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Variations of the solar granulation motions with height using the GOLFSoHO experiment.pdf

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Variations of the solar granulation motions with height using the GOLFSoHO experiment

a r X i v : 0 8 0 8 .0 4 2 2 v 1 [ a s t r o - p h ] 4 A u g 2 0 0 8 Astronomy Astrophysics manuscript no. ms15 c? ESO 2008 August 4, 2008 Variations of the solar granulation motions with height using the GOLF/SoHO experiment S. Lefebvre 1 , R. A. Garc??a 1 , S. J. Jime?nez-Reyes 2 , S. Turck-Chie?ze 1 , and S. Mathur 1,2 1 Laboratoire AIM, CEA/DSM-CNRS-Universite? Paris Diderot; CEA, IRFU, SAp, centre de Saclay, F-91191, Gif-sur-Yvette, France e-mail: sandrine.lefebvre@cea.fr; rgarcia@cea.fr 2 Instituto de Astrof??sica de Canarias, 38205, La Laguna, Tenerife, Spain Preprint online version: August 4, 2008 ABSTRACT Context. Below 1 mHz, the power spectrum of helioseismic velocity measurements is dominated by the spectrum of convective motions (granulation and supergranulation) making it difficult to detect the low-order acoustic modes and the gravity modes. Aims. We want to better understand the behavior of solar granulation as a function of the observing height in the solar atmosphere and with magnetic activity during solar cycle 23. Methods. We analyze the Power Spectral Density (PSD) of eleven years of GOLF/SOHO velocity-time series using a Harvey-type model to characterize the properties of the convective motions in the solar oscillation power spectrum. We study then the evolution of the granulation with the altitude in the solar atmosphere and with the solar activity. Results. First, we show that the traditional use of a lorentzian profile to fit the envelope of the p modes is not well suitable for GOLF data. Indeed, to properly model the solar spectrum, we need a second lorentzian profile. Second, we show that the granulation clearly evolves with the height in the photosphere but does not present any significant variation with the activity cycle. Key words. Sun: activity – Sun: chromosphere – Sun: granulation – Sun: helioseismology – Sun: oscillations – Sun: photosphere 1. Introduction The photosphere, the visible layer of the Sun, is the location wher