Zobrazeno 1 - 10
of 15
pro vyhledávání: '"Jilong Peng"'
Autor:
Mengfei Yang, Jingxiu Wang, Chi Wang, Qiugang Zong, Xiaoxin Zhang, Shuwu Dai, Yuanyong Deng, Xueshang Feng, Ying Wang, Chenglin Zhu, Yechi Zhang, Qingxiang Zhang, Fenggang Shen, Baiyi Tian, Wenyan Zhou, Linling Li, Yihua Yan, Guiping Zhou, Shangbin Yang, Ming Xiong, Aibing Zhang, Jiansen He, Hui Tian, Jiawei Li, Weiqun Gan, Lidong Xia, Jilong Peng, Changning Huang, Jie Jiang, Lin Quan
Publikováno v:
Chinese Science Bulletin. 68:859-871
Publikováno v:
AOPC 2019: Space Optics, Telescopes, and Instrumentation.
Performances of a novel solar extreme ultraviolet (EUV) slitless imaging spectrometer in a stigmatic design are presented with an aberration-correcting flat-field holographic concave grating (HCG). The instrument is based on a conventional off-axis M
Publikováno v:
Proceedings of SPIE; 2/8/2020, Vol. 11341, p1-7, 7p
Publikováno v:
Proceedings of SPIE; 2/8/2020, Vol. 11341, p1-6, 6p
Publikováno v:
Fourth Seminar on Novel Optoelectronic Detection Technology and Application.
Far ultraviolet earth night airglow is related to total electron content(TEC) of Ionosphere. Observing the night airglow nadir at OI 135.6nm emission produced by ionospheric O+ and e recombination can get the distribution of ionosphere TEC. In this p
Publikováno v:
2017 International Conference on Optical Instruments and Technology: IRMMW-THz Technologies and Applications.
Aluminum reflector, especially OAP (Off-Axis Parabolic) reflector, has been widely used in terahertz and infrared systems for its low cost, lightweight, good machinability, small size, simple structure, and having the same thermal expansion and contr
Publikováno v:
2017 International Conference on Optical Instruments and Technology: Optoelectronic Measurement Technology and Systems.
For the space solar extreme ultraviolet telescope, the star point test can not be performed in the x-ray band (19.5nm band) as there is not light source of bright enough. In this paper, the point spread function of the optical system is calculated to
Autor:
Yongmei Wang, Peng Ruyi, Xiaoyin Li, Shi Entao, Nan Jia, Liping Fu, Fang Jiang, Wang Tianfang, Jilong Peng
Publikováno v:
Astrophysics and Space Science. 355:1-7
Far Ultraviolet Nighttime Ionopsheric Photometer (FNIP) is a newly-designed instrument for low earth orbit missions, observing the earth night airglow nadir at OI 135.6 nm emission produced by ionospheric O++e recombination and receiving the horizont
Autor:
Bo Chen, Fei Wei, Jie Liu, Huaan Lin, Wang Shijin, Jilong Peng, Ke‐Ping Qiu, Zhu Guangwu, Baoquan Li, Chang‐Sheng Ma, Yan Gong, Yu‐Hua Tang, Ling‐Gao Kong, Jing‐Hong Shao
Publikováno v:
Chinese Journal of Geophysics. 48:257-265
The Solar X-EUV imaging telescope (XEIT), which operates in the 4-100Awavelength bands and the 195A EUV emission line, is designed to monitor and predict solar activities resulting in variations of space weather. The XEIT is dedicated to space weathe
Publikováno v:
SPIE Proceedings.
The space solar EUV and X ray imaging camera is the core of the solar EUV and X ray imaging telescope, which is designed to monitor and predict solar activities, such as CMEs, flare and coronal hole. This paper presents a comprehensive description of