Studying Transition Region Phenomena with Solar-B/EIS

Details Studying Transition Region Phenomena with Solar-B/EIS Studying Transition Region Phenomena with Solar-B/EIS

2007-08-13

arxiv.org/abs/0708.1672v1

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, to appear in ASP Conf. Ser. 369, New Solar Physics with the Solar-B Mission

Scientific paper

Transition region lines in active regions can become strongly enhanced in
coronal footpoints and active region blinkers. The weak transition region lines
found in the Solar-B/EIS wavebands will thus become useful for diagnostic
studies of these events. EIS count rates predicted from SOHO/CDS spectra are
presented, and a Mg VII density diagnostic is highlighted.

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