Search Results for "linux-abi" - Page 15
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Showing 406 open source projects for "linux-abi"
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Coding convenient Aero & Astro functions into one easy to use package. From rocket engine design, to flight and space dynamics.
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A tool to visualize interactively huge amounts of eventdata. Uses an innovative hierarchical zoomlens scaling from quarters down to 50 ms.
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Strip Charts for GtkPlot provides a set of GTK widgets for creating strip plots of numeric data. Horizontal 'strips' of data are ganged; supports multiple color-changing limit (alarm) lines, multiple scrollable cursors (with callbacks).
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Height Map Editor is a program meant for editing, generating and manipulating height maps (terrains) that can be used in terrain rendering engines, or even as clouds.
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libgtk3dcanvas is a Gtk set of widgets to build easily simple 3D scene render engines. You can add items (balls, stick, polygone, ...) like on libgnomecanvas, and then, you can declare several camera (OpenGL, Direct3d...) to render it.
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Mandel is a command-line program for generating Mandelbrot set fractals - support for Julia sets is coming soon. Output is in the form of 8 bit greyscale Device Independent Bitmaps, which can be readily viewed with many common graphics programs.
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AutoMeter is a X11/Xt/Xaw application scanning and representing Linux (tm) /proc/* and more metrics in a automatically optimal scalling Athena Widget, called AutoScale. AutoScale is full color and has many representation options.
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StageLight Basic is a simple automated stage lighting sequencer idea for Schools, traveling performers, shops and small theatres.
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Script language independent library for calling functions out of script files with other PLs like C/C++. This should be possible, using only some few functions as interface.
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This is a SQL interface for scilab. It will enable users of scilab to do queries to a sql database and get the results in a normal scilab array. <p> <a href="http://www-rocq.inria.fr/scilab/"'>Scilab homepage</a>
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enhancements and development for the Vis5d scientific visualization tool, a program to display volumetric datasets in 3+ dimensions.
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SINFG is a resolution-independent image manipulation package, which allows you to create a wide variety of compositions including, but not limited to, fractals and vector images.
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Solid is a library for collision detection of three-dimensional objects undergoing rigid motion and deformation. Solid is designed to be used in interactive 3D graphics applications using a VRML-like scene graph.
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EiffelOpenGL is an Eiffel wrapping of OpenGL. As of today it consists of incomplete but working wrappings of the GL and GLU libraries, as well as the GLUT library. It is licensed under EFL - The Eiffel Forum License.
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Gnome Flow is program written to calculate and visualize simple, steady-state fluid flows around objects. The program calculates the stream, vorticity and pressure using the relaxation method.
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Gscope is a software oscilloscope library build using the GTK and GNOME toolkits. Gscope can be used to monitor, display and debug various types of "real-time" data. Additionally, the scope can be used for graphing file data that is in a tuple format.
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NeTraMet is an implementation of the Meter MIB (RFC2720-2723). In short: a programmable network traffic meter. Reading information from NeTraMet for further processing can be a challenge. mr2mysql should make that easier by automatically reading flows
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VMW is a software for students of Engineering/Science/Mathematics that can be used for solving mathematical problems in their field.
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fsv, the 3D File System Visualizer, allows you to view a collection of directories and files as three-dimensional geometry. It represents all or part of a filesystem as a collection of blocks of varying sizes, each labeled with a filename, and arranged in
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A 3D viewer for molecular charge distributions. Implemented in OpenGL with GLUT. Includes a small OpenGL windowing library/widget set.
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Light Speed! is an OpenGL-based program which interactively illustrates the effects of special relativity on the appearance of moving objects. When an object accelerates beyond (roughly) two hundred million meters per second, these strange effects become
