Physics – Plasma Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsh23b1858x&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SH23B-1858
Physics
Plasma Physics
[7513] Solar Physics, Astrophysics, And Astronomy / Coronal Mass Ejections, [7851] Space Plasma Physics / Shock Waves, [7954] Space Weather / Magnetic Storms, [7959] Space Weather / Models
Scientific paper
The 2010 April 03 and August 01 CMEs were studied using observations from STEREO A and B, and SOHO LASCO, combined with ENLIL+Cone model simulations preformed at the Community Coordinated Modelling Center (CCMC). In particular, we identified the origin of CMEs using STEREO EUVI and/or SDO images. A flux-rope model fitting to the SECCHI A and B, SOHO/LASCO images was used to reconstruct the 3D structures of CMEs and determine their actual speeds. J-maps were obtained from COR-2/HI-1/HI-2 and simulations using ENLIL+cone model were conducted to study the formation and evolution of the CME-driven shocks in the inner heliosphere. We compared the simulation results with the observed height-time profiles of the shocks from white light and kilometric type II burst (Wind/WAVES) observations. The predicted shock arrival at Earth is compared with in-situ observations from ACE and Wind. We report the preliminary results of the study in this poster.
Cremades H.
Gopalswamy Nat
Mays L.
Odstrcil Dusan
St Cyr O. C.
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