posted by Dmitry Abrosimov on Mon 14th Apr 2003 22:28 UTC
"Simulation results"
The 'Kepler' Microsoft Windows demo application was developed using the mathematical models described in section 1. The application simulates the behavior of massive bodies assemblages like star clusters, galaxies, planetary systems, etc., in real time. At the beginning the user may set the following physical parameters:

  • - space dimension (2-D or 3-D);
  • - view angle (in 3-D case only);
  • - number of stars;
  • - gravity constant;
  • - initial spatial distribution of coordinates (root-mean-square (RMS) in X, Y and Z axes);
  • - time integration step (as the integration step decreases, the calculation accuracy becomes higher but the performance slows down);
  • - mean and RMS of random initial velocities;
  • - angular velocity of the conglomeration regular rotation.

    In addition, the user may choose to either use or not use the Intel Integrated Performance Primitive library (see section 3). If IPP is used, the real-time performance rate (15-20 frames per second) for ~2500 stars assemblage may be achieved on a computer operating on a 2000 MHz Intel? Pentium?4 processor.

    Fig. 2 describes an example of a spiral galaxy formation and evolution simulation. A prolate cluster of 2500 stars (Fig. 2a) was rotated counter-clockwise. Such an assemblage passes several stages of evolution and finally becomes an elliptic galaxy. To estimate the reality of this example, several photos of authentic spiral galaxies are presented in Fig. 3 (all images were taken from the NASA NSSDC web site [3] and are courtesy of the Space Telescope Science Institute).

    Table of contents
    1. "Mathematical Model"
    2. "Simulation results"
    3. "Use of Intel Integrated Performance Primitives"
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