Physics
Scientific paper
Dec 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufmsa51a..07c&link_type=abstract
American Geophysical Union, Fall Meeting 2006, abstract #SA51A-07
Physics
2431 Ionosphere/Magnetosphere Interactions (2736), 2447 Modeling And Forecasting, 2784 Solar Wind/Magnetosphere Interactions, 7509 Corona
Scientific paper
Real-time simulations executed 24 hours per day, 7 days per week are an essentail test of the robustness of both the input data retrieval and pre-processing software and of the models involved. Running a model continuously with real-time input data exposes the control software to problems such as bad data or data gaps and the model to unforseen challenges posed by extreme values in valid data. With the recent addition of automatic daily execution of solar coronal and heliospheric models, the Community-Coordinated Modeling Center (CCMC) now runs a full complement of models covering space from the solar corona all the way to the Earth's ionosphere. In this presentation we summarize what we are running, our experiences and which model combinations and alternative models for each region may be run in the near future.
Chulaki A.
Hesse Matthias
MacNeice Peter
Rastaetter Lutz
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