Xiaohong Liu
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Xiaohong Liu has a total of 25 co-authors. Here are the top co-authors by number of shared publications:
- Jinghua Mao
National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
4 shared publications - Pengda Li
National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
4 shared publications - Yongmei Wang
Laboratory of Space Environment Exploration, National Space Science Center, Beijing 100190, China
4 shared publications - Zhuo Zhang
National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China
4 shared publications - Entao Shi
Laboratory of Space Environment Exploration, National Space Science Center, Beijing 100190, China
2 shared publications - Guojun Du
Beijing Institute of Space Mechanics & Electricity, Beijing 100194, China
2 shared publications
Latest Publications
- Open Access
- 7 May 2026
- Published by MDPI AG in Remote Sensing
- Vol. 18 (10) , 1456
Pre-Launch Calibration and Performance Evaluation of OMS-N Onboard the FY-3F Satellite
The Ozone Monitor Suite-Nadir (OMS-N) onboard the FY-3F satellite is a key payload for global atmospheric ozone and trace gas detection. The data quality depends on the accuracy of ground calibration. This study presents a systematic ground calibration of OMS-N. The instrument operates over 250–500 nm, with a spatial resolution of 7 × 7 km2 and a spectral resolution of 0.5–1 nm. Radiometric calibration was performed using an integrating sphere, spectral calibration using a tunable laser, and geometric calibration using a precision turntable. All tests were conducted under controlled environmental conditions (20 ± 3 °C and 50% ± 10% humidity). The absolute radiometric calibration uncertainty was below 2.33% for UV1/UV2 and 1.69% for VIS, with relative uncertainties ≤1.84%. The spectral wavelength error was ≤0.01 nm for the VIS channel and ≤0.03 nm for the UV1/UV2 channels, and the geometric positioning uncertainty was better than 0.1 pixels. All performance indicators met or exceeded the design requirements. These results provide technical support for the quantitative application of OMS-N data in atmospheric monitoring and establish a reference framework for the ground calibration of similar ultraviolet hyperspectral instruments.
- 7 May 2026
- Published by MDPI AG in Remote Sensing
- Vol. 18 (10) , 1456
Open AccessPre-Launch Calibration and Performance Evaluation of OMS-N Onboard the FY-3F Satellite
The Ozone Monitor Suite-Nadir (OMS-N) onboard the FY-3F satellite is a key payload for global atmospheric ozone and trace gas detection. The data quality depends on the accuracy of ground calibration. This study presents a systematic ground calibration of OMS-N. The instrument operates over 250–500 nm, with a spatial resolution of 7 × 7 km2 and a spectral resolution of 0.5–1 nm. Radiometric calibration was performed using an integrating sphere, spectral calibration using a tunable laser, and geometric calibration using a precision turntable. All tests were conducted under controlled environmental conditions (20 ± 3 °C and 50% ± 10% humidity). The absolute radiometric calibration uncertainty was below 2.33% for UV1/UV2 and 1.69% for VIS, with relative uncertainties ≤1.84%. The spectral wavelength error was ≤0.01 nm for the VIS channel and ≤0.03 nm for the UV1/UV2 channels, and the geometric positioning uncertainty was better than 0.1 pixels. All performance indicators met or exceeded the design requirements. These results provide technical support for the quantitative application of OMS-N data in atmospheric monitoring and establish a reference framework for the ground calibration of similar ultraviolet hyperspectral instruments.
- Open Access
Characteristic Evaluation of an Intensifier Detector for SMILE UVI
As one of the payloads on board the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) spacecraft, the ultraviolet imager (UVI) aims to capture N2 Lyman–Birge–Hopfield (LBH) aurora continuously on a high-eccentricity orbit. The UVI instrument includes an intensified charge-coupled device (ICCD) for far ultraviolet (FUV) wavelength. It comprises a sealed image intensifier, a relay lens system, a CCD, and a mechanical housing. ICCD’s performance characteristics are evaluated before integrating with the optical system of the UVI, including the quantum efficiency, radiant gain, background characteristics, excess noise factor, image quality, and signal-to-noise ratio (SNR). The testing procedure and results are presented and discussed. The results demonstrate that the comprehensive performance of the detector is good, and provide critical technical support for quantitative applications.
Open AccessCharacteristic Evaluation of an Intensifier Detector for SMILE UVI
As one of the payloads on board the Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) spacecraft, the ultraviolet imager (UVI) aims to capture N2 Lyman–Birge–Hopfield (LBH) aurora continuously on a high-eccentricity orbit. The UVI instrument includes an intensified charge-coupled device (ICCD) for far ultraviolet (FUV) wavelength. It comprises a sealed image intensifier, a relay lens system, a CCD, and a mechanical housing. ICCD’s performance characteristics are evaluated before integrating with the optical system of the UVI, including the quantum efficiency, radiant gain, background characteristics, excess noise factor, image quality, and signal-to-noise ratio (SNR). The testing procedure and results are presented and discussed. The results demonstrate that the comprehensive performance of the detector is good, and provide critical technical support for quantitative applications.
- Open Access
- 3 September 2023
- Published by MDPI AG in Remote Sensing
- Vol. 15 (17) , 4343
In-Flight Preliminary Performance of GF-5B/Absorbing Aerosol Sensor
The Absorbing Aerosol Sensor (AAS) is carried on the Gao-Fen 5B (GF-5B) satellite, and it allows for the measurement of solar backscatter radiation by the atmosphere in the UV–Vis bands. The AAS is an imaging spectrometer that employs CCD for capturing both a continuous spectrum and the cross-track orientation with a 114° wide swath. The broad field of view provides daily global envelopment with a 4 km spatial resolution at the nadir. This paper mainly analyzes the initial working status of the instrument in orbit, including wavelength calibration, radiometric calibration, detector performance, and product availability. Preliminary observations indicate the ability of the AAS to monitor absorbing aerosols like dust, biomass burning, volcano ash, and some pollution aerosols and to identify the aerosol events in China and other regions with high spatial resolution.
- 3 September 2023
- Published by MDPI AG in Remote Sensing
- Vol. 15 (17) , 4343
Open AccessIn-Flight Preliminary Performance of GF-5B/Absorbing Aerosol Sensor
The Absorbing Aerosol Sensor (AAS) is carried on the Gao-Fen 5B (GF-5B) satellite, and it allows for the measurement of solar backscatter radiation by the atmosphere in the UV–Vis bands. The AAS is an imaging spectrometer that employs CCD for capturing both a continuous spectrum and the cross-track orientation with a 114° wide swath. The broad field of view provides daily global envelopment with a 4 km spatial resolution at the nadir. This paper mainly analyzes the initial working status of the instrument in orbit, including wavelength calibration, radiometric calibration, detector performance, and product availability. Preliminary observations indicate the ability of the AAS to monitor absorbing aerosols like dust, biomass burning, volcano ash, and some pollution aerosols and to identify the aerosol events in China and other regions with high spatial resolution.
- Open Access
- 31 July 2023
- Published by MDPI AG in Preprints.org
In-flight Preliminary Performance of GF-5B/Absorbing Aerosol Sensor
The Absorbing Aerosol Sensor (AAS) is carried on the Gao Fen 5B (GF-5B) satellite, which allows for measuring the solar backscatter radiation by the atmosphere in UV-VIS wavelength. AAS is an imaging spectrometer using CCD for capturing both continuous spectrum and the cross-track orientation with a 114° wide swath. The broad field-of-view provides daily global envelopment with a 4 km spatial resolution at the nadir. This paper mainly analyzed the initial working status of the instrument in orbit, including wavelength calibration, radiation calibration, detector performance, and product availability. Preliminary observations indicate that the AAS can monitor the absorbing aerosol like dust, biomass burning, volcano ash, and some pollution aerosol and can identify the aerosol events in China and other regions with high spatial resolution.
- 31 July 2023
- Published by MDPI AG in Preprints.org
Open AccessIn-flight Preliminary Performance of GF-5B/Absorbing Aerosol Sensor
The Absorbing Aerosol Sensor (AAS) is carried on the Gao Fen 5B (GF-5B) satellite, which allows for measuring the solar backscatter radiation by the atmosphere in UV-VIS wavelength. AAS is an imaging spectrometer using CCD for capturing both continuous spectrum and the cross-track orientation with a 114° wide swath. The broad field-of-view provides daily global envelopment with a 4 km spatial resolution at the nadir. This paper mainly analyzed the initial working status of the instrument in orbit, including wavelength calibration, radiation calibration, detector performance, and product availability. Preliminary observations indicate that the AAS can monitor the absorbing aerosol like dust, biomass burning, volcano ash, and some pollution aerosol and can identify the aerosol events in China and other regions with high spatial resolution.
- 1 January 2022
- Published by National Space Science Center, Chinese Academy of Sciences in Chinese Journal of Space Science
- Vol. 42 (6) , 1204-1209
Design and Realization of the Ultra-violet Imager Communication and Control System Based on Packet Utilization Standard
在中国传统航天器中,通信系统格式通常各不相同。随着载荷越来越复杂,通信系统的格式往往需要重建,而且由于缺乏灵活性,会产生许多限制。对于SMILE卫星中的紫外极光成像仪(UVI)工程任务, 为与国际对接,提高数据处理的效率,设计实现了基于遥控遥测包应用标准(PUS)的通信与控制系统,根据通信与控制系统的构成及工作原理,PUS业务的选择和实现,对通信功能进行设计,按照PUS标准完成遥测遥控功能,并基于PUS业务提出故障诊断和处理方法。通过对系统进行集成测试,结果表明电控箱通信与控制系统工作稳定,能够完成指令处理、科学数据接收存储、故障诊断以及多种数据包发送,满足任务需求。
- 1 January 2022
- Published by National Space Science Center, Chinese Academy of Sciences in Chinese Journal of Space Science
- Vol. 42 (6) , 1204-1209
Design and Realization of the Ultra-violet Imager Communication and Control System Based on Packet Utilization Standard
在中国传统航天器中,通信系统格式通常各不相同。随着载荷越来越复杂,通信系统的格式往往需要重建,而且由于缺乏灵活性,会产生许多限制。对于SMILE卫星中的紫外极光成像仪(UVI)工程任务, 为与国际对接,提高数据处理的效率,设计实现了基于遥控遥测包应用标准(PUS)的通信与控制系统,根据通信与控制系统的构成及工作原理,PUS业务的选择和实现,对通信功能进行设计,按照PUS标准完成遥测遥控功能,并基于PUS业务提出故障诊断和处理方法。通过对系统进行集成测试,结果表明电控箱通信与控制系统工作稳定,能够完成指令处理、科学数据接收存储、故障诊断以及多种数据包发送,满足任务需求。