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Simulation of cometary jets in interaction with the solar wind

✍ Scribed by S. Wiehle; U. Motschmann; N. Gortsas; K.-H. Glassmeier; J. Müller; C. Koenders


Book ID
113471175
Publisher
Elsevier Science
Year
2011
Tongue
English
Weight
888 KB
Volume
48
Category
Article
ISSN
0273-1177

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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