Some physical characteristics of the plasma tail of comet 1P/Halley

Details Some physical characteristics of the plasma tail of comet 1P/Halley Some physical characteristics of the plasma tail of comet 1P/Halley

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005kfnt...21..304s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 21, no. 4, p. 304-311

Computer Science

Scientific paper

The photometric scans of the plasma tail of Comet Halley are compared with the profiles of brightness distribution for the tail streams of which were calculated with the use of the diffusion model of the plasma tail. We estimated the magnetic field induction and the lifetime of ions in the tail of Comet Halley as well as the coefficients of diffusion during the observations al time. It is shown that the jump of the magnetic field induction in the plasma tail can be a result of a collision of the comet with a highstream solar wind.

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