A&A 374, 1100-1107 (2001)
DOI: 10.1051/0004-6361:20010780
Spectral analysis of solar diameter measurements recorded at Calern Observatory astrolabe during two solar cycles
R. Moussaoui1, A. Irbah1, E. Fossat2, J. Borgnino2, F. Laclare3, C. Delmas3 and F. X. Schmider21 CRAAG - Observatoire d'Alger, BP 63, Bouzaréah, Alger, Algeria
e-mail: irbah@unice.fr
2 Université de Nice-Sophia Antipolis, UMR n
3 Observatoire de la Côte d'Azur, Département CERGA, Avenue Copernic, 06130 Grasse, France
(Received 31 January 2000 / Accepted 3 May 2001 )
Abstract
Solar diameter measurements performed with the Calern Observatory astrolabe (O.C.A -
France) during more than two solar cycles show temporal variations. Due to the weather, seasonal
effects and instrumental characteristics, recorded solar data are non uniformly sampled and present
temporal gaps. Thus, to analyze these data, diameter measurements averaged over one or more months
have generally been considered. This limits the accessible harmonic terms to a low frequency range.
To determine short-term periodicities from the observed variations, all daily solar data need to be
considered and also corrected from the zenithal distance. In the present work, we use two methods
to analyze solar diameter measurements recorded at Calern Observatory astrolabe during the
observation period 1975-1996. They are based on least square fits and deconvolution of the
observation window function. Results deduced from the analysis confirm harmonic terms already found
by other authors but also reveal new higher frequencies.
Key words: Sun: fundamental parameters -- Sun: oscillations -- methods: data analysis
Offprint request: J. Borgnino, borgnino@unice.fr
© ESO 2001

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