Paper
8 July 2014 MuSICa image slicer prototype at 1.5-m GREGOR solar telescope
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Abstract
Integral Field Spectroscopy is an innovative technique that is being implemented in the state-of-the-art instruments of the largest night-time telescopes, however, it is still a novelty for solar instrumentation. A new concept of image slicer, called MuSICa (Multi-Slit Image slicer based on collimator-Camera), has been designed for the integral field spectrograph of the 4-m European Solar Telescope. This communication presents an image slicer prototype of MuSICa for GRIS, the spectrograph of the 1.5-m GREGOR solar telescope located at the Observatory of El Teide. MuSICa at GRIS reorganizes a 2-D field of view of 24.5 arcsec into a slit of 0.367 arcsec width by 66.76 arcsec length distributed horizontally. It will operate together with the TIP-II polarimeter to offer high resolution integral field spectropolarimetry. It will also have a bidimensional field of view scanning system to cover a field of view up to 1 by 1 arcmin.
© (2014) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. Calcines, R. L. López, M. Collados, and N. Vega Reyes "MuSICa image slicer prototype at 1.5-m GREGOR solar telescope", Proc. SPIE 9147, Ground-based and Airborne Instrumentation for Astronomy V, 91473I (8 July 2014); https://doi.org/10.1117/12.2053577
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Cited by 6 scholarly publications.
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KEYWORDS
Mirrors

Spectrographs

Prototyping

Solar telescopes

Diffraction

Zemax

Cameras

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