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Energy and mass content of high-speed solar-wind streams

✍ Scribed by Montgomery, Michael D.; Bame, S. J.; Hundhausen, A. J.


Book ID
119711014
Publisher
American Geophysical Union
Year
1972
Tongue
English
Weight
841 KB
Volume
77
Category
Article
ISSN
0148-0227

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It has been widely conjectured that magnetohydrodynamic (MHD) waves may provide the extra momentum or energy required to explain the high speed solar wind streams that originate in coronal holes. Although the magnetic structuring inherent in this problem has been incorporated into models of the bulk