Solar p modes in 10 years of the IRIS network

David Salabert, E Fossat, B Gelly, S Kholikov, G Greg, M Lazrek, FX Schmider

Research output: Contribution to journalArticle

31 Citations (Scopus)

Abstract

IRIS data ( the low degree l less than or equal to 3 helioseismology network) have been analysed for the study of p-mode parameters variability over the falling phase of the solar activity cycle 22 and the rising phase of the solar activity cycle 23. The IRIS duty cycle has been improved by the so-called "repetitive music method", a method of partial gap filling. We present in this paper an analysis of the dependence of p-mode frequencies and linewidths with frequency and with solar magnetic activity. We confirm also the periodicity of about 70 muHz of the high-frequency pseudo modes, with a much reduced visibility during the phase of higher activity.
Original languageEnglish
Pages (from-to)1135-1142
Number of pages8
JournalAstronomy and Astrophysics
Volume413
DOIs
Publication statusPublished - 1 Jan 2004

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