Volume 443, Number 3, December I 2005
|Page(s)||1047 - 1053|
|Published online||15 November 2005|
A polarization model for the German Vacuum Tower Telescope from in situ and laboratory measurements
Kiepenheuer-Institut für Sonnenphysik, Schöneckstr. 6, 79104 Freiburg, Germany e-mail: [cbeck;schliche;lbellot;tk]@kis.uni-freiburg.de
2 Instituto de Astrofísica de Canarias, via Láctea, La Laguna, Tenerife, Spain e-mail: firstname.lastname@example.org
3 Instituto de Astrofísica de Andalucía, Apdo. 3004, 18080 Granada, Spain e-mail: email@example.com
Accepted: 21 July 2005
It is essential to properly calibrate the polarimetric properties of telescopes, if one wants to take advantage of the capabilities of high precision spectro-polarimeters. We have constructed a model for the German Vacuum Tower Telescope (VTT) that describes its time-dependent polarization properties. Since the coelostat of the telescope changes the polarization state of the light by introducing cross talk among different polarization states, such a model is necessary to correct the measurements, in order to retrieve the true polarization as emitted from the Sun. The telescope model is quantified by a time-dependent Mueller matrix that depends on the geometry of the light beam through the telescope, and on material properties: the refractive indices of the coelostat mirrors, and the birefringence of the entrance window to the vacuum tube. These material properties were determined experimentally in-situ by feeding the telescope with known states of polarization (including unpolarized light) and by measuring its response, and from measurements of an aluminum-coated sample in the laboratory. Accuracy can in our case be determined only for the combination of telescope and spectro-polarimeter used; for the instrument POLIS at the VTT, we estimate an accuracy of ±4– for the cross talk correction coefficients.
Key words: instrumentation: polarimeters / sun: magnetic fields
© ESO, 2005
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