Acta Photonica Sinica, Volume. 52, Issue 5, 0552213(2023)
Stray Light by Dust on Objective Surface Based on Lijiang 10 cm Coronagraph
[1] ZHAO Haibin, LIN Qisheng, CHEN Yiping et al. Coronal structure and brightness profile of the total solar eclipse on August 1, 2008[J]. Chinese Science Bulletin, 54, 1790-1792(2009).
[2] LYOT B. The study of the solar corona and prominences without eclipses (George Darwin Lecture, 1939)[J]. Monthly Notices of the Royal Astronomical Society, 99, 580-594(1939).
[3] LLEBARIA A, LAMY P, DANJARD J F. Photometric calibration of the LASCO-C2 coronagraph for solar system objects[J]. Icarus, 182, 281-296(2006).
[4] LIU Yu. The first coronagraph in China settled in Lijiang, Yunnan province[J]. Amateur Astronomer, 1, 60-63(2014).
[5] ZHAO M, LIU Y, ELMHAMDI A et al. Conditions for coronal observations at the Lijiang observatory in 2011[J]. Solar physics, 293, 1-13(2018).
[6] ZHANG Xuefei. Construction and research based on the first coronagraph station in China[D](2022).
[7] ICHIMOTO K, NOGUCHI M, TANAKA N et al. A new imaging system of the corona at Norikura[J]. Publications of the Astronomical Society in Japan, 51, 383-391(1999).
[8] ZHANG Xuefei, LIU Yu, ZHAO Mingyu et al. Comparison of the coronal green-line intensities with the EUV measurements from SDO/AIA[J]. Research in Astronomy and Astrophysics, 22, 075012(2022).
[9] ZHANG Xuefei, LIU Yu, ZHAO Mingyu et al. On the relation between coronal green line brightness and magnetic fields intensity[J]. Research in Astronomy and Astrophysics, 22, 075007(2022).
[11] SPYAK P R, WOLFE W L. Scatter from particulate-contaminated mirrors. part 3: theory and experiment for dust and lambda=10.6 μm[J]. Optical Engineering, 31, 1764-1774(1992).
[12] PETTIT R, FREESE J. Wavelength dependent scattering caused by dust accumulation on solar mirrors[J]. Solar Energy Materials, 3, 1-20(1980).
[13] YOUNG R. Low-scatter mirror degradation by particle contamination[J]. Optical Engineering, 15, 516-520(1976).
[14] LIU Yu. Coronal magnetic fields inferred from IR wavelength and comparison with EUV observations[J]. Annales Geophysicae, 27, 2771-2777(2009).
[15] LIU Yu, LIN Haosheng. Observational test of coronal magnetic field models. I. Comparison with potential field model[J]. The Astrophysical Journal, 680, 1496(2008).
[16] LIU Y, LIN H, KUHN J. Coronal magnetic fields from the inversion of linear polarization measurements[J]. Proceedings of the International Astronomical Union, 5, 96-98(2009).
[17] OTSU N. A threshold selection method from gray-level histograms[J]. IEEE Transactions on Systems, Man, Cybernetics, 9, 62-66(1979).
[18] LIU Zhong, DENG Yuanyong, YANG Dehua et al. Chinese giant solar telescope[J]. Scientia Sinica Physica, Mechanica & Astronomica, 49, 35-43(2019).
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Feiyang SHA, Yu LIU, Xuefei ZHANG, Tengfei SONG, Hongqi ZHANG, Yongfeng WANG, Mingzhe SUN. Stray Light by Dust on Objective Surface Based on Lijiang 10 cm Coronagraph[J]. Acta Photonica Sinica, 2023, 52(5): 0552213
Category: Special Issue for Advanced Science and Technology of Astronomical Optics
Received: Mar. 3, 2023
Accepted: Mar. 30, 2023
Published Online: Jul. 19, 2023
The Author Email: Yu LIU (lyu@ynao.ac.cn)