Acta Optica Sinica, Volume. 41, Issue 5, 0512004(2021)
Radiation Calibration of All-Sky Auroral Imager Based on Stellar Radiation Stability
Fig. 1. Distribution of stars. (a) All-sky image of YRS; (b) star map in Stellarium
Fig. 2. Visual motion track of stars and diagram of calculating stellar coordinates. (a) 24 h visual motion track of Vega; (b) diagram of calculating stellar coordinate in all-sky image
Fig. 5. An event of DMSP F-16 satellite crossing all-sky field of view from 11:03:33 UT to 11:07:34 UT on December 2, 2005. (a) Trajectory of DMSP satellite projected onto all-sky images; (b) electron spectroscopy; (c) Keogram; (d) energy flux of precipitating electrons; (e) average energy of precipitating electrons; (f) auroral emission intensity
Fig. 6. An event of DMSP F-16 satellite crossing all-sky field of view from 10:49:50 UT to 10:52:20 UT on December 19, 2005. (a) Trajectory of DMSP satellite projected onto all-sky images; (b) electron spectroscopy; (c) Keogram; (d) energy flux of precipitating electrons; (e) average energy of precipitating electrons; (f) auroral emission intensity
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Bing Han, Guojun Li, Zejun Hu, Yisheng Zhang. Radiation Calibration of All-Sky Auroral Imager Based on Stellar Radiation Stability[J]. Acta Optica Sinica, 2021, 41(5): 0512004
Category: Instrumentation, Measurement and Metrology
Received: Sep. 11, 2020
Accepted: Nov. 2, 2020
Published Online: Apr. 7, 2021
The Author Email: Han Bing (bhan@xidian.edu.cn), Li Guojun (1556176733@qq.com), Hu Zejun (huzejun@pric.org.cn), Zhang Yisheng (zhangyisheng118@sina.com)