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Material Type: Notes; Class: Methods of Astronomy Research; Subject: Astronomy; University: University of Illinois - Urbana-Champaign; Term: Unknown 1989;
Typology: Study notes
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Developed by G. Bird (1960s) Stochastic method for solving gasdynamics flows with Kn ~ 1 (mean free path ๎ ~ size of system L ); works well into continuum regime (Kn โช 1) Used frequently in aerospace applications โ also planetary atmospheres, etc. Basic ingredients: โ (^) Particles โ Monte Carlo sampling of real particle velocity field โ (^) Trajectories โ integration of particle motion between collisions โ (^) Collisions โ fast method for including effects of collisions with appropriate correlations โ (^) Boundary conditions โ interactions with surfaces
To handle scattering we use a โmeshโ similar to the chaining mesh we use for P 3 M. Particles are associated with cells of size R > ๎ (e.g. by storing in linked lists). For each cell: loop until collisions have occurred: Choose collision pair ( i , j ). Decide if the pair will collide: Choose a random number ๎ ij
If | v i
ij v max , they collide. v max is the largest particle speed in the cell. If they collide: Choose new random directions for both particles. Conserve momentum and energy in the process.
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Probability of scattering depends only on relative particle velocities, not on their positions (except that they must be in same scattering cell). In particular, detailed dynamics of scattering process are not followed. If scattering depends on impact parameter, use โmolecular chaosโ assumption (implicit in the basic procedure) to choose a value at random. Conservation of energy and momentum (elastic hard spheres):
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Planetary rings Frezzotti
Mars Reconnaissance Orbiter aerobraking โ Hanna Prince & Striepe