THE LOCATION OF SOLAR OSCILLATIONS IN THE PHOTOSPHERE

Hanslmeier, A.(1), Kucera, A.(2), Rybák, J.(2), Wöhl, H. (3)

(1) IGAM, University of Graz, Graz, Austria
(2) Astronomical Institute, 059 60 Tatranská Lomnica, The Slovak Republic
(3) KIS, Freivurg, Germany

Applying a correlation analysis to time series of granulation it has been shown that due to the influeance of enhanced terbulent motions near the downflow regions in the intergranular lanes the turbulent motions predominate.