Results 271 to 280 of about 505,915 (296)
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Advances in Space Research, 2014
Abstract It is clear that the primary energy source for magnetospheric processes is the solar wind, but the process of energy transfer from the solar wind into the magnetosphere, or rather, to convecting magnetospheric plasma, appears to be rather complicated.
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Abstract It is clear that the primary energy source for magnetospheric processes is the solar wind, but the process of energy transfer from the solar wind into the magnetosphere, or rather, to convecting magnetospheric plasma, appears to be rather complicated.
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Statistics of bow shock nonuniformity
Journal of Geophysical Research, 1973The statistical occurrence of pulsation or oblique structure about the earth's generally nonuniform bow shock is estimated at selected points by combining a three-dimensional distribution of interplanetary field directions obtained for a six-day solar wind sector with an index of local pulsation geometry. The result, obtained with a pulsation index of
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Initial Venus Express magnetic field observations of the Venus bow shock location at solar minimum
Planetary and Space Science, 2008Wolfgang Baumjohann +2 more
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Statistical Survey of the Terrestrial Bow Shock Observed by the Cluster Spacecraft
Journal of Geophysical Research: Space Physics, 2019Milan Maksimovic +2 more
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Average and unusual locations of the Earth's magnetopause and bow shock
Journal of Geophysical Research, 1971Donald H Fairfield
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The Martian Bow Shock Over Solar Cycle 23–24 as Observed by the Mars Express Mission
Journal of Geophysical Research: Space Physics, 2019Mats Holmström +2 more
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Dynamic motion of the bow shock and the magnetopause observed by THEMIS spacecraft
Journal of Geophysical Research: Space Physics, 2009Davin Larson, Hui Zhang, David G. Sibeck
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