The Solar Wind in the Outer Heliosphere: Physical Processes in the Termination Shock and Heliosheath
The solar wind evolves as it moves outward due to interactions with both itself and with the circum-heliospheric interstellar medium. The speed is, on average, constant out to 30 AU, then starts a slow decrease due to the pickup of interstellar neutrals. These neutrals reduce the solar wind speed by...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Article |
| Language: | English |
| Published: |
Springer Netherlands,
2009-10-19T13:01:15Z.
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| Subjects: | |
| Online Access: | Get fulltext |