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Accession Number:
AD0773650
Title:
Numerical Solutions for Long Unmodulated Whistler-Mode Signals in the Geomagnetosphere,
Descriptive Note:
Corporate Author:
STANFORD UNIV CALIF INST FOR PLASMA RESEARCH
Report Date:
1973-12-20
Pagination or Media Count:
21.0
Abstract:
The author gives a method for solving the integral equation derived in a previous report, governing the temperal evolution of the amplitude of a key-down whistler-mode signal which interacts with counter-streaming gyroresonant electrons in a limited region of the geomagnetosphere. Then, for a set of values of plasma and wave parameters typical for observations at l 3, the author gives a family of solutions for a range of energetic electron densities. A certain critical density must be present in order for sustained quasi-periodic amplitude pulsations, similar to those reported in the literature, to occur. A second, and higher, critical density, above which the amplitude can actually undergo a change in sign is found this corresponds to a 180 degree phase shift in the signal. The behavior of these solutions is then discussed from both a mathematical and a physical point of view. Modified author abstract
Distribution Statement:
APPROVED FOR PUBLIC RELEASE