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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4087
Title: Characteristics of damping of the pulses in the sun
Authors: Das, G. C
Keywords: Damping
Magnetohydrodynamic Waves
Mathematical Models
Solar Oscillations
Solar Rotation
Wave Propagation
Coriolis Effect
Ionized Gases
Particle Motion
Plane Waves
Rotating Fluids
Solar Magnetic Field
Issue Date: Jun-1981
Publisher: D.Reidel Publishing Co.,
Citation: Solar Physics, Vol. 71, No. 2, pp. 215 - 221
Abstract: Mathematical modelling is used in determining the rotational frequency and the density of an ionized medium. It is noted that the technique derives from the measurement of the group travel time for a wave propagating in a rotating ionized medium, and finally a simple approximate formula determines the rotation and the density of the medium. A calculation is made of the damping of the pulse-waves in the rotating sun and there is a mathematical development to estimate more physical parameters of the solar system.
Description: Open Access
URI: http://hdl.handle.net/2248/4087
ISSN: 0038-0938
Appears in Collections:IIAP Publications

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