Abstract
view Abstract Citations (60) References (7) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The dissipation of hydromagnetic surface waves. Wentzel, D. G. Abstract When hydromagnetic surface waves travel along a surface with a thin but finite boundary layer, velocities within this layer become singular when computed according to the ideal MHD equations. The present paper computes the corresponding rate of wave damping. Sufficiently weak surface waves are dissipated either by a resonant conversion into kinetic Alfven waves or by viscosity. Astrophysically important surface waves may involve such large velocity amplitudes outside the narrow zone of linear dissipation that nonlinear phenomena limit the singularity and the method of dissipation. Even these, however, are confined to extremely narrow layers. Publication: The Astrophysical Journal Pub Date: October 1979 DOI: 10.1086/157437 Bibcode: 1979ApJ...233..756W Keywords: Magnetohydrodynamic Waves; Solar Corona; Surface Waves; Wave Attenuation; Differential Equations; Rates (Per Time); Viscosity; Wave Equations; Solar Physics; Hydrodynamics; Magnetohydrodynamics; Plasma full text sources ADS |
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
