Three-dimensional ENLIL MHD model simulations of the HCS: Cassini and Ulysses comparison

Details Three-dimensional ENLIL MHD model simulations of the HCS: Cassini and Ulysses comparison Three-dimensional ENLIL MHD model simulations of the HCS: Cassini and Ulysses comparison

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsh31a..06e&link_type=abstract

American Geophysical Union, Spring Meeting 2008, abstract #SH31A-06

Physics

2134 Interplanetary Magnetic Fields, 2139 Interplanetary Shocks

Scientific paper

We compare results from the NOAA/ENLIL solar wind MHD model with Cassini and Ulysses observations of the heliospheric current sheet (HCS) on January 26-28 2004 when Cassini was just upstream of Saturn at 8.8 AU. Ulysses was near Jupiter at 5.3 AU about 6.25 days prior to the Cassini HCS observations and it likely observed the same HCS feature. We focus our attention on the azimuthal BT component of the IMF and the solar wind speed.

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