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Bow shock: Power aspects

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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Statistics of bow shock nonuniformity

Journal of Geophysical Research, 1973
The 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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The bow shock. Preface

Il Nuovo Cimento C, 1979
J. Lemaire, M. J. Rycroft
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Bow Shocks at Comets

AIP Conference Proceedings, 2009
Andrew J. Coates   +2 more
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Initial Venus Express magnetic field observations of the Venus bow shock location at solar minimum

Planetary and Space Science, 2008
Wolfgang Baumjohann   +2 more
exaly  

Statistical Survey of the Terrestrial Bow Shock Observed by the Cluster Spacecraft

Journal of Geophysical Research: Space Physics, 2019
Milan Maksimovic   +2 more
exaly  

Average and unusual locations of the Earth's magnetopause and bow shock

Journal of Geophysical Research, 1971
Donald 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, 2019
Mats Holmström   +2 more
exaly  

Dynamic motion of the bow shock and the magnetopause observed by THEMIS spacecraft

Journal of Geophysical Research: Space Physics, 2009
Davin Larson, Hui Zhang, David G. Sibeck
exaly  

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