Time series of high resolution photospheric spectra in a quiet region of the Sun - II. Analysis of the variation of physical quantities of granular structures

• DOI: 10.48550/arxiv.1205.1725
• Publication Date: 2005-09-23
• Authors: B. Ruiz Cobo; K. G. Puschmann; K. G. Puschmann; Arnold Hanslmeier; Manuel Vázquez; J. A. Bonet
• Keywords: Astrophysics - Solar and Stellar Astrophysics; 0103 physical sciences; FOS: Physical sciences; 01 natural sciences; Solar and Stellar Astrophysics (astro-ph.SR)

From the inversion of a time series of high resolution slit spectrograms obtained from the quiet sun, the spatial and temporal distribution of the thermodynamical quantities and the vertical flow velocity is derived as a function of logarithmic optical depth and geometrical height. Spatial coherence and phase shift analyzes between temperature and vertical velocity depict the height variation of these physical quantities for structures of different size. An average granular cell model is presented, showing the granule-intergranular lane stratification of temperature, vertical velocity, gas pressure and density as a function of logarithmic optical depth and geometrical height. Studies of a specific small and a specific large granular cell complement these results. A strong decay of the temperature fluctuations with increasing height together with a less efficient penetration of smaller cells is revealed. The T -T coherence at all granular scales is broken already at log tau =-1 or z~170 km. At the layers beyond, an inversion of the temperature contrast is revealed. Vertical velocities are in phase throughout the photosphere and penetrate into the highest layers under study.<br/>13 pages, 12 figures, 1 table; Astronomy & Astrophysics, Volume 441, Issue 3, pp.1157-1169, 2005<br/>