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- W1531620138 abstract "Preliminary results of applying a model of canopy-type magnetic lines to account for observed mass fluxes in the chromosphere and transiton region are presented. A set of center-to-limb data obtained in H-alpha and C IV, and to which the model is applied, is reported. The C IV line is assumed to form everywhere at the same height, and the H-alpha formation height is derived by assuming that the absorption coefficient is proportional to the local density. The density ratio between H-alpha and C IV levels is taken to be 100. From the results, it is concluded that the model accounts for the low ratio of radial velocities C IV/H-alpha at r = 0, the increase of H-alpha velocity near the limb, and the general center-to-limb behavior in both lines." @default.
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- W1531620138 date "1985-01-01" @default.
- W1531620138 modified "2023-10-16" @default.
- W1531620138 title "Mass fluxes and magnetic structures in the chromosphere and the transition region - Canopies" @default.
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