Solar Wind Parameters for Magnetic Field Modeling

Details Solar Wind Parameters for Magnetic Field Modeling Solar Wind Parameters for Magnetic Field Modeling

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsm41d..01q&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SM41D-01

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Applications

2723 Magnetic Reconnection (7526, 7835), 2730 Magnetosphere: Inner, 2731 Magnetosphere: Outer, 2740 Magnetospheric Configuration And Dynamics, 2784 Solar Wind/Magnetosphere Interactions

Scientific paper

The magnetic field models are crucial for many space weather applications. Yet the latest Tsyganenko model T04s [Tsyganenko and Sitnov,2005] requires 5-minute solar wind data that is not always available. We show that the hourly data from OMNIWEB can be used to calculate with sufficient accuracy the W parameters used in T04s model. We also present a system to interpolate the solar wind parameters across data gaps and to evaluate W parameters in these gaps. In this case, the resulting model input parameters are reasonable, thought not necessarily accurate values. We have created a database with solar wind parameters, G parameters and W parameters from 1963 to Sept 2005, which is sufficient for use in all the Tsyganenko models: T89 [Tsyganenko, 1989], T96 [Tsyganenko, 1996], T01[Tsyganenko, 2002ab], T01s [Tsyganenko et al., 2003], T04s.

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