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The large-scale magnetic field in the solar windA literature review is presented of theoretical models of the interaction of the solar wind and interplanetary magnetic fields. Observations of interplanetary magnetic fields by the IMP and OSO spacecraft are discussed. The causes for cosmic ray variations (Forbush decreases) by the solar wind are examined. The model of Parker is emphasized. This model shows the three dimensional magnetic field lines of the solar wind to have the form of spirals wrapped on cones. It is concluded that an out-of-the-ecliptic solar probe mission would allow the testing and verification of the various theoretical models examined. Diagrams of the various models are shown.
Document ID
19760017040
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Burlaga, L. F. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Ness, N. F. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 3, 2013
Publication Date
March 1, 1976
Publication Information
Publication: Proc. of the Symp. on the Study of the Sun and Interplanetary Medium in Three Dimensions
Subject Category
Solar Physics
Accession Number
76N24128
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19760017031Collected WorksProceedings of the Symposium on the Study of the Sun and Interplanetary Medium in Three Dimensions
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