Studying Transition Region Phenomena with Solar-B/EIS
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🌌 astro-ph
keywords
regiontransitionactivebecomediagnosticlinessolar-bblinkers
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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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