Bibcode
Puschmann, K. G.; Ruiz Cobo, B.; Vázquez, M.; Bonet, J. A.; Hanslmeier, A.
Bibliographical reference
Astronomy and Astrophysics, Volume 441, Issue 3, October III 2005, pp.1157-1169
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10
2005
Journal
Citations
39
Refereed citations
36
Description
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 optical depth (logτ) and geometrical height (z).
Spatial coherence and phase shift analyses 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 logτ and z. 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 logτ = -1 or z
~ 170 km. At the layers beyond, an inversion of the temperature contrast
at granular scales >1.5 arcsec is revealed, both in logτ and z.
At deeper layers the temperature sensitivity of the H-
opacity leeds to much smaller temperature fluctuations at equal logτ
than at equal z, in concordance with Stein & Nordlund (1998, ApJ,
499, 914). Vertical velocities are in phase throughout the photosphere
and penetrate into the highest layers under study. Velocities at the
largest granular scales (~ 4´´) are still found even at
logτ ~ -2.8 or z ~ 370 km. Again a less efficient height penetration
of smaller cells concerning convective velocities is revealed, although
still at logτ ~ -2 or z ~ 280 km structures >1.4 arcsec are
detected. A similar size distribution of velocity and temperature
structures with height provides observational evidence for substantial
overshoot into the photosphere. At deep photospheric layers, the
behaviour of the vertical velocities reflected in simulations is for the
first time qualitatively reproduced by observations: intergranular
velocities are larger than the granular ones and, both reach extrema,
where the granular one is shifted towards higher layers.