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Resonance absorption of Alfvén waves at comet‐solar wind interaction regions
Author(s) -
Sharma A. S.,
Cargill P. J.,
Papadopoulos K.
Publication year - 1988
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/gl015i008p00740
Subject(s) - solar wind , physics , comet , magnetohydrodynamics , absorption (acoustics) , computational physics , plasma , geophysics , comet tail , alfvén wave , astrophysics , atomic physics , optics , nuclear physics
The interaction of the low frequency (10 −2 Hz) MHD waves, observed upstream of comets, with the structured plasma near the cometary bow wave is examined. It is suggested that the waves undergo resonant absorption due to either ambient density gradients or localized shear in the background magnetic field. The absorption process can give rise to rapid heating of the solar wind protons, in agreement with observations from comet Halley. Since the free energy for the generation of MHD waves came from deceleration (without accompanying heating) of the solar wind protons during the pick up of cometary ions, the subsequent reabsorption of the energy is equivalent to a nonlocal transformation of ordered to random energy and can be described as nonlocal viscosity.