Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh51c1693r&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SH51C-1693
Astronomy and Astrophysics
Astrophysics
[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7924] Space Weather / Forecasting
Scientific paper
We present the results from an attempt to merge in-situ magnetic cloud reconstruction techniques with white light heliospheric imager 3-D reconstruction techniques. This has been accomplished to serve two purposes: 1) to identify which features of interplanetary coronal mass ejections (ICMEs) are most prominent in heliospheric imagers; 2) to set some standards from which scientific revelations about ICMEs may be achieved. We combine the magnetic cloud model of Romashets et al. (A&A, 2007) with the elliptical force-free solution (Vandas & Romashets, A&A, 2003) and the recently-developed Tappin-Howard (TH) model (Tappin & Howard, SSR, 2009) for heliospheric imager ICMEs. Along with an analysis of the kinematic evolution of the CME we compare the 3-D structures of each of the features in the heliospheric imagers with those of the magnetic cloud.
Howard Tim
Romashets Eugene
Vandas Marek
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