Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh52a..02k&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SH52A-02
Physics
2111 Ejecta, Driver Gases, And Magnetic Clouds, 7513 Coronal Mass Ejections
Scientific paper
Driven by modern space-based solar and solar-wind observations, three-dimensional (3D) models of coronal mass ejections (CMEs), both numerical magnetohydrodynamic[1-4] and semi-analytical[5-7], have produced many exciting results. From among the current avenues of model-driven CME research, we shall highlight two areas where STEREO data might be expected to have a significant impact: 1) the near-sun geometrical relationship between the CME, the embedded prominence, and the underlying magnetic structure, and 2) the morphology and dynamics of erupting flux-ropes in the interplanetary medium, especially halo CMEs. We shall discuss the expected impact of STEREO data on "state of the art", model-driven CME research. Supported by ONR and NASA [1] Roussev et al. 2003, ApJ, 588, L45 [2] Amari et al. 2003, ApJ, 595, 1231 [3] Lynch et al. 2004, ApJ, 617, 589 [4] Manchester et al. 2004, JGR, 109, doi:10.1029/2003JA010150 [5] Chen 1996, JGR, 101, 27499 [6] Gibson and Low 2000, JGR, 105, 18187 [7] Chen and Krall 2003, JGR, 108, doi:10.1029/2003JA009849
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