Physics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh31a0223o&link_type=abstract
American Geophysical Union, Fall Meeting 2007, abstract #SH31A-0223
Physics
7509 Corona, 7513 Coronal Mass Ejections (2101)
Scientific paper
We use raytracing software to simulate white light coronagraph images of common 3D shock-like geometries, i.e. spherical and bow-shock type. We obtain the density profiles for different projections, shock thickness, and background and upstream densities. The results are compared to density profiles obtained from analyzing LASCO coronagraph images of CMEs that are good candidates to drive a shock due to their high velocities (V>1500 km/s). This work is funded by the LWS TR&T program.
Ontiveros Veronica
Vourlidas Angelos
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