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Interaction of turbulent solar with with cometary plasma tails

โœ Scribed by B. Buti


Publisher
Springer Netherlands
Year
1982
Tongue
English
Weight
349 KB
Volume
85
Category
Article
ISSN
0004-640X

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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