Towards an Operational Sun-to-Earth Model for Space Weather Forecasting

Details Towards an Operational Sun-to-Earth Model for Space Weather Forecasting Towards an Operational Sun-to-Earth Model for Space Weather Forecasting

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agusmsh51b..06g&link_type=abstract

American Geophysical Union, Spring Meeting 2002, abstract #SH51B-06

Physics

2740 Magnetospheric Configuration And Dynamics, 2753 Numerical Modeling, 2784 Solar Wind/Magnetosphere Interactions, 2788 Storms And Substorms

Scientific paper

We are presently developing a physics based, modular, large-scale model of the solar-terrestrial environment simulating space weather phenomena and providing a framework to test theories and explore the possibility of operational use in space weather forecasting. This talk will describe the main components of the model (a global MHD code, an upper atmosphere and ionosphere model, and the inner magnetosphere drift physics model). We will also discuss the testing and transitioning the model through CCMC to operational use by NOAA SEC and the Air Force. Particular attention will be paid to the need of validation and metrics studies.

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