An Observational Overview of the Ubiquitous Dust Tides in the Martian Atmosphere
Description
The datasets contained herein were used to produce the figures and analysis presented in "An Observational Overview of the Ubiquitous Dust Tides in the Martian Atmosphere" by Zhaopeng Wu, Jing Li, Tao Li, Yueming Cheng, Jun Cui, Chengyun Yang, Zhaojin Rong, Fei He, Xuan Cheng, and Yong Wei
Files
Steps to reproduce
MY33: Mars year 33; T: MCS tempeature; dust: MCS dust opacity; zonalmean: zonally averaged data; fit: tidal extraction by applying the nonlinear least squares fitting; 20lswid: data averaged using 20 solar longitude window; 5lswid: data averaged using 5 solar longitude window; DW1 3D wind: the migrating diurnal tidal wind component u, v, w; dustinitial: the initialization of the dust particles at the start of simulation, saved file by IDL; dustmoving: Lagrangian particle simulations results; 2d lat prs: latitude_altitude plane; amplifier x.0: the tidal wind is increased by x.0 times during the simulations; nc: netcdf format file.