SECCHI EUVI Observations

Details SECCHI EUVI Observations SECCHI EUVI Observations

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh52a..01n&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH52A-01

Physics

7509 Corona, 7513 Coronal Mass Ejections, 7549 Ultraviolet Emissions

Scientific paper

SECCHI EUVI will observe from multiple viewpoints the EUV emission line intensities of structures in the Transition Region and inner corona (<1.5Rsun) with a cadence comparable to the speed of a fast CME. This will address a number of key scientific issues related to the initiation of CMEs including 1) Determination of the three-dimensional coronal structure of pre/post CME regions (early mission), 2) Determination of the three-dimensional properties of the CME in the low corona (early mission), and 3) Determination of the relative timing between CME related structures (cavities, dimmings, waves, brightenings) involved in CME initiation from two angles (later mission).

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