Enhanced Super-rotation Before and During the 2018 Martian Global Dust Storm

This dataset contains information on the atmospheric fields of Mars, as generated by an assimilation of data from a Mars Global Circulation Model (MGCM) and observational data from two satellite instruments. The data has been used to study super-rotation in the martian atmosphere during the 2018 Global Dust Storm. The MGCM is the Mars atmospheric model used at the Open University, and the observational data are from: (a) the Mars Climate Sounder (MCS) instrument aboard the Mars Reconnaissance Orbiter (for Mars Years 33 and 34), and (b) the Atmospheric Chemistry Suite (ACS) aboard the ExoMars Trace Gas Orbiter (for Mars Year 34 only). Assimilation output data is provided over solar longitudes Ls = 150–240 for both years.Further information on the dataset can be found in the reference document: 'Super-rotation_during_the_2018_Martian_Global_Dust_Storm.pdf'

本数据集收录火星大气场相关信息，其数据由火星全球环流模型（Mars Global Circulation Model, MGCM）与两颗卫星仪器的观测数据同化生成。该数据集已被用于研究2018年火星全球沙尘暴期间火星大气的超旋转（super-rotation）现象。
本数据集所采用的火星全球环流模型为英国开放大学使用的火星大气模型，观测数据来源如下：(a) 搭载于火星勘测轨道飞行器（Mars Reconnaissance Orbiter）的火星气候探测仪（Mars Climate Sounder, MCS），对应火星第33、34个火星年；(b) 搭载于火星微量气体轨道探测器（ExoMars Trace Gas Orbiter）的大气化学套件（Atmospheric Chemistry Suite, ACS），仅对应火星第34个火星年。
两个火星年的同化输出数据均覆盖太阳经度Ls（solar longitudes Ls）=150~240区间。
有关本数据集的更多细节可参考文档：'Super-rotation_during_the_2018_Martian_Global_Dust_Storm.pdf'