Wide field-of-view liquid crystals-based modulator for the polarimeter of the Metis/Solar Orbiter

被引:9
|
作者
Capobianco, Gerardo [1 ]
Casti, Marta [1 ]
Fineschi, Silvano
Massone, Giuseppe [1 ]
Sertsu, Mewael G. [2 ]
Landini, Federico [3 ]
Romoli, Marco [4 ]
Antonucci, Ester [1 ]
Andretta, Vincenzo [5 ]
Naletto, Giampiero
Nicolini, Gianalfredo [1 ]
Spadaro, Daniele [6 ]
Alvarez Herrero, Alberto [7 ]
Garcia Parejo, Pilar [7 ]
Marmonti, Matteo [8 ]
机构
[1] INAF Astrophys Observ Torino, Str Osservatorio 20, I-10025 Turin, Italy
[2] Univ Padua, Via Gradenigo 6-B, I-35131 Padua, Italy
[3] INAF Astrophys Observ Arcetri, Largo E Fermi 5, I-50125 Florence, Italy
[4] Florence Univ, Via Sansone 1, I-50019 Florence, Italy
[5] INAF Astrophys Observ Capodimonte, Salita Moiariello 16, I-80131 Naples, Italy
[6] INAF Astrophys Observ Catania, Via S Sofia 78, I-95123 Catania, Italy
[7] INTA, Cra Ajalvir Km 4-5, Madrid 28850, Spain
[8] OPTEC SpA, Via Mantegna 34, I-20015 Milan, Italy
关键词
Solar Corona; Coronagraphy; Polarimeter; Calibrations; Liquid Crystals; MUELLER MATRIX;
D O I
10.1117/12.2323371
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Metis is an inverted occulted coronagraph on-board the ESA/Solar Orbiter mission. The visible light path of the instrument will observe the "white" light (580-640 nm) linearly-polarized emission from the solar corona. The coronal polarized brightness allows retrieval of physical parameters such as the electron density and temperature of the K-corona. The Metis polarimeter comprises a quarter-wave retarder, the liquid crystal polarization modulation package (PMP) and a linear polarizer working as polarization analyser. The PMP consists of two Anti-Parallel Nematic Liquid Crystal Variable Retarders (LCVRs) with the fast axes parallels one to each other and a pre-tilted angle of the molecules in opposite direction, in order to maximize the homogeneity of the retardance across instrumental wide field of view: +/- 7 deg. This presentation reports the characterization of the PMP breadboard (BB), fully representative of the optical/polarimetric performances of the flight model. This characterization consisted in determining the performances of the device in terms of retardance as function of the applied voltage at different temperatures, angle of incidence and the variation of the retardance as a function of the wavelength. The calibrations were performed by measuring the complete Mueller matrix of the PMP-BB. The experimental results have been compared with the parameters of the theoretical model (e.g., depolarization, effective retardance, cells misalignment).
引用
收藏
页数:11
相关论文
共 50 条
  • [21] Wide field-of-view Fourier Ptychography microscopy based on Fresnel propagation scheme
    Hasanzade, Mojde
    Breiby, Dag Werner
    Akram, Muhammad Nadeem
    RESULTS IN OPTICS, 2022, 8
  • [22] Wide field-of-view Fourier Ptychography microscopy based on Fresnel propagation scheme
    Hasanzade, Mojde
    Breiby, Dag Werner
    Akram, Muhammad Nadeem
    RESULTS IN OPTICS, 2022, 8
  • [23] Wide and scalable field-of-view Talbot-grid-based fluorescence microscopy
    Pang, Shuo
    Han, Chao
    Kato, Mihoko
    Sternberg, Paul W.
    Yang, Changhuei
    OPTICS LETTERS, 2012, 37 (23) : 5018 - 5020
  • [24] Chip-based wide field-of-view total internal reflection fluorescence microscopy
    Fan, Zetao
    Kuai, Yan
    Tang, Xi
    Zhang, Yifan
    Zhang, Douguo
    OPTICS LETTERS, 2022, 47 (17) : 4303 - 4306
  • [25] Wide field-of-view Talbot grid-based microscopy for multicolor fluorescence imaging
    Pang, Shuo
    Han, Chao
    Erath, Jessey
    Rodriguez, Ana
    Yang, Changhuei
    OPTICS EXPRESS, 2013, 21 (12): : 14555 - 14565
  • [26] Performance of a wide field-of-view atmospheric Cherenkov telescope prototype based on a refractive lens
    Chen, Tianlu
    Liu, Cheng
    Gao, Qi
    Cai, Hui
    Wang, Zhen
    Zhang, Yi
    Feng, Youliang
    Wang, Qun
    Guo, Yiqing
    Hu, Hongbo
    Danzengluobu
    Liu, Maoyuan
    Li, Haijin
    Xin, Guangguang
    Gou, Quanbu
    Cai, Hao
    Shi, Ying
    NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 2019, 927 : 46 - 53
  • [27] Wide field-of-view soft X-ray imaging for solar wind-magnetosphere interactions
    Walsh, B. M.
    Collier, M. R.
    Kuntz, K. D.
    Porter, F. S.
    Sibeck, D. G.
    Snowden, S. L.
    Carter, J. A.
    Collado-Vega, Y.
    Connor, H. K.
    Cravens, T. E.
    Read, A. M.
    Sembay, S.
    Thomas, N. E.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2016, 121 (04) : 3353 - 3361
  • [28] Optical System Design of a Wide Field-of-View Camera for the Characterization of Earth's Reflected Solar Radiation
    Schifano, Luca
    Smeesters, Lien
    Berghmans, Francis
    Dewitte, Steven
    REMOTE SENSING, 2020, 12 (16)
  • [30] Effect of Temporal Sampling Interval on the Irradiance for Moon-Based Wide Field-of-View Radiometer
    Zhang, Yuan
    Bi, Shengshan
    Wu, Jiangtao
    SENSORS, 2022, 22 (04)