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Progress Report on ASO-S: 2024-2026

SU Yang GAN Weiqun

SU Yang, GAN Weiqun. Progress Report on ASO-S: 2024-2026. Chinese Journal of Space Science, 2026, 46(4): 1-5 doi: 10.11728/cjss2026.04.2026-yg08
Citation: SU Yang, GAN Weiqun. Progress Report on ASO-S: 2024-2026. Chinese Journal of Space Science, 2026, 46(4): 1-5 doi: 10.11728/cjss2026.04.2026-yg08

Progress Report on ASO-S: 2024-2026

doi: 10.11728/cjss2026.04.2026-yg08 cstr: 32142.14.cjss.2026-yg08
Funds: Funded by XDB0560000, XDA15320000, 2022 YFF0503000, NSFC 12333010, NSFC 12233012, NSFC 11921003
More Information
    Author Bio:

    Male, born in Tai’an, Shandong on April 10, 1982, is currently a research fellow and lead scientist for ASO-S science at Purple Mountain Observatory, Chinese Academy of Sciences. He is also ASO-S/HXI payload scientist and data scientist. His research focuses on solar physics, hard X-ray imaging and related space astronomy. E-mail: yang.su@pmo.ac.cn

  • Figure  1.  This screenshot displays the interactive HXI flare list with comprehensive panels of flare parameters, HXI quicklook data, selection tools, EOVSA data, SDO/AIA images, etc.

    Figure  2.  Composite image presents the simultaneous eruptions of two prominences observed in Lyα by ASO-S/LST payload on 21 Sept. 2025

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    [2] GAN W Q, FENG L, SU Y. A Chinese solar observatory in space[J]. Nature Astronomy, 2022, 6(1): 165 doi: 10.1038/s41550-021-01593-9
    [3] GAN W Q, ZHU C, CHEN B, et al. China’s first comprehensive space solar observatory[J]. Chinese Astronomy and Astrophysics, 2023, 47(2): 441-445 doi: 10.1016/j.chinastron.2023.06.002
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    [9] BAI X Y, DENG Y Y, ZHANG H Y, et al. Calibration and performance of the Full−disk vector MagnetoGraph (FMG) on board the advanced space−based solar observatory (ASO−S)[J]. Solar Physics, 2024, 299(11): 157
    [10] SU Y, ZHANG Z, CHEN W, et al. The tests and calibrations of the hard X−ray imager aboard ASO−S[J]. Solar Physics, 2024, 299(10): 153 doi: 10.1007/s11207-024-02392-x
    [11] CHEN B, FENG L, ZHANG G, et al. Inflight performance and calibrations of the Lyman-alpha solar telescope on board the advanced space-based solar observatory[J]. Solar Physics, 2024, 299(8): 118 doi: 10.1007/s11207-024-02354-3
    [12] HUANG Y, LI Y P, LIU S, et al. Science operation and data analysis center of the advanced space−based solar observatory (ASO−S) mission[J]. Solar Physics, 2024, 299(9): 135 doi: 10.1007/s11207-024-02368-x
    [13] CHEN J, WIEGELMANN T, FENG L, et al. FastQSL 2: a comprehensive toolkit for magnetic connectivity analysis[J]. SCIENCE CHINA Physics, Mechanics & Astronomy, 2023, 66(1): 15
    [14] LI S T, FENG L, YING B L, et al. Carrington maps in H I Lyα and their relationships with extreme-ultraviolet and magnetic-field maps[J]. The Astrophysical Journal Letters, 2024, 969(1): L16 doi: 10.3847/2041-8213/ad5679
    [15] WANG R, HU H D, ZHAO X W, et al. A major geomagnetic storm in 2024 October linked to sympathetic coronal mass ejection─prominence eruptions[J]. The Astrophysical Journal Letters, 2026, 1002(1): L23 doi: 10.3847/2041-8213/ae5801
    [16] CHEN C X, SU Y, CHEN W, et al. Intense hard X-ray emissions in C-class flares: a statistical study with ASO-S/HXI data[J]. The Astrophysical Journal Letters, 2025, 987(1): L4 doi: 10.3847/2041-8213/addf2f
    [17] GAN Weiqun, SU Yang, FENG Li, et al. Brief review on early achievements of ASO-S in orbit[J]. Science & Technology Review, 2025, 43(16): 43-61 doi: 10.3981/j.issn.1000-7857.2025.02.00203
    [18] JING Z C, LI Y, FENG L, et al. A statistical study of solar white-light flares observed by the white-light solar telescope of the Lyman-alpha solar telescope on the advanced space-based solar observatory (ASO-S/LST/WST) at 360 nm[J]. Solar Physics, 2024, 299(2): 11 doi: 10.1007/s11207-024-02251-9
    [19] JING Z C, LI Y, LI J W, et al. The M- and X-class white-light flares in super active region NOAA 13664/13697 observed by ASO-S/LST/WST[J]. The Astrophysical Journal, 2025, 992(1): 72 doi: 10.3847/1538-4357/ae0708
    [20] LI D, HONG Z X, HOU Z Y, et al. Localizing quasiperiodic pulsations in hard X-ray, microwave, and Lyα emissions of an X6.4 flare[J]. The Astrophysical Journal, 2024, 970(1): 77 doi: 10.3847/1538-4357/ad566c
    [21] LI D. Localizing short-period pulsations in hard X-rays and γ-rays during an X9.0 flare[J]. Astronomy & Astrophysics, 2025, 695: L4 doi: 10.1051/0004-6361/202453613
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    [23] RYAN D F, MASSA P, BATTAGLIA A F, et al. Triangulation of hard X-ray sources in an X-class solar flare with ASO-S/HXI and solar orbiter/STIX[J]. Solar Physics, 2024, 299(8): 114 doi: 10.1007/s11207-024-02341-8
    [24] MROZEK T, LI Z T, KARLICKÝ M, et al. Kink-and-disconnection failed eruption in 3D[J]. Solar Physics, 2024, 299(6): 81 doi: 10.1007/s11207-024-02325-8
    [25] Palumbo B, Massa P, Stiefel M Z, et al. 3D reconstruction of thermal hard X-ray sources in solar flares from combined STIX and HXI visibilities. Astronomy & Astrophysics, 2026, 710: A105
    [26] ZHANG Q M, PAN W W, YING B L, et al. Tracking an eruptive intermediate prominence originating from the farside of the sun[J]. The Astrophysical Journal, 2025, 985(2): 237 doi: 10.3847/1538-4357/add328
    [27] HU Z Y, JI K F, CHEN J, et al. Calibration scheme for space-borne full-disk vector magnetograph under the influence of orbiter velocity[J]. Astronomy & Astrophysics, 2022, 666: A93 doi: 10.1051/0004-6361/202142920
    [28] HU Z Y, JI K F, BAI X Y, et al. Nonlinear calibration method for FMG line-of-sight magnetic field[J]. Universe, 2025, 11(4): 108 doi: 10.3390/universe11040108
    [29] XIA Y H, SU Y, LIU H, et al. A new solar hard X−ray image reconstruction algorithm for ASO−S/HXI based on deep learning[J]. Solar Physics, 2024, 299(11): 158 doi: 10.1007/s11207-024-02399-4
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出版历程
  • 收稿日期:  2026-05-20
  • 网络出版日期:  2026-07-26

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