The height dependence of temperature : velocity correlation in the solar photosphere

J. Koza, A. Kucera, J. Rybák, H. Wöhl

Research output: Chapter in Book/Report/Conference proceedingChapterAcademicpeer-review

Abstract

We derive correlation coe±cients between temperature and line-of-sight velocity as a function of optical depth throughout the solar photosphere for the non-magnetic photosphere and a small area of enhanced magnetic activity. The maximum anticorrelation of about ¡0:6 between temperature and line-of-sight velocity in the non-magnetic photosphere occurs at log ¿5 = ¡0:4. The magnetic eld is another decorrelating factor along with 5-min oscillations and seeing.
Original languageUndefined/Unknown
Title of host publicationModern solar facilities - advanced solar science : proceedings of a workshop held at Göttingen September 27 - 29, 2006
EditorsFranz Kneer, Klaus G. Puschmann, Axel D. Wittmann
Place of PublicationGöttingen
PublisherUniv.-Verl. Göttingen
Pages139-142
Number of pages381
ISBN (Print)9783938616840
Publication statusPublished - 2007

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