Line-of-sight Velocity in a Semiempirical Model of a Disappearing Granule
J. Koza(1),
L.R. Bellot Rubio(3),
A. Kucera(1),
A. Hanslmeier(2),
J. Rybak(1),
H. Wohl(3)
1 - Astronomical Institute, Slovak Academy of Sciences, SK-05960 Tatranská Lomnica, Slovakia
2 - Institut for Geophysics, Astrophysics and Meteorology, Universitätsplatz 5, A-8010 Graz, Austria
3 - Kiepenheuer-Institut fur Sonnenphysik, Schoneckstr. 6, 79104 Freiburg,
Germany
The behaviour of the line-of-sight velocity in the centre of a
disappearing granule is analyzed using an inversion method applied to a
time-series of spectra containing the Fe I 522.5 nm, 557.6 nm and 557.7 nm
lines. The temporal evolution of the line-of-sight velocity
vLOS is presented in the form of the functional dependence of
vLOS(log o/5, t) on the optical depth at 500 nm and time.
An oscillatory behaviour is found in the velocity stratification
with nearly constant phase through the photosphere. The amplitude of
variations increases from log depth = -0.3 to log depth = -2.5 reaching a
maximum of 1.2 km s-1.
A zero velocity layer is detected in every instantaneous model of the
velocity stratification. The results suggest, that the zero velocity may
occur in a considerable range of the optical depths from log
depth -2 to log depth -3.5.
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