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Distribution Functions of Type III Electrons Observed in Interplanetary Space

Published online by Cambridge University Press:  14 August 2015

R. P. Lin ,
D. W. Potter ,
K. A. Anderson ,
J. Fainberg ,
R. G. Stone  and
J. L. Steinberg
R. P. Lin
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720
D. W. Potter
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720
K. A. Anderson
Affiliation:
Space Sciences Laboratory, University of California, Berkeley, California 94720
J. Fainberg
Affiliation:
Goddard Space Flight Center, Greenbelt, Maryland 20771
R. G. Stone
Affiliation:
Goddard Space Flight Center, Greenbelt, Maryland 20771
J. L. Steinberg
Affiliation:
Department de Recherches Spatiales, Observatoire Meudon, 92190 Meudon, France

Extract

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We present simultaneous energetic electron and solar radio observations from the ISEE−3 spacecraft of several solar type III radio bursts. The UC Berkeley energetic particle experiment measures from 2 to ~ 103 keV with good energy and pitch angle resolution while the Meudon/GSFC radio experiment tracks type III radio bursts at 24 frequencies in the range 30 kHz—2 MHz.

Type
Session V - Solar Bursts - Meter-Decameter Wavelengths
Information
Symposium - International Astronomical Union , Volume 86: Radio Physics of the Sun , 1980 , pp. 311 - 313
Copyright
Copyright © Reidel 1980