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Ion sound turbulence in the solar windA stability analysis for ion sound is carried out in order to contribute to clarifying the mechanism of some observed fluctuations, which directly uses detailed measured particle distributions rather than model distributions. Correlation with measured wave activity is satisfactory. Valuable information about the instability mechanism, transport processes, and the accuracy of measured distributions can be obtained by this method. An illustration from Helios 1 data is presented.
Document ID
19800005753
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Dum, C. T. (Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Marsch, E. (Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Pilipp, W. G. (Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Gurnett, D. A. (Iowa Univ.)
Date Acquired
August 10, 2013
Publication Date
April 1, 1979
Publication Information
Publication: Contrib. to the 4th Solar Wind Conf.
Subject Category
Solar Physics
Accession Number
80N14009
Funding Number(s)
CONTRACT_GRANT: NAS5-11279
CONTRACT_GRANT: NGL-16-001-043
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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