32 projects tagged "Linux"
Updated 28 Feb 2013
aLinux
| Pop | 57.50 |
|---|---|
| Vit | 1.00 |
aLinux is an RPM-based GNU/Linux distribution that can be used for office and multimedia applications. Installing new programs and applications and updating your system is made easy by its Synaptic package management system. It can be installed from a USB stick or DVD-R.
Updated 15 Jan 2013
DISLIN
| Pop | 172.51 |
|---|---|
| Vit | 23.94 |
DISLIN is a high-level, easy-to-use plotting library for displaying data as curves, bar graphs, pie charts, 3D-colour plots, surfaces, contours, and maps. Several output formats are supported, such as X11, VGA, PostScript, PDF, CGM, HPGL, TIFF, and PNG. Plotting extensions for the interpreting languages Perl, Python, and Java are also supported for most operating systems.
Updated 22 Sep 2012
Hierarchical Data Format
| Pop | 328.93 |
|---|---|
| Vit | 50.05 |
HDF (Hierarchical Data Format) is a general purpose library and file format for storing scientific data. It arranges data into datasets (multidimensional arrays) and groups (a structure for organizing objects).
Updated 07 Aug 2012
sem2dpack
| Pop | 73.01 |
|---|---|
| Vit | 11.08 |
SEM2DPACK is a simulator of 2D elastic wave propagation and fracture dynamics that applies the Spectral Element Method (SEM, similar to mass-lumped high-order finite element methods). Flexibility and accuracy are the main goals. Although the emphasis is currently on computational seismology and earthquake source dynamics, this tool might attract a wider audience in computational mechanics, research, and engineering.
Updated 04 Aug 2012
NetCDF
| Pop | 232.96 |
|---|---|
| Vit | 24.42 |
NetCDF is a format developed at Unidata that was inspired by the CDF format from NASA. NetCDF stands for "Network Common Data Form" and is a self-describing data format, commonly used in scientific and engineering applications.
Updated 30 Jul 2012
WCSLIB
| Pop | 30.95 |
|---|---|
| Vit | 1.00 |
WCSLIB is a C library, supplied with a full set of Fortran wrappers, which implements the "World Coordinate System" (WCS) standard in FITS (Flexible Image Transport System). It also includes a PGPLOT-based routine, PGSBOX, for drawing general curvilinear coordinate graticules, and a number of utility programs. The FITS "World Coordinate System" (WCS) convention defines keywords and usage which provide descriptions of astronomical coordinate systems in a FITS image header.
Updated 30 Jul 2012
TAU
| Pop | 216.89 |
|---|---|
| Vit | 20.49 |
TAU (Tuning and Analysis Utilities) is a set of tools for analyzing the performance of C, C++, Fortran and Java programs. It collects much more information than is available through prof or gprof, the standard Unix utilities, including per-process, per-thread, and per-host information, inclusive and exclusive function times, profiling groups that allow you to organize data collection, access to hardware counters on some systems, per-class and per-instance information, the ability to separate data for each template instantiation, start/stop timers for profiling arbitrary sections of code, and support for collection of statistics on user-defined events.
Updated 24 Jul 2012
NeXus Scientific Data Format
| Pop | 29.90 |
|---|---|
| Vit | 1.00 |
NeXus Scientific Data Format is a set of data storage objects and APIs for storing data commonly collected in neutron and synchrotron experiments, to simplify the exchange and processing of these data sets, and to ease the development of new methods of processing such data.
Updated 26 Mar 2012
ECMWF GRIB
| Pop | 23.04 |
|---|---|
| Vit | 1.92 |
The ECMWF GRIB API is an application program interface accessible from C and FORTRAN programs developed for encoding and decoding WMO FM-92 GRIB edition 1 and edition 2 messages. A useful set of command line tools is also provided to give quick access to GRIB messages.
Updated 14 Dec 2011
astroPluto
| Pop | 20.52 |
|---|---|
| Vit | 1.00 |
astroPluto is modular Godunov-type code intended mainly for astrophysical applications and high Mach number flows in multiple spatial dimensions. The code embeds different hydrodynamic modules and multiple algorithms to solve the equations describing Newtonian, relativistic, MHD, or relativistic MHD fluids in Cartesian or curvilinear coordinates.
