Volume 497, Number 1, April I 2009
|Page(s)||273 - 285|
|Published online||09 February 2009|
The relationship between chromospheric emissions and magnetic field strength
Max-Planck-Institut für Sonnensystemforschung, 37191 Katlenburg-Lindau, Germany e-mail: firstname.lastname@example.org
2 Astronomical Institute, St. Petersburg University, 198504 St. Petersburg, Russia
3 Astronomy Department, University of Maryland, College Park, MD 20742, USA
Accepted: 28 January 2009
Aims. We analyze observational data from 4 instruments to study the correlations between chromospheric emission, spanning the heights from the temperature minimum region to the middle chromosphere, and photospheric magnetic field.
Methods. The data consist of radio images at 3.5 mm from the Berkeley-Illinois-Maryland Array (BIMA), UV images at 1600 Å from TRACE, Ca II K-line filtergrams from BBSO, and MDI/SOHO longitudinal photospheric magnetograms. For the first time interferometric millimeter data with the highest currently available resolution are included in such an analysis. We determine various parameters of the intensity maps and correlate the intensities with each other and with the magnetic field.
Results. The chromospheric diagnostics studied here show a pronounced similarity in their brightness structures and map out the underlying photospheric magnetic field relatively well. We find a power law to be a good representation of the relationship between photospheric magnetic field and emission from chromospheric diagnostics at all wavelengths. The dependence of chromospheric brightness on magnetic field is found to be different for network and internetwork regions.
Key words: Sun: chromosphere / Sun: radio radiation / Sun: magnetic fields
© ESO, 2009
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