Ghange of physical conditions in the plasma tail of comet Austin

Details Ghange of physical conditions in the plasma tail of comet Austin Ghange of physical conditions in the plasma tail of comet Austin

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..403s&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 5, p. 403-408

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Scientific paper

The results of the investigation of physical conditions in the plasma
tail of the long-period comet Austin /1982 1 are presented for 15 dates.
The diffusion model was used. The magnetic field and other physical
parameters of the plasma tail of the comet (after the perihelion) are
estimated.

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