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From the Solar Wind to the Magnetospheric Substorm

E.A. Ponomarev P.A. Sedykh O.V. Mager

E.A. Ponomarev, P.A. Sedykh, O.V. Mager. From the Solar Wind to the Magnetospheric Substorm[J]. 空间科学学报, 2005, 25(5): 397-405. doi: 10.11728/cjss2005.05.397
引用本文: E.A. Ponomarev, P.A. Sedykh, O.V. Mager. From the Solar Wind to the Magnetospheric Substorm[J]. 空间科学学报, 2005, 25(5): 397-405. doi: 10.11728/cjss2005.05.397
E.A. Ponomarev, P.A. Sedykh, O.V. Mager. From the Solar Wind to the Magnetospheric Substorm[J]. Journal of Space Science, 2005, 25(5): 397-405. doi: 10.11728/cjss2005.05.397
Citation: E.A. Ponomarev, P.A. Sedykh, O.V. Mager. From the Solar Wind to the Magnetospheric Substorm[J]. Journal of Space Science, 2005, 25(5): 397-405. doi: 10.11728/cjss2005.05.397

From the Solar Wind to the Magnetospheric Substorm

doi: 10.11728/cjss2005.05.397

From the Solar Wind to the Magnetospheric Substorm

  • 摘要: This paper gives a brief outline of the progression from the first substorm model developed in Ref.[4] and
    [8] based on Kennel's ideas[3], to the present views about the mechanism by which solar wind kinetic energy is converted to electromagnetic energy at the Bow Shock and by which this energy is transferred to the magnetosphere in the form of current; about the transformation of the energy of this current to gas kinetic energy of convecting plasma tubes, and, finally, the back transformation of gas kinetic energy to electromagnetic energy in secondary magnetospheric MHD generators. The questions of the formation of the magnetospheric convection system, the nature of substorm break-up, and of the matching of currents in the magnetosphere-ionosphere system are discussed.

     

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出版历程
  • 收稿日期:  1900-01-01
  • 修回日期:  1900-01-01
  • 刊出日期:  2005-09-15

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