CME evolution and 3D reconstruction with STEREO Data

Details CME evolution and 3D reconstruction with STEREO Data CME evolution and 3D reconstruction with STEREO Data

Jun 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..274..165o&link_type=abstract

Advances in Plasma Astrophysics, Proceedings of the International Astronomical Union, IAU Symposium, Volume 274, p. 165-167

Astronomy and Astrophysics

Astrophysics

Sun: Coronal Mass Ejections (Cmes), Sun: Magnetic Fields

Scientific paper

We describe a CME event, occurred in NOAA 11059 on April 3 2010, using STEREO and MDI/SOHO data. We analyze the CME evolution using data provided by SECCHI-EUVI and COR1 onboard STEREO satellites, and we perform a 3D reconstruction of the CME using the LCT-TP method. Using MDI/SOHO line-of-sight magnetograms we analyze the magnetic configuration of NOAA 11059 and we determine the magnetic helicity trend.

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