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SUAVE: a disruptive "watch dog" far UV telescope for space weather and solar variability studies

Auteur

Damé Luc

Institution

LATMOS

Thème

Theme2
Auteur(s) supplémentaire(s)M. Meftah1, N. Rouanet1, P. Gilbert1, P. Etcheto2 and J. Berthon2
Institution(s) supplémentaire(s)(2) Service Optique, CNES, 18 Avenue Edouard Belin, 31400 Toulouse, France

Abstract

SUAVE (Solar Ultraviolet Advanced Variability Experiment) is a far UV imaging solar telescope (Lyman Alpha, 121.6 nm, Herzberg continuum, 200-220 nm, etc.) of novel design for ultimate thermal stability and long lasting performances. SUAVE is a 80 mm Ritchey-Chrétien off-axis telescope with SiC mirrors and no entrance window for long and uncompromised observations in the UV (no coatings of mirrors, flux limited to less than 2 solar constants on filters to avoid their degradation), associated with an ultimate thermal control (no central obscuration resulting in limited thermal gradients and easier heat evacuation, focus control, stabilization). Design and anticipated performances will be detailed as well as progresses towards realization of a representative breadboard for tests of optical and thermal properties by the end of 2018. SUAVE is the main instrument of the polar microsatellite of the SoSWEET-SOUP (SOlar, Space Weather Extreme EvenTs and Stratospheric Ozone Ultimate Profiles) mission presently under study (ex-SUITS/SWUSV mission, Solar Ultraviolet Influence on Troposphere/Stratosphere / Space Weather and Ultraviolet Solar Variability).


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