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a Fortran Library of Geomagnetic tools:
a Fortran object library for different platforms (OpenVMS, SunOS, HPUX, Linux, MS-DOS and MS-Windows). The library has been developed on a DEC/AXP platform under the operating system OpenVMS. The modules of the library have been written conform to Standard FORTRAN 77, extended to the use of STRUCTURE and RECORD statements. These statements greatly increase the user friendliness of the library and are generally supported by all FORTRAN 77 compilers. |
QSAS: The QMW Science Analysis System for Cluster
(Contains documentation and QSAS distribution )
QSAS is a software package which provides a flexible, extendable environment for the selection, manipulation, and display of space physics data. It is written by QM as part of our role in the Cluster Science Centre within the UK. The Particle Physics and Astronomy Research Council funds this project for the express support of the UK Cluster community, and authorized supply is therefore limited. The software includes a copyright notice and disclaimer. Users are free to modify their own private copies of the software, but should keep the original QM Copyright notice/disclaimer as part of any modified copy. Although more detailed information is provided within the release kit, QSAS is written in C/C++ and is compiled for Sun/Sparcstations running Solaris 2.7 and X11R5 as well as Linux under Mandrake. Graphical output/display requires IDL version 5.0 (or higher) or PGPLOT. |
PAPCO PAPCO Software
(PAnel Plot COmposer) is the plotting software originally developed at the Max-Planck-Institute fur Aeronomy, and now maintained at NIS-2, Los Alamos National Laboratory. The prime aim of this PAnel Plot COmposer is to allow the user to put together data from a great variety of sources, to fully exploit the aims of the ISTP program. PAPCO is based on IDL and is modular in structure and allows the user to select existing modules or to construct his/her own modules for a new data set. An almost complete set of modules exist for the POLAR mission. Click below for a complete list of existing modules. Use of PAPCO is free. Please read the rules of the road statement for joining the PAPCO effort. PAPCO also provides modules for CLUSTER and has been chosen for the CASSINI magnetospheric package as a display tool |
DISLIN is a high-level plotting library for displaying data as curves, polar plots, bar graphs, pie charts, 3D-color plots, surfaces, contours and maps. DISLIN is intended to be a powerful and easy to use software package for scientists and programmers. There are only a few graphics routines with a short parameter list needed to display the desired graphical output. A large variety of parameter setting routines can then be called to create individually customized graphics. DISLIN is available for several C, Fortran 77 and Fortran 90 compilers on the operating systems UNIX, Linux, FreeBSD, OpenVMS, Windows and MS-DOS. DISLIN is free for non-commercial use for the operating systems Linux and FreeBSD and for the MS-DOS and Windows compilers GCC, G77 and LCC. The DISLIN plotting extensions for Java, Python and Perl and the DISLIN interpreter DISGCL can be used freely for non-commercial applications on all operating systems. The DISLIN software can be downloaded via HTML and from FTP servers. |
...typesetting beautiful documents...
MiKTeX (pronounced mik-tech) is an up-to-date implementation of TeX and related programs for Windows (all current variants) on x86 systems. TeX is a typesetting system invented by D. E. Knuth.
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the TEX to HTML translator ( TTH )
TTH translates TEX, the predominant mark-up language for expressing mathematics, into HTML, the language of world-wide-web browsers. It thereby enables mathematical documents to be made available on the web. Document structure, using either the Plain or LaTeX macro packages, is also translated and incorporated in the form of hyperlinks. TTH is extremely fast and completely portable. It produces more compact, faster viewing, web documents than other converters, because it really translates the equations, instead of converting them to images. |
The Common Data Format (CDF) Obtaining CDF software and documentation
The National Space Science Data Center's (NSSDC) Common Data Format (CDF) is a self-describing data abstraction for the storage and manipulation of multidimensional data in a discipline-independent fashion. When one first hears the term 'Common Data Format' one intuitively thinks of data formats in the traditional (i.e. messy/convoluted storage of data on disk or tape) sense of the word. Although CDF has its own internal self describing format, it consists of more than just a data format. CDF is a scientific data management package (known as the 'CDF Library') which allows programmers and application developers to manage and manipulate scalar, vector, and multi-dimensional data arrays. The irony of the term 'FORMAT' is that the actual data format which CDF utilizes is completely transparent to the user and accessible through a consistent set of interface (known as the 'CDF Interface) routines. Therefore, programmers are not burdened with performing low level I/O's to physically format and unformat the data file. This is all done for them. The development of CDF arose out of the recognition by the NSSDC for a class of data models that is matched to the structure of scientific data and the applications (i.e. statistical and numerical methods, visualization, and management) they serve. |
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