首席教授：舒嵘研究员

团队成员：徐卫明研究员，张锷研究员，许学森助理研究员，李鲁宁助理研究员，刘向锋助理研究员

联系人：许学森                联系方式：13164291307；xuxuesen@ucas.ac.cn

威斯尼斯人wns888入口中国上海技术物理研究所舒嵘研究员团队研制了月球与深空探测系列主动光电载荷，包括嫦娥系列红外光谱分析仪以及“祝融号”火星表面成分探测仪（MarSCoDe）等科学载荷。于2019年在威斯尼斯人wns888入口中国领衔成立了舒嵘教授工作室，工作室以行星科学学科建设为导向，科教融合发展为理念，聚焦行星物质成分探测技术，为研究月球/行星地质演化过程及探寻生命痕迹提供新方法。主要研究方向：（1）主被动光谱探测与分析；（2）遥感与行星科学数据处理与应用；（3）精密光谱测量新技术；（4）小天体探测新方法。

工作室组建了“行星环境模拟及原位探测实验室”，旨在通过实验室模拟空间环境和原位探测条件对科学载荷开展地面验证实验，利用“天­—地”数据的联用，提高科学数据定标准确度，能更准确的基于遥感光谱数据开展月球与行星物质成分识别和定量反演研究。实验室拥有行星表面环境模拟平台、火星MarSCoDe鉴定件、ASD便携式地物光谱仪、月壤无损存储和操作设备、模拟月球和行星土壤制备设备、BRDF多角度光谱测量设备、LTB-LIBS光谱仪、莱卡显微镜、远程拉曼光谱仪等设备，可以用于模拟月球和行星土壤的样品制备，利用多种光谱手段开展模拟行星表面环境的科学实验。

工作室目前正在承担中国空间站时频柜空间飞秒光梳研制、参与嫦娥七号拉曼光谱仪项目研制，并且在Nature、Spectrochimica Acta Part B、Space Science Reviews等期刊上发表论文12篇。

工作室有着开放、创新、融合的学术科研氛围，与威斯尼斯人wns888入口中国、高校（含港澳）及法国图卢兹大学天体和行星研究所(IRAP)等相关科研团队开展科研合作，欢迎有志于中国行星科学发展的你加入我们。

Professor Shu Rong’s team at Shanghai Institute of Technical Physics, Chinese Academy of Sciences has led the development of a series of lunar and deep space exploration spectroscopic scientific payloads, including Chang’E series infrared spectrum analyze and the Mars Surface Composition Detector (MarSCoDe) in China’s first Mars exploration mission. Professor Shu led the establishment of Professor Shu Rong’s Studio in Hangzhou Institute for Advanced Study (HIAS) in 2019. Oriented by the discipline construction of planetary science, and holding the idea of integrated development of science and education, the studio focuses on the detection technology of planetary material composition, providing a new method for studying the geological evolution process of the moon/planet and exploring the traces of life. The main research directions of the studio include: (1) Active and passive spectrum detection and analysis; (2) Processing and application of planetary remote sensing scientific data; (3) New technology for fine spectral measurement; (4) New methods for small celestial body exploration.

The Planetary Environment Simulation and in-situ Detection Laboratory at HIAS aims to carry out ground verification experiments on scientific payloads by utilizing the simulated space environment and the in-situ detection equipment. Based on the combination of remote sensing and laboratory data, the calibration accuracy of the scientific data is expected to be improved. Hence the composition identification / quantification based on the remote sensing spectral data can be more accurate and efficient. At present, the studio owns a space environment simulating facility, a MarSCoDe duplicate model, a spectrometer (ASD TerraSpec 4 Hi-Res), nondestructive storage and operation equipment for lunar soil, simulated lunar soil and planetary soil preparation equipment, BRDF multi-angle spectroscopic measurement devices, a LIBS system (LTB), a remote Raman system, Leica microscope, etc. Therefore the studio team is able to prepare lunar and planetary soil samples, and implement composition analysis based on passive spectroscopy and active spectroscopy like LIBS and Raman spectroscopy.

The studio is currently undertaking two major national engineering tasks, i. e. to develop 1) the time-frequency cabinet space femtosecond optical comb of China space station, and 2) the Chang’E-7 Raman spectrometer. The team has published 12 papers in world-class journals like Nature, Spectrochimica Acta Part B, Space Science Reviews, etc.

With open, innovative and integrated academic atmosphere, the studio has kept good cooperation with research teams from Chinese Academy of Sciences, domestic universities (including Hong Kong and Macao), and well-known overseas institutions, such as France Research Institute in Astrophysics and Planetology (IRAP). If you are interested in making contribution to the development of planetary science field in China, welcome to join us!

图 1 “祝融号”火星车搭载的火星物质成分探测仪（MarSCoDe）

图 2行星表面环境模拟平台（国际领先水平）

图 3风云三号气象卫星中分辨光谱成像仪全球云图

图 4 (a) 中国空间站时频柜空间飞秒光梳；(b) 全光锁定激光器重复频率