Mars PCM temperature results from MY 36 LS = 0° to MY 37 LS = 60°

We present here the numerical simulation results of the temperature in the Martian atmosphere from Martian Year (MY) 36 solar longitude (LS) 0° to MY 37 LS 60°. The data is based on the Mars PCM (version 6). A description of the model setting is presented in Fan et al. (2022), and a general description of the model architecture is given in Forget et al. (1999). The model has a 64×48×73 grid in longitude, latitude, and pressure levels, which corresponds to a horizontal resolution of 5.625° and 3.75° in longitude and latitude, respectively, and 73 hybrid terrain-following vertical pressure levels (σ-grid) from surface to ~2×10^-3 Pa. The run has 960 dynamical timesteps in each Martian day, and the physical timestep is 7.5 Martian minutes.The dust injection is semi-interactive regulated by the MY 36 and MY 37 dust scenarios.The data is seven NetCDF files, each including two Martian months. They are self-explanatory with the meanings of variables included in their headers, which contain atmosphere temperature, surface temperature, and surface pressure in the simulation, together with information about the four-dimensional grid in longitude, latitude, pressure level, and time, and also the corresponding LS at each timestep.Reference: (1) Forget et al. (1999) Improved general circulation models of the Martian atmosphere from the surface to above 80 km. Journal of Geophysical Research, 104(E10), 24155-24176. (2) Fan et al. (2022) Migrating Thermal Tides in the Martian Atmosphere during Aphelion Season Observed by EMM/EMIRS. Journal of Geophysical Research: Planets.