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Structure of the lunar wake: Two‐dimensional global hybrid simulations
Author(s) -
Trávníček Pavel,
Hellinger Petr,
Schriver David,
Bale Stuart D.
Publication year - 2005
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2004gl022243
Subject(s) - wake , physics , solar wind , turbulence , geophysics , magnetopause , computational physics , coronal mass ejection , interplanetary spaceflight , plasma , atmospheric sciences , astrophysics , mechanics , quantum mechanics
We study the structure and properties of the lunar wake with these solar wind parameters: the angle θ sw between directions of the solar wind velocity v sw and the ambient interplanetary magnetic field (IMF) B θ sw = 45° and 90° and v sw = 6 v A (where v A denotes solar wind Alfvén velocity). We examine the structure of the wake‐tail formed behind the obstacle. In agreement with in situ observations the lunar wake is formed by two counterstreaming beams which fill the wake with a relatively cold, inhomogeneous and highly anisotropic plasma. The results of this study suggest that for given solar wind conditions the downstream region of the lunar wake is dominated by electromagnetic turbulence with the frequencies near the local proton gyrofrequency. The properties and possible generating mechanisms of the low‐frequency electromagnetic turbulence are discussed.