Results from the LOWL instrument

dc.contributor.author	Schou, J
dc.contributor.author	Tomczyk, S
dc.contributor.author	Thompson, M. J
dc.date.accessioned	2007-09-25T10:10:37Z
dc.date.available	2007-09-25T10:10:37Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 2 pp. 375-378	en
dc.identifier.uri	http://hdl.handle.net/2248/1826
dc.description.abstract	We present various results from one year of observations with the LOWL instrument, which is designed to observe oscillations with degrees l from 0 to about 100. Among the results shown is an inversion for the solar rotaion rate down to approximately 0.2R, Given the long duration of the observations we have been able to obtain very low errors and good radial and latitude resolution in a substantial part of the solar interior. We will also present results of analyzing different parts of the time-series to look for temporal variations in mode frequencies and show that they seem to be associated with variations in solar activity.	en
dc.format.extent	353978 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/1996BASI...24..375S	en
dc.subject	Sun:rotation	en
dc.subject	Activity	en
dc.subject	Inversions	en
dc.title	Results from the LOWL instrument	en
dc.type	Article	en