Surface warming during the 2018/MY 34 Mars Global Dust Storm

The Surface warming during the 2018/MY 34 Mars Global Dust Storm database is composed of reanalysis products combining past spacecraft observations
with a state-of-the-art Mars Global Circulation Model (MGCM), and free-running simulations of the MGCM. Spacecraft observations of column dust optical depth and temperature
profiles from the Mars Climate Sounder (MCS) instrument on the
Mars Global Surveyor spacecraft are combined with an MGCM used at the
Open University. The standard database includes 2-hourly output of key variables such as surface temperature, surface pressure, surface shortwave and longwave flux, temperature
as a function of altitude, and column dust optical depth.Further details on this dataset can be found in the Surface_warming_2018_GDS_dataset_reference.pdf document included in this repository.

2018年火星全球尘暴期间表面温度数据库由结合过往航天器观测数据与最先进的火星全球环流模型（MGCM）再分析产品，以及MGCM的自由运行模拟构成。火星全球探测器上的火星气候声学仪（MCS）对火星大气柱尘埃光学深度和温度剖面进行的航天器观测数据，与开放大学使用的MGCM相结合。标准数据库包括关键变量如地表温度、地表气压、地表短波和长波通量、随高度变化的温度以及大气柱尘埃光学深度的每小时两次输出。关于此数据集的更多详细信息，可在本存储库中包含的Surface_warming_2018_GDS_dataset_reference.pdf文档中找到。