PHYSICAL PROPERTIES OF COOLING PLASMA IN QUIESCENT ACTIVE REGION LOOPS

In the present work, we use SOHO/SUMER, SOHO/UVCS, SOHO/EIT, SOHO/LASCO, STEREO/EUVI, and Hinode/EIS coordinated observations of an active region (AR 10989) at the west limb taken on 2008 April 8 to study the cooling of coronal loops. The cooling plasma is identified using the intensities of SUMER s...

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Bibliographic Details
Published inThe Astrophysical journal Vol. 695; no. 1
Main Authors Landi, E., Miralles, M. P., Curdt, W., Hara, H.
Format Journal Article
LanguageEnglish
Published United States 10.04.2009
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