A Fabry-Perot spectrometer for high-resolution observation of the Sun

Details A Fabry-Perot spectrometer for high-resolution observation of the Sun A Fabry-Perot spectrometer for high-resolution observation of the Sun

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001an....322..375k&link_type=abstract

Astronomische Nachrichten, vol. 322, no. 5/6, p. 375-378

Computer Science

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5

Scientific paper

Fabry-Perot interferometers (FPIs) are powerful instruments for spectro-polarimetry of the Sun with high spatial resolution. They allow easy image reconstruction of two-dimensional fields of view. Some examples of high quality results obtained with the ``Göttingen'' FPI spectrometer, mounted in the Vacuum Tower Telescope at the Observatorio del Teide/Tenerife, are presented in a poster to this workshop. We thus concentrate on the design of a new instrument for the 1.5 m GREGOR solar telescope. We discuss the pros and cons of telecentric and collimated mounting and describe the expected performance, especially the spectral resolution, of our design.

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