FAST observations of auroral MF emissions and precipitating electrons

Details FAST observations of auroral MF emissions and precipitating electrons FAST observations of auroral MF emissions and precipitating electrons

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsm44a..01b&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #SM44A-01

Physics

7847 Radiation Processes, 7867 Wave/Particle Interactions (2483, 6984)

Scientific paper

Auroral medium frequency (MF) bursts are impulsive broadband non-thermal radio emissions observed at high latitudes in the frequency range 1--4 MHz [LaBelle et al., 2005, doi:10.1029/2004JA010608]. Ground-based measurements have established that Auroral Medium Frequency (MF) bursts occur near auroral substorm onset. Although there is evidence that they are associated with > 10 keV electron precipitation, the generation mechanism of the bursts is unknown. The Fast Auroral SnapshoT (FAST) Explorer satellite has made extensive observations of high frequency electric fields (0--2 MHz) in the auroral zones. We examine FAST wave and particle observations to determine the association between bursts of MF emissions and precipitating electrons.

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