Magnetohydrodynamic tube waves and high
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P. S. Cally
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Article
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1987
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Springer
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English
β 395 KB
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