Physics
Scientific paper
May 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agusmsh53a..03m&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH53A-03
Physics
7924 Forecasting (2722), 7959 Models, 7974 Solar Effects
Scientific paper
The CCMC currently hosts a number of different MHD and semi-empirical models of the corona and heliosphere, and is running many of them in a daily operational mode. We have three different coupled models, MAS+ENLIL, Wang/Sheeley/Arge+ENLIL, and the SWMF Corona + SWMF Heliosphere. We report here on the configuration of these models at the CCMC, and on our ongoing comparative studies of their results. In particular we focus on issues relating to the tracing of fieldlines from the four inner planets, back to open field regions on the solar surface. We have developed a suite of graphical quick-look images and movies for each model combination, some of which are presented here. Each model combination is also available, through our Run-on-Request facility, to users wishing to create models of past Carrington rotations using archived synoptic magnetogram data. In addition we are now providing selected daily model runs out to 10AU in support of the Cassini Magnetospheres Working Group, and also presenting a web page by which STEREO observers can access our entire archive of daily runs.
Arge N.
Hesse Matthias
MacNeice Peter J.
Odstrcil Dusan
Rastaetter Lutz
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