Numerical simulations of comets - Predictions for Comet Giacobini-Zinner

Computer Science

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Cometary Atmospheres, Giacobini-Zinner Comet, Interplanetary Magnetic Fields, Magnetohydrodynamics, Computerized Simulation, Earth Magnetosphere, Solar Wind

Scientific paper

Simulations of Comet Giacobini-Zinner's interaction with solar wind are described and results are presented. The simulations are carried out via the numerical solution of the ideal MHD equations as an initial value problem in a uniform solar wind. The calculations are performed on a Cartesian mesh centered at the comet. Results reveal that the first significant modifications of the solar wind along the ISEE/ICE trajectory will occur 100,000 km from the solar wind comet axis.

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