The P/Giacobini-Zinner magnetotail

Details The P/Giacobini-Zinner magnetotail The P/Giacobini-Zinner magnetotail

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esla.sympq....s&link_type=abstract

Presented at the 20th ESLAB Symposium, Heidelberg, West Germany, 27 Oct. 1986

Physics

Comet Tails, Cometary Magnetospheres, Comets, Giacobini-Zinner Comet, Ice, Magnetic Fields, Electrons, Plasma Waves, Solar Wind

Scientific paper

On September 11, 1985 the International Cometary Explorer passed behind Comet Giacobini-Zinner with a closest approach distance of 7800 km. In agreement with Alfven's interplanetary magnetic field line draping model of cometary type I tails, a well defined 1 x 10 to the 4th power km diameter magnetotail was observed downstream of the inner coma. This study uses the ICE magnetic field, plasma electron, plasma wave, and energetic ion observations to investigate the structure and stability of the Giacobini-Zinner magnetic tail. Emphasis is placed on the identification of differences and similarities between cometary and planetary magnetotails. Finally, the ICE magnetotail observations are discussed in relation to the global solar wind interaction with P/Giacobini-Zinner magnetic tail.

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