Presentation + Paper
11 September 2024 Conceptual design of the infrared integral field spectropolarimeter for the European Solar Telescope
Author Affiliations +
Abstract
The European Solar Telescope (EST) will be Europe’s most ambitious ground-based infrastructure in solar physics. It will have a primary mirror with a diameter of 4.2m, which will make it the largest in Europe, and of identical aperture as the largest solar telescope available worldwide, namely the Daniel K. Inouye Telescope (DKIST) installed at the Haleakala summit, Hawai'i. EST will have two main characteristics devoted to maximising the scientific return. First, the telescope’s optical path will be polarisation-free using pairs of mirrors that compensate for instrumental polarisation. Second, the telescope will be designed together with a complete instrument suite with imaging and spectrograph instruments. EST will also bring many new technologies, such as a multi-conjugate adaptive optics system and integral field spectro-polarimeters. This contribution presents the conceptual design of the infrared (1 to 1.8 microns) integral field spectropolarimeter. The instrument will have an integral field unit composed of a mirror-based image slicer as input to a Czerny-Turner spectrograph. It will have a polarimeter to record the polarisation state of light on a dual-beam configuration to ensure high-precision spectro-polarimetry.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
C. Quintero Noda, M. J. Martínez González, S. Regalado Olivares, P. Gómez González, T. del Pino Alemán, J. C. Trelles Arjona, J. Bienes, A. Matta-Gómez, and M. Collados "Conceptual design of the infrared integral field spectropolarimeter for the European Solar Telescope", Proc. SPIE 13094, Ground-based and Airborne Telescopes X, 130942C (11 September 2024); https://doi.org/10.1117/12.3018749
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KEYWORDS
Magnetism

Equipment

Signal to noise ratio

Polarimetry

Polarization

Spatial resolution

Design

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