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The release of the first batch of scientific images of solar observation of "Kuafu I" has achieved many firsts at home and abroad

2022-12-13   

On December 13, the press conference for the first batch of scientific images of the Chinese comprehensive solar exploration satellite "Kuafu I" was held at the National Space Science Center of the Chinese Academy of Sciences in Huairou Science City, Beijing. Since the successful launch of "Kuafu 1" on October 9, 2022, several scientific observation images of the sun obtained by the three payloads during the two months of operation in orbit have been officially announced. The latest results have achieved many firsts at home and abroad, and the observation ability and progressiveness of the three payloads of "Kuafu 1" have been verified in orbit. The picture shows a comparison between the hard X-ray imaging of a C-level flare observed by "Kuafu I" HXI in "Double 11" on November 11, 2022 and the AIA/SDO ultraviolet 1700 image. The local monochromatic image and magnetic map (right) observed by the "Kuafu I" FMG in orbit are compared with the results of Huairou ground full helion magnetic field telescope (left) at the same time and in the same helion area. Comparison between the local longitudinal magnetic map (right) of 00:50:15UT observed by the FMG of "Kuafu 1" on November 6, 2022 and the observation results of American HMI/SDO (left) at the same time. On November 7, "Kuafu 1" WST/LST observed a white flare, and the red isoline on the right is the position of the continuous spectral enhancement relative to the sunspot. The eruptive prominence observed by "Kuafu I" SDI/LST on November 25, 2022. Photometric, hard X-ray imaging of the "Double 11" series flares observed by "Kuafu I" HXI on November 11, and composite images of the extreme ultraviolet/ultraviolet images with AIA/SDO. (Liu Xinshe)

Edit:Ying Ying Responsible editor:Wang Chen

Source:www.chinanews.com.cn

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