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中国科学院 长春光学精密机械与物理研究所,吉林 长春 130033
[ "王蕴琦(1990-),男,吉林长春人,助理研究员,2018年于中国科学院长春光学精密机械与物理研究所获得博士学位,主要从事光学系统设计与光学检测技术方面的研究。E-mail:wangyunqi0808@163.com" ]
陈波(1961-),男,吉林长春人,研究员,主要从事X射线-紫外波段的光学研究。E-mail:chenb@ciomp.ac.cn CHEN Bo, E-mail:chenb@ciomp.ac.cn
收稿日期:2019-06-27,
修回日期:2019-08-17,
录用日期:2019-8-17,
纸质出版日期:2020-02-15
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王蕴琦, 张广, 何玲平, 等. Lymanα与可见光双波段内掩式日冕仪[J]. 光学精密工程, 2020,28(2):303-314.
Yun-qi WANG, Guang ZHANG, Ling-ping HE, et al. Solar coronagraph imager based on internal occulting in Lyman-alpha and visible bands[J]. Optics and precision engineering, 2020, 28(2): 303-314.
王蕴琦, 张广, 何玲平, 等. Lymanα与可见光双波段内掩式日冕仪[J]. 光学精密工程, 2020,28(2):303-314. DOI: 10.3788/OPE.20202802.0303.
Yun-qi WANG, Guang ZHANG, Ling-ping HE, et al. Solar coronagraph imager based on internal occulting in Lyman-alpha and visible bands[J]. Optics and precision engineering, 2020, 28(2): 303-314. DOI: 10.3788/OPE.20202802.0303.
太阳是地球能量的主要来源,太阳活动和变化对地球影响极大。为了满足天文学家对太阳观测和研究的需求,设计一种新型Lyman α和可见光双波段内掩式日冕仪(SCI日冕仪),能够在121.6 nm和700 nm两个波段同时对日冕进行高分辨率成像观测。根据太阳在121.6 nm和700 nm日面与日冕的辐射特性确定仪器的参数,给出了日冕仪的初始结构,建立评价函数对初始结构进行优化。分析了日冕仪光学系统的成像性能和各个光学元件产生杂散光对成像性能的影响,确定影响系统杂散光抑制水平的主要光学元件和机械结构,提出了对光学元件表面粗糙度的要求,给出了里奥光阑的位置和通光口径。还设计了日冕仪光学反射镜和光学分色镜的膜系结构,实现了对内日冕在121.6 nm和700 nm两个波段的同时成像。实验结果表明:SCI日冕仪视场覆盖1.1~2.5个太阳半径(Rs
取1 Rs=0.267°),空间分辨率优于4.8″,杂散光抑制水平在1.1Rs处优于10
-6
量级,在2.5Rs处优于10
-8
量级
满足观测需求。
The sun is the main source of Earth's energy. As such solar activity and changes have a great influence on the Earth. To meet the solar observation and research needs of astronomers
a new type of Lyman alpha and visible dual-band internal occulting coronagraph was designed to meet the needs of high-resolution imaging observation of the corona at 121.6 nm and 700 nm for space. Firstly
the parameters of the instrument were determined according to the radiation characteristics of the solar disc and corona in the 121.6 nm and 700 nm bands and the initial structure of the coronagraph was given. The initial structure was optimized by an evaluation function. The imaging performance of the coronagraph optics was calculated and the influence of various optical elements on stray light was analyzed. The main optical components and mechanical structure affecting stray light were determined and the position and surface treatment method of a Lyot stop were designed. The coating film structure of the optical components and optical chromoscope of the coronagraph were designed to achieve simultaneous imaging in the 121.6 nm and 700 nm bands. The design and analysis results show that the field of view (FOV) of the coronagraph covers a 1.1 (Rs=0.267 degrees) to 2.5 solar radius
the effective focal length of the system is 945 mm
the spot radius root mean square (RMS) of the entire field of view is less than 10 um
and the angular resolution is better than 4.8 arcsec. The stray light suppression level of the system is better than 10
-6
at 1.1 Rs and 10
-8
at 2.5 Rs.
SOCKER D G, BRUECKNER G E, KORENDYKE C M, et al .. Spectrometric and spectropolarimetric observation of the solar corona with the LASCO/SOHO Lyot coronagraph[C]. SPIE's 1994 International Symposium on Optics , Imaging , and Instrumentation. Proc SPIE 2283, X-Ray and Ultraviolet Spectroscopy and Polarimetry , San Diego , CA , USA , 1994: 53-57.
VIVES S, LAMY P L, VIAL J C. Optical design of the Lyman alpha coronagraph for the LYOT microsatellite[C]. Optical Science and Technology, SPIE's 48 th Annual Meeting. Proc SPIE 5171, Telescopes and Instrumentation for Solar Astrophysics , San Diego , California , USA , 2004: 298-306.
VIAL J C, SONG X Y, LEMAIRE P, et al .. The solar high-resolution imager: coronagraph LYOT mission[C]. Astronomical Telescopes and Instrumentation. Proc SPIE 4853, Innovative Telescopes and Instrumentation for Solar Astrophysics , Waikoloa , Hawai'i , USA , 2003: 479-489.
ENRICO V, DEPPO V D, GIAMPIERO N, et al .. Preliminary internal straylight analysis of the METIS instrument for the solar orbiter ESA mission[C]. SPIE Astronomical Telescopes + I nstrumentation. Proc SPIE 8442, Space Telescopes and Instrumentation 2012: Optical , Infrared , and Millimeter Wave , Amsterdam , Netherlands , 2012: 84424N.
POLITO V, J. CORSO A, ZUPPELLA P, et al .. Analysis of optical efficiency of METIS coronagraph telescope on board of the Solar Orbiter mission[C]. SPIE Astronomical Telescopes + Instrumentation. Proc SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray , Amsterdam , Netherlands , 2012: 84433G.
FINESCHI S, ANTONUCCI E, GIAMPIERO N, et al .. METIS: a novel coronagraph design for the Solar Orbiter mission[C]. SPIE Astronomical Telescopes + Instrumentation. Proc SPIE 8443, Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray , Amsterdam , Netherlands , 2012: 84433H.
PANCRAZZI M, FOCARDI M, USLENGHI M, et al .. On board processing procedures for the Solar Orbiter METIS coronagraph[C]. SPIE Remote Sensing. Proc SPIE 8892, Image and Signal Processing for Remote Sensing XIX , Dresden , Germany , 2013: 889218.
张 红鑫 , 卢 振武 , 夏 利东 , 等 . 白光日冕仪光学系统的杂散光抑制 . 光学 精密工程 , 2009 . 17 ( 10 ): 2371 - 2376 . http://www.eope.net/CN/abstract/abstract8938.shtml http://www.eope.net/CN/abstract/abstract8938.shtml .
H X ZHANG , ZH W LU , L D XIA , 等 . Stray light suppressing of optical system in white light coronagraph . Opt. Precision Eng. , 2009 . 17 ( 10 ): 2371 - 2376 . http://www.eope.net/CN/abstract/abstract8938.shtml http://www.eope.net/CN/abstract/abstract8938.shtml .
卜 和阳 , 卢 振武 , 张 红鑫 , 等 . 内掩式透射地基日冕仪中杂光鬼像的消除 . 中国光学 , 2013 . 6 ( 2 ): 231 - 236 . http://d.old.wanfangdata.com.cn/Periodical/zggxyyygxwz201302014 http://d.old.wanfangdata.com.cn/Periodical/zggxyyygxwz201302014 .
H Y BU , ZH W LU , H X ZHANG , 等 . Suppresion of stray light ghost image in internally occulting refractive ground-based coronagraph . Chinese Optics , 2013 . 6 ( 2 ): 231 - 236 . http://d.old.wanfangdata.com.cn/Periodical/zggxyyygxwz201302014 http://d.old.wanfangdata.com.cn/Periodical/zggxyyygxwz201302014 .
卜 和阳 , 张 红鑫 , 卢 振武 , 等 . 内掩式透射日冕仪中Lyot光阑参数分析 . 光学学报 , 2014 . 34 ( 12 ): 147 - 152 . http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=gxxb201412021 http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=gxxb201412021 .
H Y BU , H X ZHANG , ZH W LU , 等 . Analysis on the parameter of Lyot Stop in internally occulting refractive coronagraph . Acta Optica Sinica , 2014 . 34 ( 12 ): 147 - 152 . http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=gxxb201412021 http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=gxxb201412021 .
李 达 , 刘 鹏 , 陈 斌 , 等 . 球面反射式日冕仪实验装置的杂光分析和实验验证 . 光学 精密工程 , 2015 . 23 ( 5 ): 1265 - 1271 . http://www.eope.net/CN/abstract/abstract15796.shtml http://www.eope.net/CN/abstract/abstract15796.shtml .
D LI , P LIU , B CHEN , 等 . Stray light analysis and experimental verification of spherical reflective coronagraph experimental devices . Opt. Precision Eng. , 2015 . 23 ( 5 ): 1265 - 1271 . http://www.eope.net/CN/abstract/abstract15796.shtml http://www.eope.net/CN/abstract/abstract15796.shtml .
X D WANG , B CHEN , T L HUO , 等 . Design of second-order 121.6-nm narrowband minus filters using asymmetrically apodized thickness modulation . Applied Physics B , 2018 . 124 ( 7 ): 139 http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=8c68ddcbfb58e980f054443b3e968e59 http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=8c68ddcbfb58e980f054443b3e968e59 .
X Dang WANG , CHEN B Bo , T L HUO , 等 . Design of first-order 121.6 nm minus filters . Applied Spectroscopy , 2018 . 72 ( 10 ): 1498 - 1502 . http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=e1e98cd80c047c99a4e7777881d8aee4 http://www.wanfangdata.com.cn/details/detail.do?_type=perio&id=e1e98cd80c047c99a4e7777881d8aee4 .
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