4.5 Article

Mars Surface Pressure Oscillations as Precursors of Large Dust Storms Reaching Gale

期刊

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1029/2021JE007005

关键词

Mars; dust storm precursors; surface pressure; planetary waves; emprical mode decomposition; singular spectrum analysis

资金

  1. Spanish Ministry of Science, Innovation and Universities [RTI2018-098728-B-C31]
  2. Instituto Nacional de Tecnica Aeroespacial
  3. NASA's Mars Science Laboratory project

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Modeling and observations have shown that dust storms on Mars significantly affect global circulation patterns and alter pressure variations. The analysis of pressure data collected by the Curiosity Rover reveals changes in pressure oscillations and phasing that serve as precursors to large-scale dust storms.
Modeling and observations have long demonstrated that Martian dust storms strongly interfere with global circulation patterns and change the diurnal and semidiurnal pressure variability as well as oscillations with periods greater than one sol associated with planetary waves. As of early 2022, five Mars years of pressure data have been collected by the Curiosity Rover in Gale crater with the Rover Environmental Monitoring Station (REMS). A combination of signal filtering techniques is used to search for pressure signatures that might warn large-scale dust storms reaching Gale. The analysis combines an exploration of changes in both baroclinic waves and thermal tides for the first time to our knowledge. Focusing on the periods preceding local opacity increases as detected by Curiosity's Mastcam observations, the pressure analysis shows changes in the coupling between the diurnal pressure tide and quasi-diurnal Kelvin wave, as well as in the temporal evolution of baroclinic waves that are harbingers of the larger dust storms. Changes in the phasing between Kelvin waves and diurnal tides are found to be precursors for the growth phase of periods Z (defined here as L-s similar to 120 degrees-160 degrees), A (L-s similar to 190 degrees-240 degrees), and C (L-s similar to 300 degrees-335 degrees) dust storms. Changes in multi-sol pressure oscillations also help predict the occurrence of A, B (L-s similar to 245 degrees-295 degrees), and C storms. The specific pressure oscillations preceding each storm period are likely to be signatures of the large-scale circulation patterns that enable the growth and propagation of the storm fronts.

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