Formation of Fast shocks by magnetic reconnection in the Solar corona
碩士 === 國立成功大學 === 物理學系碩博士班 === 93 === The fast shocks generated by magnetic reconnection can explain recent SOHO observations of the heating and acceleration of protons and heavier ions in the solar corona (Lee and Wu, 2000). The magnetic reconnection over the solar surface is expected to generate a...
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| Format: | Others |
| Language: | zh-TW |
| Published: |
2005
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| Online Access: | http://ndltd.ncl.edu.tw/handle/73481270034817684794 |