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- W83084677 abstract "Abstract Nonlinear evolution and stability of the resonant absorption layer is considered by solving the time-dependent 3D, low-β, resistive MHD equations with the Lax-Wendroff explicit method. The calculations are initiated with the solutions of the linearized version of the MHD equations (Steinolfson and Davila, 1993, Ofman et al. , 1994), with inhomogeneous background density, and a constant magnetic field. The narrow resonant heating layers are deformed by the self-consistent shear flow. When the driver amplitude is small compared to the average Alfvén speed the dissipation layer appears to be stable and the driver-period-averaged ohmic heating rate saturates at a slightly higher than the linear rate. When the driver amplitude is large ( F d ≈ 1) the resonant heating may become unstable." @default.
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- W83084677 date "1994-01-01" @default.
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- W83084677 title "Coronal Heating by the Resonant Absorption of Alfvén Waves" @default.
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- W83084677 doi "https://doi.org/10.1017/s0252921100026725" @default.
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