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On the spectropolarimetric signature of FeH in the laboratory and in sunspots

Published online by Cambridge University Press:  07 August 2014

Patrick Crozet ,
Amanda J. Ross ,
Nathalie Alleq ,
Arturo López Ariste ,
Claude Le Men  and
Bernard Gelly
Patrick Crozet
Affiliation:
Institut Lumière Matière, UMR5306 Université Lyon 1-CNRS, Université de Lyon, 69622 Villeurbanne Cedex, France. email: patrick.crozet@univ-lyon1.fr
Amanda J. Ross
Affiliation:
Institut Lumière Matière, UMR5306 Université Lyon 1-CNRS, Université de Lyon, 69622 Villeurbanne Cedex, France. email: patrick.crozet@univ-lyon1.fr
Nathalie Alleq
Affiliation:
Institut Lumière Matière, UMR5306 Université Lyon 1-CNRS, Université de Lyon, 69622 Villeurbanne Cedex, France. email: patrick.crozet@univ-lyon1.fr
Arturo López Ariste
Affiliation:
THEMIS Télescope Héliographique pour l'Etude du Magnétisme et des Instabilités Solaire, UPS853 (CNRS/Observatorio del Teide, C/Via Lactea s/n 38200 La Laguna, Tenerife, Spain.
Claude Le Men
Affiliation:
THEMIS Télescope Héliographique pour l'Etude du Magnétisme et des Instabilités Solaire, UPS853 (CNRS/Observatorio del Teide, C/Via Lactea s/n 38200 La Laguna, Tenerife, Spain.
Bernard Gelly
Affiliation:
THEMIS Télescope Héliographique pour l'Etude du Magnétisme et des Instabilités Solaire, UPS853 (CNRS/Observatorio del Teide, C/Via Lactea s/n 38200 La Laguna, Tenerife, Spain.
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Résumé

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Laboratory spectra showing Zeeman patterns in some FeH lines susceptible to be used as magnetic probes in cool stellar atmostpheres have been recorded in the laboratory, and molecular Landé factors obtained from analysis. These Landé factors have been used to model some lines recorded in Stokes V polarisation in sunspot spectra at the solar telescope THEMIS.

Keywords

electronic spectrum of FeHmolecular Landé factorsunspot spectrumStokes V profile
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S302: Magnetic Fields throughout Stellar Evolution , August 2013 , pp. 164 - 165
Copyright
Copyright © International Astronomical Union 2014 

References

Afram, N., Berdyugina, S. V., Fluri, D. M., Solanki, S. K., & Lagg, A. 2008, A.&A. 482 (2), 387Google Scholar
Harrison, J. J. & Brown, J. M., ApJ. 686 (2008) 1426Google Scholar
Vallon, R., Ashworth, S. H., Crozet, P., Field, R. W., Forthomme, D., Harker, H., Richard, C., & Ross, A. J. 2009, J. Phys. Chem. A, 113, 13159Google Scholar
Brown, J. M., Körsgen, H., Beaton, S. P., & Evenson, K. M. 2006, J. Chem. Phys. 124 (23)234309Google Scholar
Wallace, L., Livingstone, W., Bernath, P., & Ram, R. S. 1998, N. S. O. Technical Report 1998-002, Available online ftp://nsokp.nso.edu/pub/atlas/spot3altGoogle Scholar