Interaction between the Solar Coronal Mass Ejections and Heliospheric Sector Boundary
碩士 === 國立中央大學 === 太空科學研究所 === 92 === Solar wind carries the frozen magnetic field from the solar surface into interplanetary space, making a shape of Archimedes spiral due to the rotation of the sun. The sector boundary is identified at the region when large scale polarity changes are located.Some s...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2004
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| Online Access: | http://ndltd.ncl.edu.tw/handle/73149790281290572460 |