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  • 1
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    Characteristics of the interplanetary shocks formed by a sudden increase in the velocity of the solar wind from a coronal hole (1995)
    In:  Other Sources
    Details
    Publication Date: 2011-08-24
    Description: Coronal holes are the sources of the solar wind and, according to recent YOKOH observations, may undergo rapid changes which are associated with manifestations of explosive solar activity. Rapid changes in a hole's structure will produce rapid changes in the characteristics of the wind emerging from it and, in the particular c se of a sudden increase in wind velocity, this may lead to the formation of an interplanetary shock. We discuss the characteristics of shocks formed in such a way and compare them with interplanetary observations.
    Keywords: Solar Physics
    Type: International Solar Wind 8 Conference; 99; NASA-CR-199940
    Format: text
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    NASA TECHNICAL REPORTS
  • 2
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    Self consistent MHD modeling of the solar wind from coronal holes with distinct geometries (1995)
    In:  Other Sources
    Details
    Publication Date: 2011-08-24
    Description: Utilizing an iterative scheme, a self-consistent axisymmetric MHD model for the solar wind has been developed. We use this model to evaluate the properties of the solar wind issuing from the open polar coronal hole regions of the Sun, during solar minimum. We explore the variation of solar wind parameters across the extent of the hole and we investigate how these variations are affected by the geometry of the hole and the strength of the field at the coronal base.
    Keywords: Solar Physics
    Type: ; 65
    Format: text
    Location Call Number Expected Availability
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    NASA TECHNICAL REPORTS
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