Computer Science
Scientific paper
Jan 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9622785k&link_type=abstract
Conference Paper, Kiev Univ. USSR Space Plasma Lab.
Computer Science
Comet Tails, Solar Wind, Stratification, Cometary Atmospheres, Space Plasmas, Plasma Currents, Dissipation, Plasma Density, Plasma Interactions
Scientific paper
Stratification of cometary plasma due to interaction of cometary ionosphere with the solar wind stream is considered. Development of dissipative filamentation instability, which resides in division of background plasma to current structures, is studied. Typical spatial scales of these structures are evaluated. Comparison with observational phenomena is also made.
Kotsarenko Nikolay Ya.
Verkhoglyadova Olga P.
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