The Roles and Needs of Models in the Future Solar-Terrestrial Data Environment

Details The Roles and Needs of Models in the Future Solar-Terrestrial Data Environment The Roles and Needs of Models in the Future Solar-Terrestrial Data Environment

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh52c..04g&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH52C-04

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2199 General Or Miscellaneous, 2447 Modeling And Forecasting, 2722 Forecasting, 7509 Corona, 7843 Numerical Simulation Studies

Scientific paper

We have recently embarked on two projects to model the Solar Terrestrial environment through linking the regional codes together. We discuss here, from the perspective of our projects, the characteristics of the individual codes. These are well known and respected in the SPA community: the SAIC corona code, the NCAR solar wind code, the LFM magnetosphere code, the Rice RCM, and NCAR ITM code (TING). We further discuss the issues important for coupling of these codes, and explore briefly the methods from the computational and computer sciences that may help address them.

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