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Low frequency signal in the GOLF measurements

Authors :
Gérard Grec
Janine Provost
C. Renaud
Laboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides (CASSIOPEE)
Université Nice Sophia Antipolis (... - 2019) (UNS)
COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de la Côte d'Azur
Université Côte d'Azur (UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Université Côte d'Azur (UCA)-Centre National de la Recherche Scientifique (CNRS)
Source :
Journal of Physics: Conference Series, Journal of Physics: Conference Series, IOP Publishing, 2011, 271, pp.2050. ⟨10.1088/1742-6596/271/1/012050⟩
Publication Year :
2011
Publisher :
HAL CCSD, 2011.

Abstract

This paper shows the results obtained using a revisited method to normalize the velocity evaluation extracted from the measurements, for roughly 14 years of GOLF data. For the search of g modes, we calculate the low frequency power spectrum of the signal with 2 different approaches: • The classical calculation of the power spectrum of the velocity signal. • An alternative calculation, extracting first the variations along the time of the p-mode frequencies, then calculating the power spectrum of those frequency modulation [4]. Both spectra are compared to the g-mode frequency spectrum calculated for a solar model. Several observed frequencies are in close agreement with the calculated g modes. A careful statistical analysis of this result should now follow.

Details

Language :
English
ISSN :
17426588 and 17426596
Database :
OpenAIRE
Journal :
Journal of Physics: Conference Series, Journal of Physics: Conference Series, IOP Publishing, 2011, 271, pp.2050. ⟨10.1088/1742-6596/271/1/012050⟩
Accession number :
edsair.doi.dedup.....480410c5a466a4aebdf9cd5bfaa2ee0d
Full Text :
https://doi.org/10.1088/1742-6596/271/1/012050⟩