Modeling the Solar Terrestrial Environment from the Corona to the Atmosphere

Details Modeling the Solar Terrestrial Environment from the Corona to the Atmosphere Modeling the Solar Terrestrial Environment from the Corona to the Atmosphere

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsm22b..06g&link_type=abstract

American Geophysical Union, Spring Meeting 2002, abstract #SM22B-06

Astronomy and Astrophysics

Astrophysics

2700 Magnetospheric Physics, 7500 Solar Physics, Astrophysics, And Astronomy, 2100 Interplanetary Physics, 2400 Ionosphere

Scientific paper

Traditionally, numerical modeling has focused on distinct regions of the Solar Terrestrial Environment such as the corona, magnetosphere, or ionosphere/thermosphere (ITM). More recently several efforts have begun to model this closely coupled system through linking the regional codes together. We discuss here from the perspective of our project the characteristics of the individual codes, which 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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