Study of CME Related Phenomena Using STEREO/EUVI Data

Details Study of CME Related Phenomena Using STEREO/EUVI Data Study of CME Related Phenomena Using STEREO/EUVI Data

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agusmsh41a..08r&link_type=abstract

American Geophysical Union, Spring Meeting 2007, abstract #SH41A-08

Physics

7509 Corona, 7513 Coronal Mass Ejections (2101), 7974 Solar Effects

Scientific paper

The main goal of the STEREO mission is to address the three-dimensional structure of the Sun's corona, with emphasis in the origin and development of coronal mass ejections (CMEs). SECCHI/EUVI, the extreme ultraviolet imager onboard STEREO, provides full Sun coverage with improved cadence and spatial resolution with respect to SOHO/EIT. This allows an improved study of CME signatures in EUV. The present work provides an insight analysis of CME related phenomena in the EUV, such as filaments and post-eruptive arcades. By combining simultaneous images from both spacecraft, information on the 3D configuration of the solar structures can be obtained. The identification of the same feature in both images and the calculation of the displacement between them (parallax) are used to obtain the height of the structures seen in EUV images.

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