On the comet model of Biermann et AL

Physics

Scientific paper

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Atmospheric Ionization, Comet Tails, Cosmic Plasma, Electromagnetic Radiation, Shock Waves, Solar Wind, Charged Particles, Discontinuity

Scientific paper

The Biermann equations for the interaction between solar wind and comets
are solved for gamma = 2 and gamma = .5/3. The interplanetary magnetic
field in the ionized atmosphere of comets is described.

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