Computer Science
Scientific paper
Sep 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001em%26p...87...59p&link_type=abstract
Earth, Moon, and Planets, v. 87, Issue 2, p. 59-71 (1999).
Computer Science
3
Ac Electric Field, Relativistic Whistler, Uranus, Ac Electric Field, Relativistic Whistler, Uranus
Scientific paper
Relativistic whistler wave mode with a perpendicular AC electric field has been studied for generalized distribution function with an index j, which is reducible to bi-Maxwellian for j = 0, loss-cone for j = 1 and delta function for j = ∞. Based on particle trajectories, the dispersionrelation is obtained using the techniques of a kinetic approach anda method of characteristic solutions Calculations are compassed with observations of low frequency waves of Voyager 2 The growth rates for the plasma parameters suited to the magnetosphere of Uranus are obtained. It is inferred that, not the magnitude but the frequency of the AC field, influences the growth rate. In addition to the temperature anisotropy, plasma particles having a loss-cone provide an additional source of energy. The relativistic electrons along with increasing the growth rate, widen the band width so as to cover a wide frequency range thus may explain the entire spectrum of whistler emissions at Uranian bow shock.
Pandey R. P.
Pandey R. S.
Singh Manoj K.
No associations
LandOfFree
A Theoretical Study Of The Whistler Mode Instability At The Uranian Bow Shock does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A Theoretical Study Of The Whistler Mode Instability At The Uranian Bow Shock, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A Theoretical Study Of The Whistler Mode Instability At The Uranian Bow Shock will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1488967