26 13:58:18.143636
1920.00000000 13627.93015254 14216.95401307 32356.13706868 -1.083991976 1.260802347 -1.810193903 2006 6 26 15:58:18.143649
2040.00000000 2963.26486560 18243.85063641 11868.25797486 -1.908015447 -0.747870342 -4.134004492 2006 6 26 17:58:18.143622
2160.00000000 3155.85126036 -15750.70393364 1422.32496953 2.620085624 -2.748990396 4.473527039 2006 6 26 19:58:18.143636
2280.00000000 15510.15191770 -17620.71002219 26050.43525345 1.035454678 0.925111006 2.408534465 2006 6 26 21:58:18.143649
2400.00000000 19801.67198812 -8174.33337167 37821.38577439 0.211812700 1.558576937 0.928231880 2006 6 26 23:58:18.143622
2520.00000000 18965.46529379 3565.19666242 39847.97510998 -0.433459945 1.637120585 -0.364653213 2006 6 27 1:58:18.143636
2640.00000000 13525.88227400 14335.15978787 32162.13236536 -1.093537945 1.250868256 -1.835451681 2006 6 27 3:58:18.143649
2760.00000000 2776.30574260 18156.98538451 11425.73046481 -1.920632199 -0.820370733 -4.181839232 2006 6 27 5:58:18.143622
2880.00000000 3417.20931587 -16038.79510665 1894.74934058 2.585515864 -2.596818146 4.456882556 2006 6 27 7:58:18.143636
9880 xx
0.00000000 13020.06750784 -2449.07193500 1.15896030 4.247363935 1.597178501 4.956708611
120.00000000 19190.32482476 9249.01266902 26596.71345328 -0.624960193 1.324550562 2.495697637 2006 6 25 15:28:40.058423
240.00000000 11332.67806218 16517.99124008 38569.78482991 -1.400974747 0.710947006 0.923935636 2006 6 25 17:28:40.058396
360.00000000 328.74217398 19554.92047380 40558.26246145 -1.593281066 0.126772913 -0.359627307 2006 6 25 19:28:40.058410
480.00000000 -10684.90590680 18057.15728839 33158.75253886 -1.383205997 -0.582328999 -1.744412556 2006 6 25 21:28:40.058423
600.00000000 -17069.78000550 9944.86797897 13885.91649059 0.044133354 -1.853448464 -3.815303117 2006 6 25 23:28:40.058396
720.00000000 13725.09398980 -2180.70877090 863.29684523 3.878478111 1.656846496 4.944867241 2006 6 26 1:28:40.058410
840.00000000 19089.63879226 9456.29670247 27026.79562883 -0.656614299 1.309112636 2.449371941 2006 6 26 3:28:40.058423
960.00000000 11106.41248373 16627.60874079 38727.35140296 -1.409722680 0.698582526 0.891383535 2006 6 26 5:28:40.058396
1080.00000000 72.40958621 19575.08054144 40492.12544001 -1.593394604 0.113655142 -0.390556063 2006 6 26 7:28:40.058410
1200.00000000 -10905.89252576 17965.41205111 32850.07298244 -1.371396120 -0.601706604 -1.782817058 2006 6 26 9:28:40.058423
1320.00000000 -17044.61207568 9635.48491849 13212.59462953 0.129244030 -1.903551430 -3.884569098 2006 6 26 11:28:40.058396
1440.00000000 14369.90303735 -1903.85601062 1722.15319853 3.543393116 1.701687176 4.913881358 2006 6 26 13:28:40.058410
1560.00000000 18983.96210441 9661.12233804 27448.99557732 -0.687189304 1.293808870 2.403630759 2006 6 26 15:28:40.058423
1680.00000000 10878.79336704 16735.31433954 38879.23434264 -1.418239666 0.686235750 0.858951848 2006 6 26 17:28:40.058396
1800.00000000 -184.03743100 19593.09371709 40420.40606889 -1.593348925 0.100448697 -0.421571993 2006 6 26 19:28:40.058410
1920.00000000 -11125.12138631 17870.19488928 32534.21521208 -1.359116236 -0.621413776 -1.821629856 2006 6 26 21:28:40.058423
2040.00000000 -17004.43272827 9316.53926351 12526.11883812 0.220330736 -1.955594322 -3.955058575 2006 6 26 23:28:40.058396
2160.00000000 14960.06492693 -1620.68430805 2574.96359381 3.238634028 1.734723385 4.868880331 2006 6 27 1:28:40.058410
2280.00000000 18873.46347257 9863.57004586 27863.46574735 -0.716736981 1.278632817 2.358448535 2006 6 27 3:28:40.058423
2400.00000000 10649.86857581 16841.14172669 39025.48035006 -1.426527152 0.673901057 0.826632332 2006 6 27 5:28:40.058396
2520.00000000 -440.53459323 19608.95524423 40343.10675451 -1.593138597 0.087147884 -0.452680559 2006 6 27 7:28:40.058410
2640.00000000 -11342.45028909 17771.44223942 32211.12535721 -1.346344015 -0.641464291 -1.860864234 2006 6 27 9:28:40.058423
2760.00000000 -16948.06005711 8987.64254880 11826.28284367 0.318007297 -2.009693492 -4.026726648 2006 6 27 11:28:40.058396
2880.00000000 15500.53445068 -1332.90981042 3419.72315308 2.960917974 1.758331634 4.813698638 2006 6 27 13:28:40.058410
9998 xx
0.00000000 25532.98947267 -27244.26327953 -1.11572421 2.410283885 2.194175683 0.545888526
-1440.00000000 -11362.18265118 -35117.55867813 -5413.62537994 3.137861261 -1.011678260 0.267510059 2005 5 27 19:03:37.089777
-1380.00000000 309.25349929 -36960.43090143 -4198.48007670 3.292429375 -0.002166046 0.402111628 2005 5 27 20:03:37.089763
-1320.00000000 11949.04009077 -35127.37816804 -2565.89806468 3.119942784 1.012096444 0.497284100 2005 5 27 21:03:37.089790
-1260.00000000 22400.45329336 -29798.63236321 -677.91515122 2.638533344 1.922477736 0.542792913 2005 5 27 22:03:37.089777
-1200.00000000 30640.84752458 -21525.02340201 1277.34808722 1.903464941 2.634294312 0.534540934 2005 5 27 23:03:37.089763
-1140.00000000 35899.56788035 -11152.71158138 3108.72535238 0.997393045 3.079858548 0.474873291 2005 5 28 0:03:37.089790
-1080.00000000 37732.45438600 288.18821054 4643.87587495 0.016652226 3.225184410 0.371669746 2005 5 28 1:03:37.089777
-1020.00000000 36045.92961699 11706.61816230 5746.32646574 -0.942409065 3.069888941 0.236662980 2005 5 28 2:03:37.089763
-960.00000000 31076.77273609 22063.44379776 6325.93403705 -1.794027976 2.642072476 0.083556127 2005 5 28 3:03:37.089790
-900.00000000 23341.26015320 30460.88002531 6342.91707895 -2.469409743 1.990861658 -0.073612096 2005 5 28 4:03:37.089777
-840.00000000 13568.39733054 36204.45930900 5806.79548733 -2.919354203 1.178920217 -0.221646814 2005 5 28 5:03:37.089763
-780.00000000 2628.58762420 38840.10855897 4771.91979854 -3.114400514 0.276239109 -0.348926401 2005 5 28 6:03:37.089790
-720.00000000 -8535.81598158 38171.79073851 3331.00311285 -3.043839958 -0.644462527 -0.445808894 2005 5 28 7:03:37.089777
11801 xx
0.00000000 7473.37102491 428.94748312 5828.74846783 5.107155391 6.444680305 -0.186133297
360.00000000 -3305.22148694 32410.84323331 -24697.16974954 -1.301137319 -1.151315600 -0.283335823 1980 8 17 13:06:40.136822
720.00000000 14271.29083858 24110.44309009 -4725.76320143 -0.320504528 2.679841539 -2.084054355 1980 8 17 19:06:40.136822
1080.00000000 -9990.05800009 22717.34212448 -23616.88515553 -1.016674392 -2.290267981 0.728923337 1980 8 18 1:06:40.136822
1440.00000000 9787.87836256 33753.32249667 -15030.79874625 -1.094251553 0.923589906 -1.522311008 1980 8 18 7:06:40.136822
14128 xx
0.00000000 34747.57932696 24502.37114079 -1.32832986 -1.731642662 2.452772615 0.608510081
120.00000000 18263.33439094 38159.96004751 4186.18304085 -2.744396611 1.255583260 0.528558932 2006 6 25 2:40:57.987566
240.00000000 -3023.38840703 41783.13186459 7273.03412906 -3.035574793 -0.271656544 0.309645251 2006 6 25 4:40:57.987539
360.00000000 -23516.34391907 34424.42065671 8448.49867693 -2.529120477 -1.726186020 0.009582303 2006 6 25 6:40:57.987553
480.00000000 -37837.46699511 18028.39727170 7406.25540271 -1.360069525 -2.725794686 -0.292555349 2006 6 25 8:40:57.987566
600.00000000 -42243.58460661 -3093.72887774 4422.91711801 0.163110919 -3.009980598 -0.517584362 2006 6 25 10:40:57.987539
720.00000000 -35597.57919549 -23407.91145393 282.09554383 1.641405246 -2.506773678 -0.606963478 2006 6 25 12:40:57.987553
840.00000000 -19649.19834455 -37606.11623860 -3932.71525948 2.689647056 -1.349150016 -0.537710698 2006 6 25 14:40:57.987566
960.00000000 1431.30912160 -41982.04949668 -7120.45467057 3.035263353 0.160882945 -0.327993994 2006 6 25 16:40:57.987539
1080.00000000 22136.97605384 -35388.19823762 -8447.62393401 2.587624889 1.630097136 -0.032349004 2006 6 25 18:40:57.987553
1200.00000000 37050.15790219 -19537.23321425 -7564.83463543 1.461844494 2.674654256 0.272202191 2006 6 25 20:40:57.987566
1320.00000000 42253.81760945 1431.81867593 -4699.87621174 -0.049247334 3.019518960 0.505890058 2006 6 25 22:40:57.987539
1440.00000000 36366.59147396 22023.54245720 -601.47121821 -1.549681546 2.571788981 0.607057418 2006 6 26 0:40:57.987553
1560.00000000 20922.12287985 36826.33975981 3654.91125886 -2.644070068 1.447521216 0.548722983 2006 6 26 2:40:57.987566
1680.00000000 -23.77224182 41945.51688402 6950.29891751 -3.043358385 -0.057417440 0.346112094 2006 6 26 4:40:57.987539
1800.00000000 -20964.17821076 36039.06206172 8418.91984963 -2.642795221 -1.546099886 0.052725852 2006 6 26 6:40:57.987553
1920.00000000 -36401.63863057 20669.75286162 7677.19769359 -1.549488154 -2.627052310 -0.254079652 2006 6 26 8:40:57.987566
2040.00000000 -42298.30327543 -119.03351118 4922.96388841 -0.052232768 -3.018152669 -0.493827331 2006 6 26 10:40:57.987539
2160.00000000 -37125.62383511 -20879.63058368 879.86971348 1.456499841 -2.619358421 -0.604081694 2006 6 26 12:40:57.987553
2280.00000000 -22250.12320553 -36182.74736487 -3393.15365183 2.583161226 -1.536647628 -0.556404555 2006 6 26 14:40:57.987566
2400.00000000 -1563.06258654 -42035.43179159 -6780.02161760 3.034917506 -0.052702046 -0.363395654 2006 6 26 16:40:57.987539
2520.00000000 19531.64069587 -36905.65470956 -8395.46892032 2.693682199 1.446079999 -0.075256054 2006 6 26 18:40:57.987553
2640.00000000 35516.53506142 -22123.71916638 -7815.04516935 1.646882125 2.568416058 0.232985912 2006 6 26 20:40:57.987566
2760.00000000 42196.03535976 -1547.32646751 -5187.39401981 0.166491841 3.019211549 0.480665780 2006 6 26 22:40:57.987539
2880.00000000 37802.25393045 19433.57330019 -1198.66634226 -1.359930580 2.677830903 0.602507466 2006 6 27 0:40:57.987553
16925 xx
0.00000000 5559.11686836 -11941.04090781 -19.41235206 3.392116762 -1.946985124 4.250755852
120.00000000 12339.83273749 -2771.14447871 18904.57603433 -0.871247614 2.600917693 0.581560002 2006 5 31 18:10:47.226141
240.00000000 -3385.00215658 7538.13955729 200.59008616 -2.023512865 -4.261808344 -6.856385787 2006 5 31 20:10:47.226115
360.00000000 12805.22442200 -10258.94667177 13780.16486738 0.619279224 1.821510542 2.507365975 2006 5 31 22:10:47.226128
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20413 xx
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23333 xx
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23599 xx
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pyorbital-1.0.0/pyorbital/tests/test_aiaa.py 0000664 0000000 0000000 00000013404 12567135624 0021205 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2011, 2014 SMHI
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Test cases from the AIAA article.
"""
# TODO: right formal unit tests.
from __future__ import with_statement
import os
from pyorbital.orbital import Orbital, OrbitElements, _SGDP4
from pyorbital.tlefile import ChecksumError
from pyorbital import tlefile, astronomy
import numpy as np
from datetime import timedelta, datetime
import unittest
class LineOrbital(Orbital):
"""Read TLE lines instead of file.
"""
def __init__(self, satellite, line1, line2):
satellite = satellite.upper()
self.satellite_name = satellite
self.tle = tlefile.read(satellite, line1=line1, line2=line2)
self.orbit_elements = OrbitElements(self.tle)
self._sgdp4 = _SGDP4(self.orbit_elements)
def get_results(satnumber, delay):
"""Get expected results from result file.
"""
path = os.path.dirname(os.path.abspath(__file__))
with open(os.path.join(path, "aiaa_results")) as f_2:
line = f_2.readline()
while(line):
if line.endswith(" xx\n") and int(line[:-3]) == satnumber:
line = f_2.readline()
while(not line.startswith("%.8f"%delay)):
line = f_2.readline()
sline = line.split()
if delay == 0:
utc_time = None
else:
utc_time = datetime.strptime(sline[-1], "%H:%M:%S.%f")
utc_time = utc_time.replace(year=int(sline[-4]),
month=int(sline[-3]),
day=int(sline[-2]))
return (float(sline[1]),
float(sline[2]),
float(sline[3]),
float(sline[4]),
float(sline[5]),
float(sline[6]),
utc_time)
line = f_2.readline()
class AIAAIntegrationTest(unittest.TestCase):
"""Test against the AIAA test cases.
"""
def test_aiaa(self):
"""Do the tests against AIAA test cases.
"""
path = os.path.dirname(os.path.abspath(__file__))
with open(os.path.join(path, "SGP4-VER.TLE")) as f__:
test_line = f__.readline()
while(test_line):
if test_line.startswith("#"):
test_name = test_line
if test_line.startswith("1 "):
line1 = test_line
if test_line.startswith("2 "):
line2 = test_line[:69]
times = str.split(test_line[69:])
times = np.arange(float(times[0]),
float(times[1]) + 1,
float(times[2]))
if test_name.startswith("# SL-14 DEB"):
# FIXME: we have to handle decaying satellites!
test_line = f__.readline()
continue
try:
o = LineOrbital("unknown", line1, line2)
except NotImplementedError, e:
test_line = f__.readline()
continue
except ChecksumError, e:
self.assertTrue(test_line.split()[1] in ["33333", "33334", "33335"])
for delay in times:
try:
test_time = timedelta(minutes=delay) + o.tle.epoch
pos, vel = o.get_position(test_time, False)
res = get_results(int(o.tle.satnumber), float(delay))
except NotImplementedError:
# Skipping deep-space
break
# except ValueError, e:
# from warnings import warn
# warn(test_name + ' ' + str(e))
# break
delta_pos = 5e-6 # km = 5 mm
delta_vel = 5e-9 # km/s = 5 um/s
delta_time = 1e-3 # 1 milisecond
self.assertTrue(abs(res[0] - pos[0]) < delta_pos)
self.assertTrue(abs(res[1] - pos[1]) < delta_pos)
self.assertTrue(abs(res[2] - pos[2]) < delta_pos)
self.assertTrue(abs(res[3] - vel[0]) < delta_vel)
self.assertTrue(abs(res[4] - vel[1]) < delta_vel)
self.assertTrue(abs(res[5] - vel[2]) < delta_vel)
if res[6] is not None:
dt = astronomy._days(res[6] - test_time) * 24 * 60
self.assertTrue(abs(dt) < delta_time)
test_line = f__.readline()
def suite():
"""The suite for test_aiaa
"""
loader = unittest.TestLoader()
mysuite = unittest.TestSuite()
mysuite.addTest(loader.loadTestsFromTestCase(AIAAIntegrationTest))
return mysuite
pyorbital-1.0.0/pyorbital/tests/test_astronomy.py 0000664 0000000 0000000 00000003674 12567135624 0022355 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2013, 2014 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
import unittest
from datetime import datetime
import pyorbital.astronomy as astr
class TestAstronomy(unittest.TestCase):
def setUp(self):
pass
def test_jdays(self):
"""Test julian day functions.
"""
t = datetime(2000, 1, 1, 12, 0)
self.assertEqual(astr.jdays(t), 2451545.0)
self.assertEqual(astr.jdays2000(t), 0)
t = datetime(2009, 10, 8, 14, 30)
self.assertEqual(astr.jdays(t), 2455113.1041666665)
self.assertEqual(astr.jdays2000(t), 3568.1041666666665)
def test_sunangles(self):
"""Test the sun-angle calculations:
"""
lat, lon = 58.6167, 16.1833 # Norrkoping
time_slot = datetime(2011, 9, 23, 12, 0)
sun_theta = astr.sun_zenith_angle(time_slot, lon, lat)
self.assertEqual(sun_theta, 60.371433482557833)
sun_theta = astr.sun_zenith_angle(time_slot, 0., 0.)
self.assertEqual(sun_theta, 1.8751916863323426)
def suite():
"""The suite for test_astronomy
"""
loader = unittest.TestLoader()
mysuite = unittest.TestSuite()
mysuite.addTest(loader.loadTestsFromTestCase(TestAstronomy))
return mysuite
pyorbital-1.0.0/pyorbital/tests/test_geoloc.py 0000664 0000000 0000000 00000014300 12567135624 0021556 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2014 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Test the geoloc module.
"""
import unittest
from pyorbital.geoloc_instrument_definitions import avhrr
from pyorbital.geoloc import (ScanGeometry, qrotate,
subpoint, geodetic_lat)
import numpy as np
from datetime import datetime, timedelta
class TestQuaternion(unittest.TestCase):
"""Test the quaternion rotation.
"""
def test_qrotate(self):
"""Test quaternion rotation
"""
vector = np.array([[1, 0, 0]]).T
axis = np.array([[0, 1, 0]]).T
angle = np.deg2rad(90)
self.assertTrue(np.allclose(qrotate(vector, axis, angle),
np.array([[0, 0, 1]]).T))
axis = np.array([0, 1, 0])
self.assertTrue(np.allclose(qrotate(vector, axis, angle),
np.array([[0, 0, 1]]).T))
vector = np.array([[1, 0, 0],
[0, 0, 1]]).T
axis = np.array([0, 1, 0])
angle = np.deg2rad(90)
self.assertTrue(np.allclose(qrotate(vector, axis, angle),
np.array([[0, 0, 1],
[-1, 0, 0]]).T))
axis = np.array([[0, 1, 0]]).T
self.assertTrue(np.allclose(qrotate(vector, axis, angle),
np.array([[0, 0, 1],
[-1, 0, 0]]).T))
class TestGeoloc(unittest.TestCase):
"""Test for the core computing part.
"""
def test_scan_geometry(self):
"""Test the ScanGeometry object.
"""
instrument = ScanGeometry(np.deg2rad(np.array([[10, 0],
[0, 0],
[-10, 0]])),
np.array([-0.1, 0, 0.1]))
self.assertTrue(np.allclose(np.rad2deg(instrument.fovs[:, 0]),
np.array([10, 0, -10])))
# Test vectors
pos = np.array([[0, 0, 7000]]).T
vel = np.array([[1, 0, 0]]).T
vec = instrument.vectors(pos, vel)
self.assertTrue(np.allclose(np.array([[0, 0, -1]]),
vec[:, 1]))
# minus sin because we use trigonometrical direction of angles
self.assertTrue(np.allclose(np.array([[0,
-np.sin(np.deg2rad(10)),
-np.cos(np.deg2rad(10))]]),
vec[:, 0]))
self.assertTrue(np.allclose(np.array([[0,
-np.sin(np.deg2rad(-10)),
-np.cos(np.deg2rad(-10))]]),
vec[:, 2]))
# Test times
start_of_scan = datetime(2014, 1, 8, 11, 30)
times = instrument.times(start_of_scan)
self.assertEquals(times[1], start_of_scan)
self.assertEquals(times[0], start_of_scan - timedelta(seconds=0.1))
self.assertEquals(times[2], start_of_scan + timedelta(seconds=0.1))
def test_geodetic_lat(self):
"""Test the determination of the geodetic latitude.
"""
a = 6378.137 # km
b = 6356.75231414 # km, GRS80
point = np.array([7000, 0, 7000])
self.assertEqual(geodetic_lat(point), 0.78755832699854733)
points = np.array([[7000, 0, 7000],
[7000, 0, 7000]]).T
self.assertTrue(np.allclose(geodetic_lat(points),
np.array([0.78755832699854733,
0.78755832699854733])))
def test_subpoint(self):
"""Test nadir determination.
"""
a = 6378.137 # km
b = 6356.75231414 # km, GRS80
point = np.array([0, 0, 7000])
nadir = subpoint(point, a, b)
self.assertTrue(np.allclose(nadir, np.array([[0, 0, b]]).T))
point = np.array([7000, 0, 7000])
nadir = subpoint(point, a, b)
self.assertTrue(np.allclose(nadir,
np.array([[4507.85431429,
0,
4497.06396339]]).T))
points = np.array([[7000, 0, 7000],
[7000, 0, 7000]]).T
nadir = subpoint(points, a, b)
self.assertTrue(np.allclose(nadir,
np.array([[4507.85431429,
0,
4497.06396339]]).T))
class TestGeolocDefs(unittest.TestCase):
"""Test the instrument definitions.
"""
def test_avhrr(self):
"""Test the definition of the avhrr instrument
"""
avh = avhrr(1, np.array([0, 1023.5 ,2047]))
self.assertTrue(np.allclose(np.rad2deg(avh.fovs[:, 0]),
np.array([55.37, 0, -55.37])))
avh = avhrr(1, np.array([0, 1023.5 ,2047]), 10)
self.assertTrue(np.allclose(np.rad2deg(avh.fovs[:, 0]),
np.array([10, 0, -10])))
def suite():
"""The suite for test_geoloc
"""
loader = unittest.TestLoader()
mysuite = unittest.TestSuite()
mysuite.addTest(loader.loadTestsFromTestCase(TestQuaternion))
mysuite.addTest(loader.loadTestsFromTestCase(TestGeoloc))
mysuite.addTest(loader.loadTestsFromTestCase(TestGeolocDefs))
return mysuite
pyorbital-1.0.0/pyorbital/tests/test_orbital.py 0000664 0000000 0000000 00000010640 12567135624 0021745 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2012-2014 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Test the geoloc orbital.
"""
import unittest
from datetime import datetime, timedelta
import numpy as np
from pyorbital import orbital
eps_deg = 10e-3
class Test(unittest.TestCase):
def test_get_orbit_number(self):
"""Testing getting the orbitnumber from the tle"""
sat = orbital.Orbital("NPP",
line1="1 37849U 11061A 12017.90990040 -.00000112 00000-0 -32693-4 0 772",
line2="2 37849 98.7026 317.8811 0001845 92.4533 267.6830 14.19582686 11574")
dobj = datetime(2012, 1, 18, 8, 4, 19)
orbnum = sat.get_orbit_number(dobj)
self.assertEqual(orbnum, 1163)
def test_sublonlat(self):
sat = orbital.Orbital("ISS (ZARYA)",
line1="1 25544U 98067A 03097.78853147 .00021906 00000-0 28403-3 0 8652",
line2="2 25544 51.6361 13.7980 0004256 35.6671 59.2566 15.58778559250029")
d = datetime(2003, 3, 23, 0, 3, 22)
lon, lat, alt = sat.get_lonlatalt(d)
expected_lon = -68.199894472013213
expected_lat = 23.159747677881075
expected_alt = 392.01953430856935
self.failUnless(np.abs(lon - expected_lon) < eps_deg, 'Calculation of sublon failed')
self.failUnless(np.abs(lat - expected_lat) < eps_deg, 'Calculation of sublat failed')
self.failUnless(np.abs(alt - expected_alt) < eps_deg, 'Calculation of altitude failed')
def test_observer_look(self):
sat = orbital.Orbital("ISS (ZARYA)",
line1="1 25544U 98067A 03097.78853147 .00021906 00000-0 28403-3 0 8652",
line2="2 25544 51.6361 13.7980 0004256 35.6671 59.2566 15.58778559250029")
d = datetime(2003, 3, 23, 0, 3, 22)
az, el = sat.get_observer_look(d, -84.39733, 33.775867, 0)
expected_az = 122.45169655331965
expected_el = 1.9800219611255456
self.failUnless(np.abs(az - expected_az) < eps_deg, 'Calculation of azimut failed')
self.failUnless(np.abs(el - expected_el) < eps_deg, 'Calculation of elevation failed')
def test_orbit_num_an(self):
sat = orbital.Orbital("METOP-A",
line1="1 29499U 06044A 11254.96536486 .00000092 00000-0 62081-4 0 5221",
line2="2 29499 98.6804 312.6735 0001758 111.9178 248.2152 14.21501774254058")
d = datetime(2011, 9, 14, 5, 30)
self.assertEqual(sat.get_orbit_number(d), 25437)
def test_orbit_num_non_an(self):
sat = orbital.Orbital("METOP-A",
line1="1 29499U 06044A 13060.48822809 .00000017 00000-0 27793-4 0 9819",
line2="2 29499 98.6639 121.6164 0001449 71.9056 43.3132 14.21510544330271")
dt = timedelta(minutes=98)
self.assertEqual(sat.get_orbit_number(sat.tle.epoch + dt), 33028)
def test_orbit_num_equator(self):
sat = orbital.Orbital("SUOMI NPP",
line1="1 37849U 11061A 13061.24611272 .00000048 00000-0 43679-4 0 4334",
line2="2 37849 98.7444 1.0588 0001264 63.8791 102.8546 14.19528338 69643")
t1 = datetime(2013, 3, 2, 22, 2, 25)
t2 = datetime(2013, 3, 2, 22, 2, 26)
on1 = sat.get_orbit_number(t1)
on2 = sat.get_orbit_number(t2)
self.assertEqual(on1, 6973)
self.assertEqual(on2, 6974)
pos1, vel1 = sat.get_position(t1, normalize=False)
pos2, vel2 = sat.get_position(t2, normalize=False)
del vel1, vel2
self.assertTrue(pos1[2] < 0)
self.assertTrue(pos2[2] > 0)
def suite():
"""The suite for test_orbital
"""
loader = unittest.TestLoader()
mysuite = unittest.TestSuite()
mysuite.addTest(loader.loadTestsFromTestCase(Test))
return mysuite
pyorbital-1.0.0/pyorbital/tests/test_tlefile.py 0000664 0000000 0000000 00000006445 12567135624 0021745 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2014 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Testing TLE file reading
"""
from pyorbital.tlefile import Tle
import datetime
import unittest
line0 = "ISS (ZARYA)"
line1 = "1 25544U 98067A 08264.51782528 -.00002182 00000-0 -11606-4 0 2927"
line2 = "2 25544 51.6416 247.4627 0006703 130.5360 325.0288 15.72125391563537"
class TLETest(unittest.TestCase):
"""Test TLE reading.
We're using the wikipedia example::
ISS (ZARYA)
1 25544U 98067A 08264.51782528 -.00002182 00000-0 -11606-4 0 2927
2 25544 51.6416 247.4627 0006703 130.5360 325.0288 15.72125391563537
"""
def check_example(self, tle):
"""Check the *tle* instance against predetermined values.
"""
# line 1
self.assertEqual(tle.satnumber, "25544")
self.assertEqual(tle.classification, "U")
self.assertEqual(tle.id_launch_year, "98")
self.assertEqual(tle.id_launch_number, "067")
self.assertEqual(tle.id_launch_piece.strip(), "A")
self.assertEqual(tle.epoch_year, "08")
self.assertEqual(tle.epoch_day, 264.51782528)
epoch = (datetime.datetime(2008, 1, 1)
+ datetime.timedelta(days=264.51782528 - 1))
self.assertEqual(tle.epoch, epoch)
self.assertEqual(tle.mean_motion_derivative, -.00002182)
self.assertEqual(tle.mean_motion_sec_derivative, 0.0)
self.assertEqual(tle.bstar, -.11606e-4)
self.assertEqual(tle.ephemeris_type, 0)
self.assertEqual(tle.element_number, 292)
# line 2
self.assertEqual(tle.inclination, 51.6416)
self.assertEqual(tle.right_ascension, 247.4627)
self.assertEqual(tle.excentricity, .0006703)
self.assertEqual(tle.arg_perigee, 130.5360)
self.assertEqual(tle.mean_anomaly, 325.0288)
self.assertEqual(tle.mean_motion, 15.72125391)
self.assertEqual(tle.orbit, 56353)
def test_from_line(self):
tle = Tle("ISS (ZARYA)", line1=line1, line2=line2)
self.check_example(tle)
def test_from_file(self):
from tempfile import mkstemp
from os import write, close, remove
filehandle, filename = mkstemp()
try:
write(filehandle, "\n".join([line0, line1, line2]))
close(filehandle)
tle = Tle("ISS (ZARYA)", filename)
self.check_example(tle)
finally:
remove(filename)
def suite():
"""The suite for test_tlefile
"""
loader = unittest.TestLoader()
mysuite = unittest.TestSuite()
mysuite.addTest(loader.loadTestsFromTestCase(TLETest))
return mysuite
pyorbital-1.0.0/pyorbital/tlefile.py 0000664 0000000 0000000 00000022464 12567135624 0017543 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2011, 2012, 2013, 2014, 2015.
# Author(s):
# Esben S. Nielsen
# Martin Raspaud
# Panu Lahtinen
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
import logging
import datetime
import urllib2
import os
import glob
TLE_URLS = ('http://celestrak.com/NORAD/elements/weather.txt',
'http://celestrak.com/NORAD/elements/resource.txt')
LOGGER = logging.getLogger(__name__)
def read_platform_numbers(in_upper=False, num_as_int=False):
'''Read platform numbers from $PPP_CONFIG_DIR/platforms.txt if available.
'''
out_dict = {}
if "PPP_CONFIG_DIR" in os.environ:
platform_file = os.path.join(os.environ["PPP_CONFIG_DIR"],
"platforms.txt")
try:
fid = open(platform_file, 'r')
except IOError:
LOGGER.error("Platform file %s not found.", platform_file)
return out_dict
for row in fid:
# skip comment lines
if not row.startswith('#'):
parts = row.split()
if in_upper:
parts[0] = parts[0].upper()
if num_as_int:
parts[1] = int(parts[1])
out_dict[parts[0]] = parts[1]
fid.close()
return out_dict
SATELLITES = read_platform_numbers(in_upper=True, num_as_int=False)
'''
The platform numbers are given in a file $PPP_CONFIG/platforms.txt
in the following format:
# Mappings between satellite catalogue numbers and corresponding
# platform names from OSCAR.
ALOS-2 39766
CloudSat 29107
CryoSat-2 36508
CSK-1 31598
CSK-2 32376
CSK-3 33412
CSK-4 37216
DMSP-F15 25991
DMSP-F16 28054
DMSP-F17 29522
DMSP-F18 35951
DMSP-F19 39630
EOS-Aqua 27424
EOS-Aura 28376
EOS-Terra 25994
FY-2D 29640
FY-2E 33463
FY-2F 38049
FY-2G 40367
FY-3A 32958
FY-3B 37214
FY-3C 39260
GOES-13 29155
GOES-14 35491
GOES-15 36411
Himawari-6 28622
Himawari-7 28937
Himawari-8 40267
INSAT-3A 27714
INSAT-3C 27298
INSAT-3D 39216
JASON-2 33105
Kalpana-1 27525
Landsat-7 25682
Landsat-8 39084
Meteosat-7 24932
Meteosat-8 27509
Meteosat-9 28912
Meteosat-10 38552
Metop-A 29499
Metop-B 38771
NOAA-15 25338
NOAA-16 26536
NOAA-17 27453
NOAA-18 28654
NOAA-19 33591
RadarSat-2 32382
Sentinel-1A 39634
SMOS 36036
SPOT-5 27421
SPOT-6 38755
SPOT-7 40053
Suomi-NPP 37849
TanDEM-X 36605
TerraSAR-X 31698
'''
def read(platform, tle_file=None, line1=None, line2=None):
"""Read TLE for *satellite* from *tle_file*, from *line1* and *line2*, from
the newest file provided in the TLES pattern, or from internet if none is
provided.
"""
return Tle(platform, tle_file=tle_file, line1=line1, line2=line2)
def fetch(destination):
"""fetch TLE from internet and save it to *destination*.
"""
with open(destination, "w") as dest:
for url in TLE_URLS:
response = urllib2.urlopen(url)
dest.write(response.read())
class ChecksumError(Exception):
'''ChecksumError.
'''
pass
class Tle(object):
"""Class holding TLE objects.
"""
def __init__(self, platform, tle_file=None, line1=None, line2=None):
self._platform = platform.strip().upper()
self._tle_file = tle_file
self._line1 = line1
self._line2 = line2
self.satnumber = None
self.classification = None
self.id_launch_year = None
self.id_launch_number = None
self.id_launch_piece = None
self.epoch_year = None
self.epoch_day = None
self.epoch = None
self.mean_motion_derivative = None
self.mean_motion_sec_derivative = None
self.bstar = None
self.ephemeris_type = None
self.element_number = None
self.inclination = None
self.right_ascension = None
self.excentricity = None
self.arg_perigee = None
self.mean_anomaly = None
self.mean_motion = None
self.orbit = None
self._read_tle()
self._checksum()
self._parse_tle()
@property
def line1(self):
'''Return first TLE line.'''
return self._line1
@property
def line2(self):
'''Return second TLE line.'''
return self._line2
@property
def platform(self):
'''Return satellite platform name.'''
return self._platform
def _checksum(self):
"""Performs the checksum for the current TLE.
"""
for line in [self._line1, self._line2]:
check = 0
for char in line[:-1]:
if char.isdigit():
check += int(char)
if char == "-":
check += 1
if (check % 10) != int(line[-1]):
raise ChecksumError(self._platform + " " + line)
def _read_tle(self):
'''Read TLE data.
'''
if self._line1 is not None and self._line2 is not None:
tle = self._line1.strip() + "\n" + self._line2.strip()
else:
if self._tle_file:
urls = (self._tle_file,)
open_func = open
elif "TLES" in os.environ:
# TODO: get the TLE file closest in time to the actual satellite
# overpass, NOT the latest!
urls = (max(glob.glob(os.environ["TLES"]),
key=os.path.getctime), )
LOGGER.debug("Reading TLE from %s", urls[0])
open_func = open
else:
LOGGER.debug("Fetch TLE from the internet.")
urls = TLE_URLS
open_func = urllib2.urlopen
tle = ""
designator = "1 " + SATELLITES.get(self._platform, '')
for url in urls:
fid = open_func(url)
for l_0 in fid:
if l_0.strip() == self._platform:
l_1, l_2 = fid.next(), fid.next()
tle = l_1.strip() + "\n" + l_2.strip()
break
if(self._platform in SATELLITES and
l_0.strip().startswith(designator)):
l_1 = l_0
l_2 = fid.next()
tle = l_1.strip() + "\n" + l_2.strip()
LOGGER.debug("Found platform %s, ID: %s",
self._platform,
SATELLITES[self._platform])
break
fid.close()
if tle:
break
if not tle:
raise KeyError("Found no TLE entry for '%s'" % self._platform)
self._line1, self._line2 = tle.split('\n')
def _parse_tle(self):
'''Parse values from TLE data.
'''
def _read_tle_decimal(rep):
'''Convert *rep* to decimal value.
'''
if rep[0] in ["-", " ", "+"]:
digits = rep[1:-2].strip()
val = rep[0] + "." + digits + "e" + rep[-2:]
else:
digits = rep[:-2].strip()
val = "." + digits + "e" + rep[-2:]
return float(val)
self.satnumber = self._line1[2:7]
self.classification = self._line1[7]
self.id_launch_year = self._line1[9:11]
self.id_launch_number = self._line1[11:14]
self.id_launch_piece = self._line1[14:17]
self.epoch_year = self._line1[18:20]
self.epoch_day = float(self._line1[20:32])
self.epoch = (datetime.datetime.strptime(self.epoch_year, "%y") +
datetime.timedelta(days=self.epoch_day - 1))
self.mean_motion_derivative = float(self._line1[33:43])
self.mean_motion_sec_derivative = _read_tle_decimal(self._line1[44:52])
self.bstar = _read_tle_decimal(self._line1[53:61])
try:
self.ephemeris_type = int(self._line1[62])
except ValueError:
self.ephemeris_type = 0
self.element_number = int(self._line1[64:68])
self.inclination = float(self._line2[8:16])
self.right_ascension = float(self._line2[17:25])
self.excentricity = int(self._line2[26:33]) * 10 ** -7
self.arg_perigee = float(self._line2[34:42])
self.mean_anomaly = float(self._line2[43:51])
self.mean_motion = float(self._line2[52:63])
self.orbit = int(self._line2[63:68])
def __str__(self):
import pprint
import StringIO
s_var = StringIO.StringIO()
d_var = dict(([(k, v) for k, v in
self.__dict__.items() if k[0] != '_']))
pprint.pprint(d_var, s_var)
return s_var.getvalue()[:-1]
def main():
'''Main for testing TLE reading.
'''
tle_data = read('Noaa-19')
print tle_data
if __name__ == '__main__':
main()
pyorbital-1.0.0/pyorbital/version.py 0000664 0000000 0000000 00000001473 12567135624 0017601 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2014, 2015 Martin Raspaud
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
"""Version file.
"""
__version__ = "v1.0.0"
pyorbital-1.0.0/setup.cfg 0000664 0000000 0000000 00000000120 12567135624 0015342 0 ustar 00root root 0000000 0000000 [bdist_rpm]
requires=numpy
release=1
doc_files = doc/Makefile doc/source/*.rst
pyorbital-1.0.0/setup.py 0000664 0000000 0000000 00000003476 12567135624 0015254 0 ustar 00root root 0000000 0000000 #!/usr/bin/env python
# -*- coding: utf-8 -*-
# Copyright (c) 2011-2014
# Author(s):
# Martin Raspaud
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
# GNU General Public License for more details.
# You should have received a copy of the GNU General Public License
# along with this program. If not, see .
from setuptools import setup
import imp
version = imp.load_source('pyorbital.version', 'pyorbital/version.py')
setup(name='pyorbital',
version=version.__version__,
description='Orbital parameters and astronomical computations in Python',
author='Martin Raspaud, Esben S. Nielsen',
author_email='martin.raspaud@smhi.se, esn@dmi.dk',
classifiers=["Development Status :: 5 - Production/Stable",
"Intended Audience :: Science/Research",
"License :: OSI Approved :: GNU General Public License v3 " +
"or later (GPLv3+)",
"Operating System :: OS Independent",
"Programming Language :: Python",
"Topic :: Scientific/Engineering",
"Topic :: Scientific/Engineering :: Astronomy"],
url="https://github.com/mraspaud/pyorbital",
test_suite='pyorbital.tests.suite',
package_dir = {'pyorbital': 'pyorbital'},
packages = ['pyorbital'],
install_requires=['numpy>=1.6.0'],
zip_safe=False,
)