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The role of the inner tail to midtail plasma sheet in channeling solar wind power to the ionosphere

✍ Scribed by Hamrin, M. ;Marghitu, O. ;Norqvist, P. ;Buchert, S. ;André, M. ;Klecker, B. ;Kistler, L. M. ;Dandouras, I.


Book ID
111967164
Publisher
American Geophysical Union
Year
2012
Tongue
English
Weight
486 KB
Volume
117
Category
Article
ISSN
0148-0227

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A comparative study of the viscous transport of solar wind momentum to the upper layers of the Venus ionosphere with that occurring within the trans-terminator flow leads to estimates of the ratio of the viscosity coefficients that are applicable to both cases. Support for viscous forces between the