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タイトルEntropy Generation Across Earth's Bow Shock
本文(外部サイト)http://hdl.handle.net/2060/20120002025
著者(英)McCarthy, Michael; Wilber, Mark; Fu, Suiyan; Lee E. s; Cao, Jinbin; Lin, Naiguo; Goldstein, Melvyn L.; Parks, George K.; Canu, Patrick; Reme, Henri; Dandouras, Iannis S.; Fazakerley, Andrew
著者所属(英)NASA Goddard Space Flight Center
発行日2011-12-04
言語eng
内容記述Earth's bow shock is a transition layer that causes an irreversible change in the state of plasma that is stationary in time. Theories predict entropy increases across the bow shock but entropy has never been directly measured. Cluster and Double Star plasma experiments measure 3D plasma distributions upstream and downstream of the bow shock that allow calculation of Boltzmann's entropy function H and his famous H-theorem, dH/dt ~ O. We present the first direct measurements of entropy density changes across Earth's bow shock. We will show that this entropy generation may be part of the processes that produce the non-thermal plasma distributions is consistent with a kinetic entropy flux model derived from the collisionless Boltzmann equation, giving strong support that solar wind's total entropy across the bow shock remains unchanged. As far as we know, our results are not explained by any existing shock models and should be of interests to theorists.
NASA分類Geophysics
レポートNOSH53B-2052
GSFC.ABS.5717.2011
権利Copyright, Distribution as joint owner in the copyright


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