Poster + Presentation + Paper
13 December 2020 Tor Vergata Synoptic Solar Telescope: spectral characterization of potassium KI D1 MOFs
Daniele Calchetti, Giorgio Viavattene, Luciano Terranegra, Ermanno Pietropaolo, Maurizio Oliviero, Neil Murphy, Stuart M. Jefferies, Luca Giovannelli, Dario Del Moro, Francesco Berrilli
Author Affiliations +
Conference Poster
Abstract
Synoptic telescopes are fundamental tools in Solar Physics and Space Weather. Their typical high cadence full-disk observations are pivotal to assess the physical conditions on the Sun and to forecast the evolution in time of those conditions. The TSST (Tor vergata Synoptic Solar Telescope) is a synoptic telescope composed of two main full-disk instruments: an H-alpha Daystar SR-127 telescope and a Magneto Optical Filter (MOF)-based telescope in the Potassium KI at 769.90 nm. The MOF consists in a glass cell containing a Potassium vapor where a longitudinal magnetic field is applied. The MOF-based channel produces full disk Line-of-Sight magnetic field and velocity maps of the solar photosphere at 300 km above the solar surface. In this work, we present the optical setup, the spectral characterization of the MOF-based telescope, and details on the spectral characterization of the MOFs cells which is a required test to obtain calibrated magnetograms and dopplergrams.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Daniele Calchetti, Giorgio Viavattene, Luciano Terranegra, Ermanno Pietropaolo, Maurizio Oliviero, Neil Murphy, Stuart M. Jefferies, Luca Giovannelli, Dario Del Moro, and Francesco Berrilli "Tor Vergata Synoptic Solar Telescope: spectral characterization of potassium KI D1 MOFs", Proc. SPIE 11445, Ground-based and Airborne Telescopes VIII, 114452T (13 December 2020); https://doi.org/10.1117/12.2562454
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KEYWORDS
Telescopes

Solar processes

Micro optical fluidics

Solar telescopes

Doppler effect

Magnetism

Potassium

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