Planetary Waves Traveling Between Mars Science Laboratory and Mars 2020

被引:6
|
作者
Battalio, J. Michael [1 ]
Martinez, German [2 ]
Newman, Claire [3 ]
Juarez, Manuel de la Torre [4 ]
Sanchez-Lavega, Agustin [5 ]
Viudez-Moreiras, Daniel [6 ]
机构
[1] Yale Univ, Dept Earth & Planetary Sci, New Haven, CT 06520 USA
[2] USRA, Lunar & Planetary Inst, Houston, TX USA
[3] Aeolis Res, Pasadena, CA USA
[4] CALTECH, Jet Prop Lab, Pasadena, CA USA
[5] Univ Basque Country, UPV EHU, Dept Fis Aplicada 1, Bilbao, Spain
[6] Ctr Astrobiol INTA CSIC, Madrid, Spain
基金
美国国家航空航天局;
关键词
Mars; planetary waves; Mars Science Laboratory; 2020; reanalysis; MONITORING STATION OBSERVATIONS; GALE CRATER; MARTIAN ATMOSPHERE; DUST STORMS; EXTRACTING ENVELOPES; SOUTHERN-HEMISPHERE; TRANSIENT EDDIES; SURFACE PRESSURE; PART I; METEOROLOGY;
D O I
10.1029/2022GL100866
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Using Perseverance (Mars 2020) and Mars Science Laboratory (MSL) measurements, we obtain planetary waves with a period of 1.5-30 sols in the 1.5 m temperature, winds (Mars 2020), surface pressure, and relative humidity. Planetary waves emerge and propagate latitudinally across all variables. Short-period waves peak at periods of similar to 2, 3, and 4.5 sols, confirming previous detections of waves, and wave amplitudes agree at Mars 2020 and MSL for all variables. The simultaneous detection of waves within Gale and Jezero craters in multiple variables indicates that planetary-scale dynamics influences many facets of local weather throughout the year. Multiple waves are correlated or anti-correlated between MSL and Mars 2020, suggesting waves originate in both hemispheres. Further, waves at one site do not always lead the other, suggesting a combination of baroclinic and barotropic processes as wave sources, determined from the phasing of the temperature and winds in Jezero compared to the Ensemble Mars Atmospheric Reanalysis System.
引用
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页数:12
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