Open Source Windows Astronomy Software - Page 12

QuickFlash is a C++-based analysis library for data files generated by the Flash hydrodynamics code. It provides high-performance access to large datasets in low memory situations and other restrictive environments.

This is the VB6 Source code for the RCOS TCC software

As an amateur astrophotographer, I like to use a small laptop to control my gear, the problem is that a standard display will ruin your acquired night vision. This program turns (temporarily) everything red to minimize the impact of the display on your night vision. You may want to install a red cursor scheme, one is included (from Oxygen Cursors by LAvalon in GPL 3.0) in the source distribution.

The purpose of this project is to build a client-server application that will send summaries from Seti@Home clients distributed all across a network to a central host, allowing that way to a monitoring program to show results and statistics for multiple c

Client desktop application to download and browse MSL Curiosity images from Mars. Program is written in PHP-GTK and uses MySQL database.

SBIG ST-7 camera controller

A SETI@Home/BOINC client watcher! User statistics powered by BOINCStats. But now built with the .NET environment.

python, SExtractor. A python module to read, write and manage SExtractor catalogs.

Spectroheliograph like Sol'Ex captured SER videos processing with simultaneous extraction and processing of main line image, subtracting image (for Helium), main2 image (for Doppler) and reference image for geometric processing of main image. Saves resulting images (main and reference) in FITS and XCF formats. Separate delta positions from baseline fitted curve for all lines (main, main2/subtractive and reference). Correction of inclination and size ratio of images. Doppler color image creation from adjoining lines (main1/main2). Transversalium correction. Glare reduction. Opens resulting images on Image16 for further processing.

SOFA.NET is a faithful implementation of the original FORTRAN SOFA software libraries. The SOFA libraries are a collection of classes which implement official IAU algorithms for fundamental-astronomy computations.

SPIDR (Space Physics Interactive Data Resource) is a distributed database and application server network, built to select, visualize and model historical space weather data. SPIDR is a web-application and a grid of data mining web-services.

Better than NASA--avoid sending *your* Mars probe off to empty space! SafeUnits is a Java-based project providing measurement-related classes whose instances, when exported, can only be imported to classes of matching types. NASA, just a friendly jibe

Satellite Tracking Web Service

ScenicSkies is a open source planetarium software under development which in time is going to have photorealistic rendering of the skies both during the day and night.

Improving the speed of the signal analysis code for Seti@home. Leveraging modern processors advanced features such as SIMD and parallel execution units, as well as identifying better methods to code existing functions.

Setistaus is a PHP script that displays the status of one or more SETI@home clients on a Web page.

*nix Sidereal Clock Application

Feature extraction toolkit based on a wavelet multiscale vision model. Includes 1D signal processing sample application for line identification and classification of astronomical spectra.

Simulation of star movements with great visualizations of flights through star fields.

Sky Observer's Almanac is a tool to assist astronomers in planning an observing session. By defining targets and events that one wishes to observe, it allows the user to schedule these targets in an optimal fashion, and spend more time observing.

SkyNET is a sky chart program for .NET

SkytechX is free astronomical planetarium for rendering real objects (stars, planets, comets etc.) on the map. Program works with range of years 1 AD and 3000 AD. Main catalogue is Tycho2 with more than 2.5 millions of bright stars. Customized internal catalogue of non-stellar objects has been composed of several sources like NGC, IC, PGC, Messier etc. and contains more than 100,000 of objects. The planetarium allows you to connect your telescope via ASCOM6 platform. You can search for solar or moon eclipses, planet conjunctions and other events in given time range. Supports work with overlayed DSS-FITS images directly on the map.

Program vznikol ako ročníková práca z informatiky na Gymnáziu Jána Adama Raymana v Prešove. Vznikol na základe programu PC – Sun (autor: V. Feik), ktorý slúži na digitalizáciu pozorovaní Slnka na Hvezdárni Františka Pešty v Sezimovom Ústí (ČR). Program Slnečné škvrny slúži na digitalizáciu pozorovaní slnečných škvŕn a fakulových polí. Pozorovania sú následne štatisticky spracované do tabuliek a grafov popisujúcich aktivitu Slnka. Program taktiež umožňuje výpočet fyzikálnych súradníc Slnka, Carringtonovej otočky a juliánskeho dátumu. Program je určený pre astronómov – amatérov aj profesionálnych astronómov. Program rieši komplexne problém pozorovania slnečných škvŕn. Taktiež realizuje kontrolu vstupných dát od užívateľa. Pre správne fungovanie programu je potrebné dať užívateľovi právo zapisovať do priečinku "C:\Program Files\Slnecne skvrny".

The software simulates the motion of the solar system by different numerical methods. On start, the software expects the input file planeten.txt in the same folder. This file should contain the desired initial conditions. The separator may be adjusted via the file settings.ini.

The Solar Monitor fetch the plots from NOAA's SWPC. First public release coming soon.