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A&A 380, L5-L8 (2001)
DOI: 10.1051/0004-6361:20011505
Zeeman-split opposite-polarity OH lines in sunspot spectra: Resolution of a puzzle
S. V. Berdyugina1 and S. K. Solanki21 Astronomy Division, PO Box 3000, 90014 University of Oulu, Finland
2 Max-Planck-Institut für Aeronomie, 37191 Katlenburg-Lindau, Germany
(Received 7 September 2001 / Accepted 10 October 2001 )
Abstract
We present the first synthetic Zeeman-split Stokes I and V profiles of
OH lines. They explain the puzzling observations reported by Harvey
(1985) of two pairs of lines from the infrared (2, 0)
band with Stokes V profiles exhibiting opposite polarities. Our new
perturbation calculations of the Zeeman effect in diatomic molecules, which
allow states of any multiplicity to be treated, resolve the puzzle. They
reveal that the unusual behaviour of these lines stems from the fact that
the two pairs have effective Landé factors of similar magnitude, but of
opposite signs.
Key words: Sun: sunspots -- molecules -- polarization
Offprint request: S. V. Berdyugina, Sveta.Berdyugina@oulu.fi
© ESO 2001
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