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Ionosphere response to solar wind high-speed streams

✍ Scribed by Jiuhou Lei; Jeffrey P. Thayer; Jeffrey M. Forbes; Qian Wu; Chengli She; Weixing Wan; Wenbin Wang


Book ID
111880322
Publisher
American Geophysical Union
Year
2008
Tongue
English
Weight
862 KB
Volume
35
Category
Article
ISSN
1944-8007

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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