Studying Transition Region Phenomena with Solar-B/EIS

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dc.creatorYoung, P. R.
dc.date2007-08-13
dc.date.accessioned2026-07-07T08:23:23Z
dc.date.available2026-07-07T08:23:23Z
dc.descriptionTransition 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.
dc.description4 pages, 3 figures, to appear in ASP Conf. Ser. 369, New Solar Physics with the Solar-B Mission
dc.identifierhttps://arxiv.org/abs/0708.1672
dc.identifierhttp://arxiv.org/abs/0708.1672
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/135978
dc.subjectAstrophysics
dc.titleStudying Transition Region Phenomena with Solar-B/EIS
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