Thermal tides are atmospheric planetary-scale waves with periods that are harmonics of the solar day. In the Martian atmosphere thermal tides are known to be especially significant compared to any other known planet. Based on the data set of pressure timeseries produced by the InSight lander, which is unprecedented in terms of accuracy and temporal coverage, we investigate thermal tides on Mars and we find harmonics even beyond the number 24, which exceeds significantly the number of harmonics previously reported by other works. We explore comparatively the characteristics and seasonal evolution of tidal harmonics and find that even and odd harmonics exhibit some clearly differentiated trends that evolve seasonally and respond to dust events. High-order tidal harmonics with small amplitudes could transiently interfere constructively to produce meteorologically relevant patterns.
Impact of gravity waves on the middle atmosphere of Mars: a non-orographic gravity wave parameterization based on Global Climate modeling and MCS observations
Diurnal temperature variations and migrating thermal tides in the Martian lower atmosphere observed by the Emirates Mars InfraRed Spectrometer
Southern University of Science and Technology（南方科技大学）；LMD/IPSL, Sorbonne Université, PSL Research Université, École Normale Supérieure, École Polytechnique, CNRS（巴黎文理研究大学）；NASA Goddard Space Flight Center（美国国家航空航天局戈达德太空飞行中心）；NASA Ames Research Center（美国国家航空航天局艾姆斯研究中心）；Mohammed Bin Rashid Space Centre（穆罕默德·本·拉希德航天中心）；University of Maryland Baltimore County（马里兰大学巴尔的摩县分校）；University of Aberdeen（阿伯丁大学）；United Arab Emirates University（阿联酋大学）；Northern Arizona University（北亚利桑那大学）；Arizona State University（亚利桑那州立大学）；University of Colorado Boulder（科罗拉多大学博尔德分校）
Evolution of a synchronous planet-moon pair due to solar tides. Demise of the synchronous moon that initiated Mars' triaxiality. A possible link to tidalites in Vastitas Borealis and Gale Crater
Using physics-based simulation towards eliminating empiricism in extraterrestrial terramechanics applications
School of Naval Architecture, Ocean and Civil Engineering, Shanghai Jiao Tong University（上海交通大学船舶海洋与建筑工程学院）；University of Wisconsin-Madison（威斯康星大学麦迪逊分校）；Ames Research Center, NASA（美国国家航空航天局艾姆斯研究中心）；NASA, Glenn Research Center（美国国家航空航天局格伦研究中心）；ProtoInnovations, LLC（ProtoInnovations有限责任公司）；Massachusetts Institute of Technology（麻省理工学院）
Results from NASA's First Radio Telescope on the Moon: Terrestrial Technosignatures and the Low-Frequency Galactic Background Observed by ROLSES-1 Onboard the Odysseus Lander
