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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4087
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dc.contributor.authorDas, G. C-
dc.date.accessioned2008-12-16T14:58:01Z-
dc.date.available2008-12-16T14:58:01Z-
dc.date.issued1981-06-
dc.identifier.citationSolar Physics, Vol. 71, No. 2, pp. 215 - 221en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/4087-
dc.descriptionOpen Access-
dc.description.abstractMathematical 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.isoenen
dc.publisherD.Reidel Publishing Co.,en
dc.relation.urihttp://www.springerlink.com/content/k53mvn7143l6266k/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1981SoPh...71..215Den
dc.rightsD.Reidel Publishing Co.,-
dc.subjectDampingen
dc.subjectMagnetohydrodynamic Wavesen
dc.subjectMathematical Modelsen
dc.subjectSolar Oscillationsen
dc.subjectSolar Rotationen
dc.subjectWave Propagationen
dc.subjectCoriolis Effecten
dc.subjectIonized Gasesen
dc.subjectParticle Motionen
dc.subjectPlane Wavesen
dc.subjectRotating Fluidsen
dc.subjectSolar Magnetic Fielden
dc.titleCharacteristics of damping of the pulses in the sunen
dc.typeArticleen
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