Simple Project List Software Map

178 projects in result set
Última actualización: 2014-05-15 00:17

Mars Simulation Project

The Mars Simulation Project is an open source Java project to create a simulation of a future human settlement on the planet Mars.

Última actualización: 2015-09-07 06:40

Smart KP Horary Astrology

時間占星術は星占い占星術を占星術星占い、占星術師で、質問に回答する時間を構築することによって質問に答えるしようの古代ブランチです。スマート ソフトウェア。!AstroOpenSource@gmail.com。

(Machine Translation)
Última actualización: 2011-07-02 20:51

Stellarium

Stellarium renders 3D photo-realistic skies in real time with OpenGL. It displays stars, constellations, planets, nebulas and others things like ground, landscape, fog, etc.

Última actualización: 2014-03-16 18:06

INDI

INDI is an instrument-neutral distributed interface control protocol that aims to provide backend driver support and automation for a wide range of astronomical devices (telescopes, focusers, CCDs, etc.). Current supported devices include many telescopes, CCDs, filter wheels, focusers, and video cams. INDI is used in popular astronomy suites like Xephem, KStars, DCD, and Cartes Du Ciel.

Última actualización: 2022-03-07 13:31

Sky Chart / Cartes du Ciel

SkyChart は、たくさんの星々や星雲の一覧表からアマチュア天文家が夜空の天文図を描画するためのソフトウェアです。 惑星の位置を表示し、様々な食(日食や月食など)をシミュレートし、人工衛星を観察することができます。また、望遠鏡を動かすこともできます。

Última actualización: 2009-05-13 12:38

Xplanet

Xplanet was inspired by Xearth, which renders an image of the earth into the X root window. All of the major planets and most satellites can be drawn, similar to JPL's Solar System Simulator. A number of different map projections are also supported, including azimuthal, Mercator, Mollweide, orthographic, and rectangular.

Última actualización: 2013-04-05 19:52

AstroAviBrowser

AstroAviBrowser is a small tool for astronomy imaging capture/processing. It allows you to open a video file, select the good frames, and save the new sequence in a new avi file using raw or lossless codecs. You may also de-bayer your frames and separate RGB plans. It's a kind of "AviRaw" for Linux.

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Última actualización: 2005-10-13 02:57

SImg

SImg is a software for astronomical image processing. It contains a tool for visualization of highly dynamic images. The package consists of a library and applications which use it. Some of the features are deconvolution (various methods), Video4Linux support, PSF computation, approximation by linear combination of images and polynoms, various color transforms, automatic shifting of image sets (for addition and color composition), and more.

(Machine Translation)
Última actualización: 2008-05-16 10:54

StarPlot

StarPlot is a GTK-based program, written in C++,
which can be used interactively to view
three-dimensional perspective charts of stars.
Charts can be recentered, rotated, or zoomed in or
out with a mouse click (this can also, of course,
be done via dialog boxes for more precision).
Stars may be viewed (or ignored) by spectral class
and absolute magnitude. Other features include
support for both celestial and galactic coordinate
systems, the ability to display extended
non-stellar objects, and a pop-up
Hertzsprung-Russell diagram. StarPlot is also
packaged with starconvert, a utility which
converts line-oriented stellar data records to
StarPlot format. Most star data files available on
the Internet can be converted this way if a short
file describing the original file format is
provided to starconvert.

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Última actualización: 2005-06-09 00:42

Sky Chart

SkyChart is software to draw a map of the night sky for the amateur astronomer from a bunch of stars and nebulae catalogs. It shows the position of the planets, simulates an eclipse, and shows artificial satellites. It can also drive the telescope.

Última actualización: 2004-11-02 17:10

Cactus

Cactus is a general, modular, parallel environment for solving systems of partial differential

equations. The code has been developed over many years by a large international collaboration of numerical relativity and computational science research groups and can be used to provide a portable platform for solving any system of partial differential equations.

Última actualización: 2014-03-02 18:11

Lynkeos

Lynkeos processes astronomical webcam images. By
stacking the best images, the signal to noise
ratio is increased, and details lost in the noise
of individual images become visible in the
resulting image. This software accepts, as input,
QuickTime, AVI, and MPEG sequences, or still images, in any image format supported by its active plugins (TIFF, FITS) and Cocoa. It generates a 16-bit RGB TIFF or a monochrome FITS image as output, to be further processed with some all-purpose image processing application.

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Última actualización: 2013-11-11 21:47

CFITSIO

CFITSIO is a library of C and Fortran subroutines for reading and writing data files in the FITS (Flexible Image Transport System) data format. It simplifies the task of writing software that deals with FITS files by providing an easy to use set of high-level routines that insulate the programmer from the internal complexities of the FITS file format.

Última actualización: 2013-08-11 18:04

ChiantiPy

ChiantiPy is a Python interface to the CHIANTI atomic database for astrophysical spectroscopy. The CHIANTI atomic database for astrophysical spectroscopy provides the information necessary to calculate the emission spectrum from hot plasmas. ChiantiPy provides several top-level classes to access the database and calculate continuum and emission line intensities.

(Machine Translation)
Última actualización: 2006-03-10 13:59

Simulum

Simulum deals with different simulations of star movements
and their visualizations. At first it looks at the projection and
accumulation of star brightness. In actually doing this it
distributes stars among a three dimensional figure. To get a
nice effect it combines the photographic image production
with a moving view point. So the outcome is the visual
impression of flying through a star field. Secondly it studies
different algorithms of particle movements and clustering.
The primary approach uses a combination of Newton's
gravitational law, energy, and impulse conservation. At all
these stages an highly dynamic view of the processes is able
to be produced.

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