Fast shock and Alfvén Waves Acceleration of Protons and Heliums：Formation of H+ / He++ Differential Streams in the Solar Wind
碩士 === 國立成功大學 === 物理學系碩博士班 === 94 === At 1AU, the high-speed solar wind has the following characteristics: (a) the velocity of high-speed solar wind is nearly 800km/s；(b)) the temperature of protons in the perpendicular direction to magnetic field is larger than in the parallel direction；(c) the num...
| Main Authors: | , |
|---|---|
| Other Authors: | |
| Format: | Others |
| Language: | zh-TW |
| Published: |
2006
|
| Online Access: | http://ndltd.ncl.edu.tw/handle/99302435137919510465 |