Mathematics – Logic
Scientific paper
Dec 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufmsm11a..05t&link_type=abstract
American Geophysical Union, Fall Meeting 2005, abstract #SM11A-05
Mathematics
Logic
2431 Ionosphere/Magnetosphere Interactions (2736), 2722 Forecasting (7924, 7964), 2753 Numerical Modeling, 2784 Solar Wind/Magnetosphere Interactions, 7513 Coronal Mass Ejections (2101)
Scientific paper
Space weather forecasting requires faster than real-time simulations of the entire Sun-to-Earth model chain at high enough spatial and temporal resolution to resolve the important geoeffective features in the solar wind and the magnetosphere-ionosphere-thermosphere system. We present a complete end-to-end simulation of one of the most intensive solar storms, the October 28, 2003 CME. The physical domain models spanning from the Solar Corona model to the Upper Atmosphere model are self-consistently coupled together by the high-performance Space Weather Modeling Framework (SWMF). We discuss technological advances enabling the faster than real-time operation of the SWMF with high resolution. We also compare the simulation results with observations.
de Zeeuw Darren L.
Gombosi Tamas I.
Manchester Ward B.
Ridley Aaron J.
Roussev Ilia I.
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