ULF waves in solar wind high speed streams influence on the magnetosphere

Details ULF waves in solar wind high speed streams influence on the magnetosphere ULF waves in solar wind high speed streams influence on the magnetosphere

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsm51b..02k&link_type=abstract

American Geophysical Union, Spring Meeting 2002, abstract #SM51B-02

Physics

2772 Plasma Waves And Instabilities, 2784 Solar Wind/Magnetosphere Interactions, 2154 Planetary Bow Shocks

Scientific paper

We show a new correlation between high speed streams in 1995 and ULF waves (Pc5 range) upstream from Earth's bow shock. These ULF waves occur in the compression region at the leading and trailing edges of high speed streams, and are further enhanced through interaction with the quasi-parallel bow shock. We compare our new correlation to a closely similar correlation between high speed streams and Pc5 pulsations in the magnetosphere. This comparison suggests a physical relation that may be the result of a direct transmission during times of nearly radial IMF or a perturbation driving magnetopause displacements.

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