Elongation and Separation of Flare Ribbons by Using SDO/AIA
碩士 === 國立中央大學 === 太空科學研究所 === 106 === The flare ribbon structure seen in ultraviolet images can be either caused by the flare-accelerated particles impacting on the lower solar atmosphere or related to the thermal conduction. Besides the separation between two ribbons expected by the CSHKP model, th...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2018
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| Online Access: | http://ndltd.ncl.edu.tw/handle/njjzr9 |