An Estimation of Global p-mode Frequencies and Splittings from the IRIS Network Data: 1989–1996
Sh. A. EhgamberdievUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya-33, Tashkent-700052, UzbekistanA. SerebryanskiyUlugh Beg Astronomical Institute of the Uzbek Academy of Sciences, Astronomicheskaya-33, Tashkent-700052, UzbekistanS. KhalikovInstitute of Material Science, “Solnce”, Parkent-702226, UzbekistanE. FossatParc Valerose, F-06108 Nice Cedex, FranceB. GellyParc Valerose, F-06108 Nice Cedex, Francethe IRIS teem
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Annotatsiya
The IRIS network has accumulated low- l p -modes data since July, 1989, i.e. one complete solar cycle. Since the last publication of a frequency table (Gelly et al. 1997) the IRIS data bank was not only filled with new data, but also has been supplemented with data from other helioseismology instruments, through cooperative programs. The results of a new estimations of frequencies and splitting obtained from IRIS ++ data (Gelly et al. 1998) for period 1989-1996, as well as their variation along the solar magnetic activity cycle are presented.
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