Instability of the cometary plasma tail — the instability in a plasma sheet

Details Instability of the cometary plasma tail — the instability in a plasma sheet Instability of the cometary plasma tail — the instability in a plasma sheet

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011raa....11..617l&link_type=abstract

Research in Astronomy and Astrophysics, Volume 11, Issue 5, pp. 617-624 (2011).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We consider the instability of the cometary plasma tail which is composed of a neutral sheet, two lobes of the ion tail and solar wind. The plasma is assumed to be highly conductive and incompressible. The unstable state yields a magnetic field which is perpendicular to the tail axis. Our result is consistent with findings about plasma from the International Cometary Explorer (ICE).

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