Numerical simulation of interplanetary disturbances

Details Numerical simulation of interplanetary disturbances Numerical simulation of interplanetary disturbances

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477..281o&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Statistics

Computation

3

Solar Wind, Coronal Mass Ejections, Interplanetary Shocks, Numerical Simulations, Space Weather

Scientific paper

Improved understanding of the propagation of solar wind disturbances is needed to support space weather research and forecasting. Essential to this effort is a computational model capable of simulating the propagation, evolution, and interaction of transient disturbances on their way to Earth. An overview of the ongoing effort performed at the NOAA Space Environment Center is presented with examples illustrating: (a) global 3-D interaction of a CME propagating in structured background solar wind, (b) incorporation of a more realistic ambient solar wind, (c) merging of coronal and heliospheric models to track CMEs, and (d) high-resolution AMR simulation of magnetic cloud interactions.

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