3-D simulations of ICMEs by coupled coronal and heliospheric models

Details 3-D simulations of ICMEs by coupled coronal and heliospheric models 3-D simulations of ICMEs by coupled coronal and heliospheric models

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.535..541o&link_type=abstract

In: Solar variability as an input to the Earth's environment. International Solar Cycle Studies (ISCS) Symposium, 23 - 28 June 2

Physics

4

Coronal Mass Ejection, Magnetic Flux Rope, Solar Wind, Interplanetary Shock, Magnetohydrodynamic Model, Numerical Simulation

Scientific paper

We overview the main features and approximations of the heliospheric modeling system based on a 3-D ideal magnetohydrodynamic (MHD) model that can be driven by various analytic, empirical, and numerical models of the solar corona. Results are presented for two different self-consistent simulations of Sun-to-Earth transient events: (1) propagation of an interplanetary magnetic flux rope driven by the 3-D MHD coronal model; and (2) the May 12-15, 1997 interplantary event driven by an empirical model of the ambient solar wind and fitted parameters for the halo coronal mass ejection (CME).

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