Abstract
Using spectrograms of high spatial resolution we investigated the functional interdependence between the convective intensity fluctuations at τ5000 = 1 and the line broadening of magnetically sensitive absorption lines in active and nonactive regions. We found an extra broadening in the intergranular regions. The variation of this broadening with height in the photosphere can be attributed to the variation of the magnetic filling factor as well as to enhanced nonthermal velocities.
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Komm, F., Mattig, W., and Nesis, A.: 1990, to be published in Astron. Astrophys.
Narain, U., and Ulmschneider, P.: 1990, to appear in Space Science Reviews
Nesis, A., Hanslmeier, A., Hammer, R., Komm, R., and Mattig, W.: 1990, in The Dynamic Sun, Proceedings of the 6th European Meeting on Solar Physics, ed. L. Dezsŏ
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© 1991 Springer-Verlag Berlin Heidelberg
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Nesis, A., Hanslmeier, A., Hammer, R., Komm, R., Mattig, W. (1991). On the Dynamics of Granulation in Active Regions and the Heating Problem. In: Ulmschneider, P., Priest, E.R., Rosner, R. (eds) Mechanisms of Chromospheric and Coronal Heating. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-87455-0_8
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DOI: https://doi.org/10.1007/978-3-642-87455-0_8
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