Characteristics of damping of the pulses in the sun

Details Characteristics of damping of the pulses in the sun Characteristics of damping of the pulses in the sun

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...71..215d&link_type=abstract

Solar Physics, vol. 71, June 1981, p. 215-221. Research supported by the Council of Scientific and Industrial Research of India.

Physics

Damping, Magnetohydrodynamic Waves, Mathematical Models, Solar Oscillations, Solar Rotation, Wave Propagation, Coriolis Effect, Ionized Gases, Particle Motion, Plane Waves, Rotating Fluids, Solar Magnetic Field

Scientific paper

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.

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