Near-lunar proton velocity distribution explained by electrostatic acceleration
The observation of parallel ion velocity in the near-lunar wake approximately equal to external solar wind velocity can be explained within uncertainties by an analytic electrostatic expansion model. The one-dimensional model frequently used is inadequate because it does not account for the moon...
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| Format: | Article |
| Language: | en_US |
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American Geophysical Union (AGU)
2015
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| Online Access: | http://hdl.handle.net/1721.1/95829 |
| Summary: | The observation of parallel ion velocity in the near-lunar wake approximately equal to external solar wind velocity can be explained within uncertainties by an analytic electrostatic expansion model. The one-dimensional model frequently used is inadequate because it does not account for the moon's spherical shape. However, application of a more recent generalization to three dimensions of the solution along characteristics predicts higher velocities and is probably sufficient to account for the SARA observations on the Chandrayaan-1 spacecraft. |
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