Studying Transition Region Phenomena with Solar-B/EIS

P. R. Young

Studying Transition Region Phenomena with Solar-B/EIS

Astrophysics 2007-08-14 v1

Authors: P. R. Young

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.

Keywords

solar physics atomic spectroscopy

Cite

@article{arxiv.0708.1672,
  title  = {Studying Transition Region Phenomena with Solar-B/EIS},
  author = {P. R. Young},
  journal= {arXiv preprint arXiv:0708.1672},
  year   = {2007}
}

Comments

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

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