Data associated with ”Different behavior of density perturbations between dayside and nightside in the Martian thermosphere and the ionosphere associated with atmospheric gravity waves”

This provides the results of the 2-fluid model used to assess how well the neutral and ion observations from MAVEN-NGIMS can be matched to a theoretical atmospheric gravity wave. The data provide the location of each sample, and the measure of the goodness of fit to the model output.A full description of the 2-fluid model can be found in England, S. L., G. Liu, E. Yiğit, P. R. Mahaffy, M. Elrod, M. Benna, H. Nakagawa, N. Terada, and B. Jakosky (2017), MAVEN NGIMS observations of atmospheric gravity waves in the Martian thermosphere, J. Geophys. Res. Space Physics, 122, doi:10.1002/2016JA023475. A version of the code is available at https://github.com/NASA-Planetary-Science/wave-fit-toolkit.The MAVEN-NGIMS data are available from NASA PDS at https://pds-atmospheres.nmsu.edu/data_and_services/atmospheres_data/MAVEN/ngims.html

本数据集提供了使用双流体模型对MAVEN-NGIMS的中性和离子观测结果与理论大气重力波匹配程度进行评估的结果。数据集提供了每个样本的位置信息以及与模型输出的拟合优度测量。关于双流体模型的详细描述可参考England, S. L., G. Liu, E. Yiğit, P. R. Mahaffy, M. Elrod, M. Benna, H. Nakagawa, N. Terada, 和 B. Jakosky (2017) 发表的论文《火星热层大气重力波的MAVEN NGIMS观测》，发表于《地球物理研究空间物理》期刊，第122卷，DOI: 10.1002/2016JA023475。代码的版本可在https://github.com/NASA-Planetary-Science/wave-fit-toolkit上获取。MAVEN-NGIMS数据可通过NASA PDS在https://pds-atmospheres.nmsu.edu/data_and_services/atmospheres_data/MAVEN/ngims.html获取。