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Magnetospherically reflected whistlers as a source of plasmaspheric hiss

Journal Article · · Geophysical Research Letters (American Geophysical Union); (United States)
DOI:https://doi.org/10.1029/91GL03167· OSTI ID:5448046
Ray-tracing simulations and estimates of whistler wave damping show that magnetospherically reflected whistlers can persist for {approximately}10{sup 2} s in a low frequency band (f {approximately} 1 kHz). The combined contribution from whistler rays produced by a single lightning flash but entering the magnetosphere at different points form a continuous hiss-like signal, as observed at a fixed point. Estimates indicate that the total whistler wave energy input into the magnetosphere from lightning discharges may maintain experimentally observed levels of magnetospheric hiss.
OSTI ID:
5448046
Journal Information:
Geophysical Research Letters (American Geophysical Union); (United States), Journal Name: Geophysical Research Letters (American Geophysical Union); (United States) Vol. 19:3; ISSN 0094-8276; ISSN GPRLA
Country of Publication:
United States
Language:
English

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