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RASI:the Robotic All-Sky narrowband Imager
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作者 Yuxin Xin baoli lun +6 位作者 Zejun Hu Yue Zhong Kai Ye Hongying Xu Yufeng Fan Bin Li Dehong Huang 《Astronomical Techniques and Instruments》 2025年第6期348-357,共10页
We report a new standalone Robotic All-Sky narrowband Imager(RASI)for auroral and airglow studies.RASI has new optics and an electromechanical system,low operation and installation costs,easy deployment and fully auto... We report a new standalone Robotic All-Sky narrowband Imager(RASI)for auroral and airglow studies.RASI has new optics and an electromechanical system,low operation and installation costs,easy deployment and fully automatic features.The new optics provide an all-sky field of view with excellent image quality and sensitivity.The new electromechanical system design offers a more compact size and the capability for outdoor independent deployment.We have also developed a fully automatic data acquisition software for RASI,which is based on the perception of solar altitude and the all-sky cloud cover.In conclusion,the RASI demonstrates significant advantages over the traditional all-sky narrowband imager,and it is highly suitable for the intensity measurements of large-scale auroras and airglow distributions. 展开更多
关键词 ROBOTIC All-sky imager AURORAS AIRGLOW Optical imaging
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Observations of the solar corona during the total solar eclipse on 21 August 2017
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作者 Hui Tian ZhongQuan Qu +15 位作者 YaJie Chen LinHua Deng ZhengHua Huang Hao Li Yue Zhong Yu Liang JingWen Zhang YiGong Zhang baoli lun XiangMing Cheng XiaoLi Yan ZhiKe Xue YuXin Xin ZhiMing Song YingJie Zhu Tanmoy Samanta 《Earth and Planetary Physics》 2017年第1期68-71,共4页
The Sun’s tenuous outer atmosphere,the corona,emits only about one-millionth as much light as the solar surface.In ancient times the corona was observed by human beings only during total solar eclipses,when the stron... The Sun’s tenuous outer atmosphere,the corona,emits only about one-millionth as much light as the solar surface.In ancient times the corona was observed by human beings only during total solar eclipses,when the strong emission of visible light from the photosphere was completely blocked by the Moon.In 1931, 展开更多
关键词 solar corona solar eclipse solar magnetic fields coronal heating
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