Characteristics of damping of the pulses in the sun

dc.contributor.author	Das, G. C
dc.date.accessioned	2008-12-16T14:58:01Z
dc.date.available	2008-12-16T14:58:01Z
dc.date.issued	1981-06
dc.identifier.citation	Solar Physics, Vol. 71, No. 2, pp. 215 - 221	en
dc.identifier.issn	0038-0938
dc.identifier.uri	http://hdl.handle.net/2248/4087
dc.description	Open Access
dc.description.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.	en
dc.language.iso	en	en
dc.publisher	D.Reidel Publishing Co.,	en
dc.relation.uri	http://www.springerlink.com/content/k53mvn7143l6266k/	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1981SoPh...71..215D	en
dc.rights	D.Reidel Publishing Co.,
dc.subject	Damping	en
dc.subject	Magnetohydrodynamic Waves	en
dc.subject	Mathematical Models	en
dc.subject	Solar Oscillations	en
dc.subject	Solar Rotation	en
dc.subject	Wave Propagation	en
dc.subject	Coriolis Effect	en
dc.subject	Ionized Gases	en
dc.subject	Particle Motion	en
dc.subject	Plane Waves	en
dc.subject	Rotating Fluids	en
dc.subject	Solar Magnetic Field	en
dc.title	Characteristics of damping of the pulses in the sun	en
dc.type	Article	en