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Whistler waves observed upstream from collisionless shocksWaves in the frequency range 0.5 - 4 Hz were studied in the region upstream of the earth's bow shock using data from the fluxgate magnetic field experiment on IMP-6. Analysis of 150 examples of these waves during a three month interval indicates that amplitudes are generally less than 1 or 2 gammas and propagation directions generally make angles of between 20 and 40 degrees with the field direction. The waves as measured in the spacecraft frame of reference are either left or right hand polarized with respect to the average field direction. It is concluded that the observed waves are right handed waves in the plasma frame of reference with wavelengths of approximately 100 km propagating upstream in the whistler mode. Doppler shifting reduces the observed frequencies in the spacecraft frame and reverses the observed polarization for those waves propagating more directly upstream. Similar waves are seen ahead of most interplanetary shocks.
Document ID
19730015687
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Fairfield, D. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 2, 2013
Publication Date
May 1, 1973
Subject Category
Geophysics
Report/Patent Number
X-692-73-129
NASA-TM-X-66245
Report Number: X-692-73-129
Report Number: NASA-TM-X-66245
Accession Number
73N24414
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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