• Opto-Electronic Engineering
  • Vol. 47, Issue 9, 190049 (2020)
WangJia1、2、3、*, Liu Yangyi1、2, and Rao Changhui1、2
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • 3[in Chinese]
  • show less
    DOI: 10.12086/oee.2020.190049 Cite this Article
    WangJia, Liu Yangyi, Rao Changhui. A calibration method for Lyot filter[J]. Opto-Electronic Engineering, 2020, 47(9): 190049 Copy Citation Text show less
    References

    [1] Goode P R, Denker C J, Didkovsky L I, et al. 1.6 M Solar telescope in big bear-the NST[J]. Journal of the Korean Astronomical Society, 2003, 36(spc1): 125–133.

         Goode P R, Denker C J, Didkovsky L I, et al. 1.6 M Solar telescope in big bear-the NST[J]. Journal of the Korean Astronomical Society, 2003, 36(spc1): 125–133.

    [2] Ichimoto K, Ishii T T, Otsuji K, et al. A new solar imaging system for observing high-speed eruptions: Solar Dynamics Doppler Imager (SDDI)[J]. Solar Physics, 2017, 292(4): 63.

         Ichimoto K, Ishii T T, Otsuji K, et al. A new solar imaging system for observing high-speed eruptions: Solar Dynamics Doppler Imager (SDDI)[J]. Solar Physics, 2017, 292(4): 63.

    [3] Bethge C, Peter H, Kentischer T J, et al. The chromospheric telescope[J]. Astronomy & Astrophysics, 2011, 534: A105.

         Bethge C, Peter H, Kentischer T J, et al. The chromospheric telescope[J]. Astronomy & Astrophysics, 2011, 534: A105.

    [4] Yan X L, Xue Z K, Xiang YY, et al. Fine-scale structures and material flows of quiescent .laments observed by the New Vacuum Solar Telescope[J]. Research in Astronomy and Astrophysics, 2015, 15(10): 1725–1734.

         Yan X L, Xue Z K, Xiang YY, et al. Fine-scale structures and material flows of quiescent .laments observed by the New Vacuum Solar Telescope[J]. Research in Astronomy and Astrophysics, 2015, 15(10): 1725–1734.

    [10] Mudge J, Tarbell T. In situ calibration of tunable filters: lyot and michelson[J]. Applied Optics, 2014, 53(22): 4978–4986.

         Mudge J, Tarbell T. In situ calibration of tunable filters: lyot and michelson[J]. Applied Optics, 2014, 53(22): 4978–4986.

    [11] Couvidat S, Rajaguru S P, Wachter R, et al. Line-of-sight observables algorithms for the helioseismic and magnetic imager (hmi) instrument tested with interferometric bidimensional spectrometer (IBIS) observations[J]. Solar Physics, 2012, 278: 217–240.

         Couvidat S, Rajaguru S P, Wachter R, et al. Line-of-sight observables algorithms for the helioseismic and magnetic imager (hmi) instrument tested with interferometric bidimensional spectrometer (IBIS) observations[J]. Solar Physics, 2012, 278: 217–240.

    [12] Rimmele T R, Hubbard R P, Balasubramaniam K S, et al. Instrumentation for the advanced technology solar telescope[J]. Proceedings of SPIE, 2004, 5492: 944–957.

         Rimmele T R, Hubbard R P, Balasubramaniam K S, et al. Instrumentation for the advanced technology solar telescope[J]. Proceedings of SPIE, 2004, 5492: 944–957.

    [13] Rao C H, Zhu L, Gu N T, et al. A high-resolution multi-wavelength simultaneous imaging system with solar adaptive optics[J]. The Astronomical Journal, 2017, 154(4): 143.

         Rao C H, Zhu L, Gu N T, et al. A high-resolution multi-wavelength simultaneous imaging system with solar adaptive optics[J]. The Astronomical Journal, 2017, 154(4): 143.

    WangJia, Liu Yangyi, Rao Changhui. A calibration method for Lyot filter[J]. Opto-Electronic Engineering, 2020, 47(9): 190049
    Download Citation