Relationships between the IMF and the Two-cell Aurora
碩士 === 國立中央大學 === 太空科學研究所 === 94 === The main feature of the two-cell aurora is azimuthally elongated over at least four hours of local time on both the duskside and dawnside. The two-cell aurora is believed to be associated with a convection enhancement caused by southward interplanetary magnetic f...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2006
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| Online Access: | http://ndltd.ncl.edu.tw/handle/h2d85k |