On the p-mode Asymmetry between Velocity and Intensity from the GONG+ Data

dc.contributor.author	Tripathy, S. C
dc.contributor.author	Jain, K
dc.contributor.author	Hill, F
dc.contributor.author	Toner, C. G
dc.date.accessioned	2008-06-05T09:59:30Z
dc.date.available	2008-06-05T09:59:30Z
dc.date.issued	2003
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 321 - 323	en
dc.identifier.uri	http://hdl.handle.net/2248/2406
dc.description.abstract	We have analyzed the local acoustic spectra of small regions over the solar surface at different locations from disk center to limb via the technique of ring diagrams. The analysis suggest that the frequency shifts between velocity and intensity is a function of location on the disk and is higher near the disk center than those near the limb.	en
dc.format.extent	90266 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..321T	en
dc.subject	Solar oscillation	en
dc.subject	Intensity	en
dc.subject	GONG+	en
dc.title	On the p-mode Asymmetry between Velocity and Intensity from the GONG+ Data	en
dc.type	Article	en