On the L-dependence of whistler-triggered emissions as based on the measurement at Ceduna, Australia (L = 1.93)

Details On the L-dependence of whistler-triggered emissions as based on the measurement at Ceduna, Australia (L = 1.93) On the L-dependence of whistler-triggered emissions as based on the measurement at Ceduna, Australia (L = 1.93)

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992p%26ss...40.1193h&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 40, no. 9, p. 1193-1195.

Physics

Ionospheric Propagation, Very Low Frequencies, Whistlers, Australia, Hiss, Isis Satellites, Lightning, Radiation Belts, Temporal Distribution, Wave-Particle Interactions

Scientific paper

The L-dependence of whistler-triggered VLF emissions was investigated on the basis of the wide-band observations made at Ceduna, Australia (L = 1.93), during the period 9-24, August, 1989. Most VLF emissions triggered by whistlers are of the hiss type, and it is found from the nose-extension method that those whistler-triggered emissions have taken place in the L range from 1.7 to 2.7, with the maximum occurrence from L = 2.1 to 2.3 in the electron slot region, and at L = 3.0-3.3.

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