Počet záznamů: 1  

Optical design of the multi-wavelength imaging coronagraph Metis for the solar orbiter mission

  1. 1.
    0541105 - ÚFP 2021 RIV NL eng J - Článek v odborném periodiku
    Fineschi, S. - Naletto, G. - Romoli, M. - Da Deppo, V. - Antonucci, E. - Moses, D. - Malvezzi, M.A. - Nicolini, G. - Spadaro, D. - Teriaca, L. - Andretta, V. - Capobianco, G. - Crescenzio, G. - Focardi, M. - Frassetto, F. - Landini, F. - Massone, G. - Melich, Radek - Nicolosi, P. - Pancrazzi, M. - Pelizzo, M.-G. - Poletto, L. - Schühle, U.H. - Uslenghi, M. - Vives, S. - Solanki, S.K. - Heinzel, Petr - Berlicki, A. - Cesare, S. - Morea, D. - Mottini, S. - Sandri, P. - Alvarez-Herrero, A. - Castronuovo, M.M.
    Optical design of the multi-wavelength imaging coronagraph Metis for the solar orbiter mission.
    Experimental Astronomy. Roč. 49, č. 3 (2020), s. 239-263. ISSN 0922-6435. E-ISSN 1572-9508
    Institucionální podpora: RVO:61389021 ; RVO:67985815
    Klíčová slova: Coronagraphy * Solar instrumentation * Ultraviolet imaging * Visible-light polarimetry
    Obor OECD: Optics (including laser optics and quantum optics)
    Impakt faktor: 2.012, rok: 2020
    Způsob publikování: Open access
    https://link.springer.com/content/pdf/10.1007/s10686-020-09662-z.pdf

    This paper describes the innovative optical design of the Metis coronagraph for the Solar Orbiter ESA-NASA mission. Metis is a multi-wavelength, externally occulted telescope for the imaging of the solar corona in both the visible and ultraviolet wavelength ranges. Metis adopts a novel occultation scheme for the solar disk, that we named “inverse external occulter”, for reducing the extremely high thermal load on the instrument at the spacecraft perihelion. The core of the Metis optical design is an aplanatic Gregorian telescope common to both the visible and ultraviolet channels. A suitable dichroic beam-splitter, optimized for transmitting a narrow-band in the ultraviolet (121.6 nm, HI Lyman-α) and reflecting a broadband in the visible (580–640 nm) spectral range, is used to separate the two optical paths. Along the visible light optical path, a liquid crystal electro-optical modulator, used for the first time in space, allows making polarimetric measurements.
    Trvalý link: http://hdl.handle.net/11104/0318690

     
     
Počet záznamů: 1  

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