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Calibration of the Solar X-ray Detector on-board the Macao Science Satellite-1B for Soft X-ray Detection

  • Man-Hei Ng,
  • Xiaoping Zhang,
  • Jianwu Chen,
  • Yongqiang Shi,
  • Fuchang Zuo,
  • Wenxi Peng,
  • Weichun Fu,
  • Liansheng Li,
  • Pengwei Luo,
  • Chi-Long Tang,
  • Guozheng Zhang,
  • Zhiwu Mei,
  • Li Wang,
  • Cunhui Li,
  • Jiaming Ou,
  • Yanyan Xu

摘要

The Solar X-ray Detector (SXD) on-board the Macao Science Satellite-1B (MSS-1B) was successfully launched via the Chinese Long March-2C rocket on 21 May 2023, and commenced operations in early June of the same year. The MSS-1B/Soft X-ray Detection Units (SXDUs) employ two silicon drift detectors (SDDs), providing a wide range of energy spectra spanning from 0.7 to 24 keV. Notably, the SXDUs deliver a high-resolution capability of 0.14 keV@5.9 keV and operate with a time cadence of 1 second. Here, we perform thorough calibrations of the MSS-1B/SXDUs, employing a combination of ground experiments and simulations. In addition, quantitative analysis comparing the flux measurements obtained by the MSS-1B/SXDUs to the data collected by the Geostationary Operational Environmental Satellite (GOES), provides compelling evidence of their consistency. Furthermore, the preliminary spectral analysis results showcase the robustness and expected performance of the MSS-1B/SXDUs, unlocking their potential for facilitating the study of dynamic evolution of solar flares. Moreover, the innovative MSS-1B/Solar X-ray Detector facilitates concurrent observations of solar soft and hard X-rays, thereby making valuable contributions to the advancements in solar research.