A model for X-ray emission from loop prominences |
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Authors: | K J H Phillips J B Zirker |
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Institution: | (1) Institute for Astronomy, University of Hawaii, Honolulu, HI |
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Abstract: | A study is made of X-ray line emission observed during the developing stages of a set of post-flare loop prominences. The time behaviour of the line emission can be described by a model consisting of two flux tubes containing plasma heated impulsively at the flash phase; the plasma cools by radiation and by conduction to the chromosphere. These ideas are extended to the possible formation of H prominences from low-lying hot loops. |
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