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Interplanetary stream magnetism: Kinematic effectsThe particle density, and the magnetic field intensity and direction are calculated in corotating streams of the solar wind, assuming that the solar wind velocity is constant and radial and that its azimuthal variations are not two rapid. The effects of the radial velocity profile in corotating streams on the magnetic fields were examined using kinematic approximation and a variety of field configurations on the inner boundary. Kinematic and dynamic effects are discussed.
Document ID
19750011027
Acquisition Source
Legacy CDMS
Document Type
Preprint (Draft being sent to journal)
Authors
Burlaga, L. F. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Barouch, E. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 3, 2013
Publication Date
November 1, 1974
Subject Category
Astrophysics
Report/Patent Number
NASA-TM-X-70836
X-690-74-344
Accession Number
75N19099
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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