Optical performance of the Metis coronagraph on the Solar Orbiter ESA mission

Fabio Frassetto; Vania Da Deppo; Paola Zuppella; Marco Romoli; Silvano Fineschi; Ester Antonucci; Giana Nicolini; Giampiero Naletto; Piergiorgio Nicolosi; Daniele Spadaro; Vincenzo Andretta; Marco Castronuovo; Marta Casti; Gerardo Capobianco; Giuseppe Massone; Roberto Susino; Federico Landini; Maurizio Pancrazzi; Luca Teriaca; Udo Schühle; Klaus Heerlein; Michela Uslenghi

doi:10.1117/12.2536169

12 July 2019 Optical performance of the Metis coronagraph on the Solar Orbiter ESA mission

Fabio Frassetto, Vania Da Deppo, Paola Zuppella, Marco Romoli, Silvano Fineschi, Ester Antonucci, Giana Nicolini, Giampiero Naletto, Piergiorgio Nicolosi, Daniele Spadaro, Vincenzo Andretta, Marco Castronuovo, Marta Casti, Gerardo Capobianco, Giuseppe Massone, Roberto Susino, Federico Landini, Maurizio Pancrazzi, Luca Teriaca, Udo Schühle, Klaus Heerlein, Michela Uslenghi

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Proceedings Volume 11180, International Conference on Space Optics — ICSO 2018; 111806Y (2019) https://doi.org/10.1117/12.2536169
Event: International Conference on Space Optics - ICSO 2018, 2018, Chania, Greece

Abstract

The Metis coronagraph aboard the Solar Orbiter ESA spacecraft is expected to provide new insights into the solar dynamics. In detail, it is designed to address three main questions: the energy deposition mechanism at the poles (where the fast wind is originated), the source of the slow wind at lower altitude, and how the global corona evolves, in particular in relation to the huge plasma ejections that occasionally are produced. To obtain the required optical performance, not only the Metis optical design has been highly optimized, but the alignment procedure has also been subjected to an accurate evaluation in order to fulfill the integration specifications. The telescope assembling sequence has been constructed considering all the subsystems manufacturing, alignment and integration tolerances. The performance verification activity is an important milestone in the instrument characterization and the obtained results will assure the fulfillment of the science requirements for its operation in space.

The entire alignment and verification phase has been performed by the Metis team in collaboration with Thales Alenia Space Torino and took place in ALTEC (Turin) at the Optical Payload System Facility using the Space Optics Calibration Chamber infrastructure, a vacuum chamber especially built and tested for the alignment and calibration of the Metis coronagraph, and suitable for tests of future payloads.

The goal of the alignment, integration, verification and calibration processes is to measure the parameters of the telescope, and the characteristics of the two Metis channels: visible and ultraviolet. They work in parallel thanks to the peculiar optical layout. The focusing and alignment performance of the two channels must be well understood, and the results need to be easily compared to the requirements. For this, a dedicated illumination method, with both channels fed by the same source, has been developed; and a procedure to perform a simultaneous through focus analysis has been adopted.

In this paper the final optical performance achieved by Metis is reported and commented.

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Fabio Frassetto, Vania Da Deppo, Paola Zuppella, Marco Romoli, Silvano Fineschi, Ester Antonucci, Giana Nicolini, Giampiero Naletto, Piergiorgio Nicolosi, Daniele Spadaro, Vincenzo Andretta, Marco Castronuovo, Marta Casti, Gerardo Capobianco, Giuseppe Massone, Roberto Susino, Federico Landini, Maurizio Pancrazzi, Luca Teriaca, Udo Schühle, Klaus Heerlein, and Michela Uslenghi "Optical performance of the Metis coronagraph on the Solar Orbiter ESA mission", Proc. SPIE 11180, International Conference on Space Optics — ICSO 2018, 111806Y (12 July 2019); https://doi.org/10.1117/12.2536169

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