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.
