Trapped VLF radiation as a signature of the dynamical processes in the heliosphere

Details Trapped VLF radiation as a signature of the dynamical processes in the heliosphere Trapped VLF radiation as a signature of the dynamical processes in the heliosphere

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993adspr..13..223c&link_type=abstract

Advances in Space Research (ISSN 0273-1177), vol. 13, no. 6, p. 223-226.

Physics

1

Heliosphere, Plasma Density, Ray Tracing, Solar Wind Velocity, Trapped Particles, Plasma Interactions, Very Low Frequencies, Voyager Project

Scientific paper

A numerical ray tracing technique is used to study the time evolution of VLF radiation (2-3 kHz Voyager band) trapped in the heliosphere. Simulations include effects of co-rotating and merging interaction regions, heliolatitudinal dependence of solar wind speed and absorption by free-free transitions. The results imply constraints on solar wind dynamics as well as on the size and the tail geometry of the heliosphere.

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