Evidence for the control of Pc 3,4 magnetic pulsations by the solar wind velocity

H. J. Singer, C. T. Russell, M. G. Kivelson, E. W. Greenstadt, J. V. Olson

doi:10.1029/gl004i009p00377

Evidence for the control of Pc 3,4 magnetic pulsations by the solar wind velocity

DOI Web Site Web Site 被引用文献3件

書誌事項

公開日: 1977-09

権利情報

http://onlinelibrary.wiley.com/termsAndConditions#vor

DOI

10.1029/gl004i009p00377

公開者: American Geophysical Union (AGU)

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説明

<jats:p>The amplitude of Pc 3,4 magnetic pulsations at Calgary is shown to increase as the solar wind velocity increases. The pulsation amplitude dependence on solar wind velocity can be understood in terms of the Kelvin‐Helmholtz instability at the magnetopause boundary.</jats:p>