The Relationship Between Magnetosheath and Solar Wind Parameters

ORAL

Abstract

In general, solar wind drives magnetospheric activity and is used to quantify it. In reality, it is the magnetosheath which is in contact with the magnetosphere. Parameters in the magnetosheath therefore modulate magnetospheric activity. We expect that the relationship between solar wind and magnetosheath parameters will have a linear relationship at low solar wind magnetic field values. However, at high solar wind magnetic field values, the LFM Global MHD code predicts a non- linear relationship between the solar wind and magnetosheath parameters. Using simultaneous spacecraft observations from WIND and GEOTAIL, we examine several periods of low solar wind magnetic field and high solar wind magnetic field to confirm the observed relationship between the magnetosheath and solar wind magnetic fields and compare this to the LFM Global MHD code predictions.

*This material is based upon work supported by CISM, which is funded by the STC Program of the National Science Foundation under Agreement Number ATM-0120950

Authors

  • Crystal Red Eagle

    • UT Arlington
  • Phyllis Whittlesey

    • UT Arlington
  • Robert Allen

    • The University of Texas at Arlington
    • UT Arlington
  • Sophia Cockrell

    • UT Arlington
  • Elizabeth Mitchell

    • University of Texas at Arlington
    • UT Arlington
  • Ramon Lopez

    • UT Arlington
    • University of Texas at Arlington
    • The Department of Physics, the University of Texas at Arlington, USA