Physical Conditions in a CME from Hinode, STEREO, and SOHO Observations

Details Physical Conditions in a CME from Hinode, STEREO, and SOHO Observations Physical Conditions in a CME from Hinode, STEREO, and SOHO Observations

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..428..201l&link_type=abstract

SOHO-23: Understanding a Peculiar Solar Minimum ASP Conference Series Vol. 428, proceedings of a workshop held 21-25 September 2

Astronomy and Astrophysics

Astronomy

Scientific paper

In the present work we analyze multiwavelength observations from Hinode, SOHO, and STEREO of the early phases of a CME. We use EIS, UVCS, and XRT to measure the physical properties of the CME ejecta as a function of time at 1.1 and 1.9 Rsun. EUVI, COR 1, EIT, and LASCO images are used to measure the CME trajectory, velocity, and acceleration in 3D up to 5 Rsun. The diagnostic results are used to determine the energy budget of the CME plasma and the heating rate, and to compare it to theoretical predictions.

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