The GREGOR polarimetric calibration unit

The new Solar telescope GREGOR is designed to observe small‐scale dynamic magnetic structures below a size of 70 km on the Sun with high spectral resolution and polarimetric accuracy. For this purpose, the polarimetric concept of GREGOR is based on a combination of post‐focus polarimeters with pre‐f...

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Bibliographic Details
Published in:Astronomische Nachrichten Vol. 333; no. 9; pp. 854 - 862
Main Authors: Hofmann, A., Arlt, K., Balthasar, H., Bauer, S.M., Bittner, W., Paschke, J., Popow, E., Rendtel, J., Soltau, D., Waldmann, T.
Format: Journal Article
Language:English
Published: Berlin WILEY-VCH Verlag 01-11-2012
WILEY‐VCH Verlag
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Summary:The new Solar telescope GREGOR is designed to observe small‐scale dynamic magnetic structures below a size of 70 km on the Sun with high spectral resolution and polarimetric accuracy. For this purpose, the polarimetric concept of GREGOR is based on a combination of post‐focus polarimeters with pre‐focus equipment for high precision calibration. The Leibniz‐Institute for Astrophysics Potsdam developed the GREGOR calibration unit which is an integral part of the telescope. We give an overview of the function and design of the calibration unit and present the results of extensive testing series done in the Solar Observatory “Einsteinturm” and at GREGOR (© 2012 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)
Bibliography:istex:C993E83BE7ECE5CC23B77162C1D829D67D76ACF5
Kiepenheuer-Institut für Sonnenphysik in Freiburg with the Leibniz-Institut für Astrophysik Potsdam
ark:/67375/WNG-BW3TZW8Z-8
ArticleID:ASNA201211733
Institut für Astrophysik Göttingen
Astronomical Institute of the Academy of Sciences of the Czech Republic
Max-Planck-Institut für Sonnensystemforschung in Katlenburg-Lindau
ObjectType-Article-2
SourceType-Scholarly Journals-1
ObjectType-Feature-1
content type line 23
ISSN:0004-6337
1521-3994
DOI:10.1002/asna.201211733