Abnormal Phase Structure of Thermal Tides During Major Dust Storms on Mars: Implications for the Excitation Source of High‐altitude Water Ice Clouds-Reference-Cited by-同舟云学术

Abnormal Phase Structure of Thermal Tides During Major Dust Storms on Mars: Implications for the Excitation Source of High‐altitude Water Ice Clouds

Published:2021-04 Issue:4 Volume:126 Page:
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J Geophys Res Planets

Author:

Wu Zhaopeng¹²^ORCID,Li Tao³²^ORCID,Li Jing¹³,Zhang Xi⁴^ORCID,Yang Chengyun³²^ORCID,Cui Jun¹²⁵^ORCID

Affiliation:

1. Planetary Environmental and Astrobiological Research Laboratory School of Atmospheric Sciences Sun Yat‐sen University Zhuhai Guangdong People's Republic of China

2. CAS Center for Excellence in Comparative Planetology Hefei Anhui People's Republic of China

3. CAS Key Laboratory of Geospace Environment School of Earth and Space Sciences University of Science and Technology of China Hefei Anhui People's Republic of China

4. Department of Earth and Planetary Sciences University of California Santa Cruz Santa Cruz CA USA

5. CAS Key Laboratory of Lunar and Deep Space Exploration National Astronomical Observatories Chinese Academy of Sciences Beijing People's Republic of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2020JE006758

Reference57 articles.

1. Water Vapor Vertical Profiles on Mars in Dust Storms Observed by TGO/NOMAD

2. Atmospheric tides in Earth-like planets

3. Thermal tides and stationary waves on Mars as revealed by Mars Global Surveyor thermal emission spectrometer

4. Forced waves in the martian atmosphere from MGS TES nadir data

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