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Chorus, energetic electrons and magnetospheric substormsThe 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.
Document ID
19800037032
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Tsurutani, B. T. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Smith, E. J. (California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
West, H. I., Jr. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Buck, R. M. (California, University Lawrence Livermore Laboratory, Livermore, Calif., United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1979
Subject Category
Geophysics
Meeting Information
Meeting: Wave instabilities in space plasmas
Location: Helsinki
Country: Finland
Start Date: July 31, 1978
End Date: August 8, 1978
Accession Number
80A21202
Funding Number(s)
CONTRACT_GRANT: NAS7-100
CONTRACT_GRANT: W-7405-ENG-48
Distribution Limits
Public
Copyright
Other

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