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The effects of 8 Helios observed solar proton events of interplanetary magnetic field fluctuationsThere have been recent suggestions that large fluxes during solar energetic particle events may produce their own turbulence. To verify this argument it becomes essential to find out whether these flows cause an enhancement of interplanetary magnetic field fluctuations. In the present work, power and helicity spectra of the IMF before, during and after 8 Helios-observed solar proton events in the range 0.3 - 1 AU are analyzed. In order to detect proton self generated waves, the time evolution of spectra are followed.
Document ID
19960021432
Acquisition Source
Jet Propulsion Laboratory
Document Type
Conference Paper
Authors
ValdezGalicia, J. F.
(Universidad Nacional Autonoma de Mexico Coyoacan, Mexico)
Alexander, P.
(Universidad Nacional Autonoma de Mexico Coyoacan, Mexico)
Otaola, J. A.
(Universidad Nacional Autonoma de Mexico Coyoacan, Mexico)
Date Acquired
August 17, 2013
Publication Date
June 30, 1995
Publication Information
Publication: International Solar Wind 8 Conference
Subject Category
Solar Physics
Accession Number
96N24828
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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