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Pulsating auroras produced by interactions of electrons and time domain structures

Previous evidence has suggested that either lower band chorus waves or kinetic Alfven waves scatter equatorial kilovolt electrons that propagate to lower altitudes where they precipitate or undergo further low-altitude scattering to make pulsating auroras. Recently, time domain structures (TDSs) were shown, both theoretically and experimentally, to efficiently scatter equatorial electrons. To assess the relative importance of these three mechanisms for production of pulsating auroras, 11 intervals of equatorial THEMIS data a ...

Mozer, F.; Agapitov, O.; Hull, A.; Lejosne, S.; . Y. Vasko, I;

YEAR: 2017     DOI: 10.1002/2017JA024223

pulsating auroras; Van Allen Probes; wave scattering