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- W1569842921 abstract "The dissipation depths of Alfven and sound waves in the magnetic structure of the solar chromosphere and corona are obtained with allowance for the decay process and nonlinear phase advance in Alfven and sound waves. In the calculations it was assumed that energy balance occurs in each volume element: The amount of wave energy epsilon/sub dis/ dissipated here is equal to the emission power epsilon/sub emis/. The calculations were made for three mechanisms of losses to emission, namely, in accordance with a) a given population of the second level, b) a Boltzmann distribution by levels, and c) emission at high temperatures in accordance with the results of (D. P. Cox and W. H. Tucker, Astrophys. J. 157, 1157 (1969)). The depths are given in Table I. Sound waves dissipate rapidly both in the chromosphere and in the corona. Under certain conditions, which can be estimated from Eqs. (17) -(19), taking phi/..pi.. and ..mu.. on the order of unity there, Alfven waves penetrate to greater heights, and at the same time the dissipation of these waves in magnetic tubes is still sufficient for the heating." @default.
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- W1569842921 date "1977-09-01" @default.
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- W1569842921 title "Dissipation of convective noise waves in the magnetic structure of the upper layers of the solar atmosphere" @default.
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