Studying Transition Region Phenomena with Solar-B/EIS
Abstract
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.
- Publication:
-
New Solar Physics with Solar-B Mission
- Pub Date:
- October 2007
- DOI:
- 10.48550/arXiv.0708.1672
- arXiv:
- arXiv:0708.1672
- Bibcode:
- 2007ASPC..369..307Y
- Keywords:
-
- Astrophysics
- E-Print:
- 4 pages, 3 figures, to appear in ASP Conf. Ser. 369, New Solar Physics with the Solar-B Mission