Excitation of oblique whistler waves in magnetosphere and in interplanetary space at 1 A.U.

Details Excitation of oblique whistler waves in magnetosphere and in interplanetary space at 1 A.U. Excitation of oblique whistler waves in magnetosphere and in interplanetary space at 1 A.U.

Feb 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ep%26s...54..159p&link_type=abstract

Earth, Planets and Space, Volume 54, p. 159-165.

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Scientific paper

The oblique whistler waves have been studied having k vector at an angle to magnetic field for a generalized distribution function reducible to bi-maxwellian and loss-cone. The dispersion relation and growth rate have been obtained for oblique whistler mode instability incorporating the trajectory of the particles, in the presence of perpendicular a-c electric field by method of characteristic solutions. The effects of distribution function and beam effect have been discussed for the space plasma at magnetospheric height and at 1 A.U. The results are compared with satellite observations and reported results obtained by other techniques. Excitation of two separate, but simultaneous left hand polarized whistler mode at 1 A.U. by electron been are demonstrated.

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