NASA NTRS · 19800037032
Chorus, energetic electrons and magnetospheric substorms
Abstract
The paper investigates possible chorus generation mechanisms by means of simultaneous OGO-5 measurements of chorus, energetic (79 + or - 23 keV) electron fluxes and pitch angle distributions, and ambient magnetic fields. Further, the solar wind data during high-latitude dayside chorus events are examined. It is reported that the highly eccentric orbit had an apogee of 24 earth radii and an inclination of 30 deg to the geographic equator.
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Tsurutani, B. T., Smith, E. J., West, H. I., Jr., Buck, R. M.. 1979-01-01. Chorus, energetic electrons and magnetospheric substorms. https://ntrs.nasa.gov/citations/19800037032
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