Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..812i&link_type=abstract
(Astronomicheskii Zhurnal, vol. 61, July-Aug. 1984, p. 812-814) Soviet Astronomy (ISSN 0038-5301), vol. 28, July-Aug. 1984, p. 4
Astronomy and Astrophysics
Astronomy
Comet Tails, Cometary Atmospheres, Interplanetary Magnetic Fields, Ionospheres, Solar Wind, Ion Density (Concentration), Kelvin-Helmholtz Instability
Scientific paper
A possible mechanism for the penetration of a cometary atmosphere by a
magnetic field is presented. The mechanism is based on the known pattern
of solar wind propagation through a cometary ionosphere. It is shown
through a series of calculations that the penetrating field has a
braided configuration and can reach a velocity of 100,000 cm/s.
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