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 language | Undefined/Unknown |
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Title of host publication | Modern solar facilities - advanced solar science : proceedings of a workshop held at Göttingen September 27 - 29, 2006 |
Editors | Franz Kneer, Klaus G. Puschmann, Axel D. Wittmann |
Place of Publication | Göttingen |
Publisher | Univ.-Verl. Göttingen |
Pages | 139-142 |
Number of pages | 381 |
ISBN (Print) | 9783938616840 |
Publication status | Published - 2007 |