Whistler-mode chorus and morningside aurorae

Details Whistler-mode chorus and morningside aurorae Whistler-mode chorus and morningside aurorae

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992georl..19..653i&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 19, April 3, 1992, p. 653-656. Research supported by Lockheed Independent Re

Physics

28

Auroras, Dawn Chorus, Extremely Low Frequencies, Very Low Frequencies, Whistlers, Earth Magnetosphere, Gyrofrequency, Particle Precipitation

Scientific paper

Quasi-electrostatic ELF/VLF chorus emissions immediately above the equatorial half-gyrofrequency, observed to propagate with wave normal angle within 0.4-1.2 deg of the resonance cone (Muto et al., 1987), are shown to efficiently resonate with 0.1-10 keV electrons. These waves may thus be important in driving the relatively low energy (less than 10 keV) component of pulsating aurorae and the morningside diffuse aurorae (about 1 keV).

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