Data for "High-Latitude Zonal Jets in the Martian Upper Atmosphere Driven by Non-Orographic Gravity Waves"

Published: 26 February 2026| Version 1 | DOI: 10.17632/72k7t8rh75.1
Contributors:
Jiandong Liu,

Description

The NGIMS/MAVEN wind data used in this study are publicly available from the Planetary Data System (PDS) at https://atmos.nmsu.edu/PDS/data/PDS4/MAVEN/ngims_bundle/l3/. The associated built-in configuration files used in our analysis, including model setup parameters, are provided in this repository. The derived data generated in this study, including all model outputs used for figures and analysis, have been archived in a this repository . A README file is included to guide users on the location and usage of the configuration files, ensuring that the results can be fully reproduced without rerunning the simulations.

Files

Steps to reproduce

1. Unzip the .zip files 2. Use python script and the provided data to reproduce the following figures: Figure-1 in MY34: python Figure_lst_lat_ls.py Figure-2 in u_du_drag_epflux_stream1: python Figure01seismic_01.py Figure-3 in MY35: python winds_lon_latonoff_180clim_obsdiurnal_Spectual.py Figure-4 in MY34: python Figure04_lst_alt_winds.py Figure-5 in MY34: python Figure05appendix_v03_f03.py Figure-6 in u_du_drag_epflux_stream: python Figure06-02_A4_new.py

Categories

Thermosphere, Mars, Atmosphere Modeling, Atmospheric Circulation

Funders

Licence