Abstract
Applying a correlation analysis to time series of granulation it has been shown that due to the influence of enhanced turbulent motions near the downflow regions in the intergranular lanes the turbulent motions predominate.
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References
Espagnet, O., Muller, R., Roudier, T, Mein, P., Mein, N., and Malherbe, J.M.: 1996,A&A 313, 297.
Hanslmeier, A., Nesis, A., and Mattig, W.: 1991, A&A 251, 307.
Hanslmeier, A., Kučera, A., Rybák, J., Neunteufel, B., and Wöhl, H.: 2000, A&A accepted.
Mattig, W. and Schlebbe, H., 1974: Solar Phys. 34, 299.
Nesis, A., Hammer, R., Kiefer, M., Schleicher, H., Sigwarth, M., and Staiger, J.: 1999,A&A 345, 265.
Rimmele, Th., Goode, P., Harold, E., and Stebbins, R.: 1995, ApJ 444, L119.
Schröter, E.H., Soltau, D., and Wiehr, E.: 1985, Vistas Astron. 28, 519.
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Hanslmeier, A., Kučera, A., Rybák, J., Wöhl, H. (2001). The Location of Solar Oscillations in the Photosphere. In: Hanslmeier, A., Messerotti, M., Veronig, A. (eds) The Dynamic Sun. Astrophysics and Space Science Library, vol 259. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0760-3_22
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DOI: https://doi.org/10.1007/978-94-010-0760-3_22
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