Abstract
The solar X-ray and Extreme Ultraviolet Imager (X-EUVI), which was developed by CIOMP, is China’s first space-based solar X-ray and Extreme Ultraviolet (EUV) imager; it has been loaded onto the Fengyun-3E Satellite, which is supported by the China Meteorological Administration (CMA), for solar observation. It commenced working on July 11, 2021, and was used to obtain the first X-ray and EUV images in China. X-EUVI employs an innovation dual band design to monitor a much larger temperature range across the Sun, covering the 0.6–8.0 nm wavelength band of the X-ray region and the 19.5 nm band of the EUV region.
Highlights
The solar X-ray and Extreme Ultraviolet Imager (X-EUVI), which was developed by CIOMP, is China’s first space-based solar X-ray and Extreme Ultraviolet (EUV) imager; it has been loaded onto the Fengyun-3E Satellite, which is supported by the China Meteorological Administration (CMA), for solar observation
This represents a breakthrough for solar observation in the X-ray and EUV regions in China, and images obtained from the X-EUVI will play an important role in solar research and space weather forecasting[1–5]
The X-EUVI was developed by the research team in CIOMP
Summary
The solar X-ray and Extreme Ultraviolet Imager (X-EUVI), which was developed by CIOMP, is China’s first space-based solar X-ray and Extreme Ultraviolet (EUV) imager; it has been loaded onto the Fengyun-3E Satellite, which is supported by the China Meteorological Administration (CMA), for solar observation. The team at Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences (CIOMP), developed X-EUVI, China’s first space-based solar X-ray and Extreme Ultraviolet (EUV) imager.
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