๐”– Bobbio Scriptorium
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On the long-tail solar wind electron velocity distribution

โœ Scribed by Michael F. Shlesinger; Michael A. Coplan


Publisher
Springer
Year
1988
Tongue
English
Weight
259 KB
Volume
52
Category
Article
ISSN
0022-4715

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Cometary tail rays are traces of the magnetic fields caught in the cometary magnetosphere. Time variations of these rays give us a way to measure the local solar wind velocity at the location of a comet. We introduce a simple method for determining the radial velocity of the solar wind by observing