Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh13b1553l&link_type=abstract
American Geophysical Union, Fall Meeting 2008, abstract #SH13B-1553
Physics
2101 Coronal Mass Ejections (7513), 2111 Ejecta, Driver Gases, And Magnetic Clouds, 2134 Interplanetary Magnetic Fields, 2139 Interplanetary Shocks
Scientific paper
Since the launch of STEREO in November 2006, continuous white-light observations of solar transients on their way to the Earth have been made possible. STEREO/SECCHI observations have also revealed the complexity and dynamic structure of the interplanetary medium. In this talk, we will discuss the significance of 3-D numerical simulations in the interpretation of observations taken by SECCHI. Our focus will be on a series of two ejections on January, 24-25, 2007, which have been simulated with the Space Weather Modeling Framework (SWMF). We will discuss the appearance of coronal mass ejections (CMEs) and dense streams in the Heliospheric Imagers' field-of-view. Detailed comparisons between the real and simulated time-elongation plots will be presented. We will also discuss how observations of CME-CME interaction can be distinguished from the interaction of CMEs with dense streams in the solar wind using the simulations.
Lugaz Noé
Roussev Ilia I.
Vourlidas Angelos
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