Pre-launch characterization of the spectrometer of Hard X-ray Imager (HXI) onboard the ASO-S mission. (1st May 2022)

• Record Type: Journal Article
• Authors: Liu, W.; Zhang, Z.; Wu, J.; Ma, T.; Zhang, Y.; Hu, Y.M.; Zhang, Y.Q.; Huang, Y.Y.; Wang, H.X.; Jiang, X.K.; Chen, D.Y.
• Is Part Of: Journal of instrumentation. Volume 17:Number 5(2022)
• Publication Date: 2022-05-01
• Subjects: Detector alignment and calibration methods (lasers, sources, particle-beams) -- Spectrometers -- X-ray detectors and telescopes; Scientific apparatus and instruments -- Periodicals; 502.84
• DOI: 10.1088/1748-0221/17/05/P05045
• Languages: English
• ISSNs: 1748-0221

Abstract

Abstract: As one of the three payloads of the Advanced Space-based Solar Observatory (ASO-S), the pre-launch characterization of HXI includes the characterization of the collimator and the spectrometer. This article focuses on the pre-launch characterization of HXI's spectrometer, including detection efficiency, energy resolution, and energy to ADC channel (E-C) relationship. The detection efficiency characterization necessitates a sufficient number of calibrated energy points in the HXI observation energy range, with a refined measurement around the absorption edge of the lanthanum bromide crystal, and is calibrated with an X-ray beam. The characterization results are consistent with the simulations and show that the detection efficiency difference between detector modules is controlled within ±3%. Radioactive sources 133 Ba and 137 Cs are used to calibrate the energy resolution and E-C relationship. The characterization results show that all detector modules' energy resolutions are better than 26% at 32 keV, meeting the design specification. And their E-C relationships vary regularly with voltage. All of the characterization results indicate that the flight model of the HXI spectrometer meets the performance requirements and is capable of performing on-orbit observation activities.