4.5 Article

A Comodulation Analysis of Atmospheric Energy Injection Into the Ground Motion at InSight, Mars

期刊

出版社

AMER GEOPHYSICAL UNION
DOI: 10.1029/2020JE006538

关键词

atmosphere‐ induced noise; comodulation; ground motion; marsquakes; method of moments; noise discrimination

资金

  1. UK Space Agency [ST/N001044/1, ST/R002096/1, ST/W002523/1] Funding Source: researchfish

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A novel method is presented to partition observed signals into seismic and environmental contributions, with atmospheric pressure and wind fluctuations shown to exhibit temporal cross-frequency coupling across multiple bands. By working in the time-frequency domain, the relationship between comodulated signals is exploited to identify their sources, allowing for an understanding of the site's environmental sensitivity and quantification of wind and pressure injection.
Seismic observations involve signals that can be easily masked by noise injection. For the NASA Mars lander InSight, the atmosphere is a significant noise contributor, impeding the identification of seismic events for two-thirds of a Martian day. While the noise is below that seen at even the quietest sites on Earth, the amplitude of seismic signals on Mars is also considerably lower, requiring an understanding and quantification of environmental injection at unprecedented levels. Mars' ground and atmosphere are a continuously coupled seismic system, and although atmospheric functions are of distinct origins, the superposition of these noise contributions is poorly understood, making separation a challenging task. We present a novel method for partitioning the observed signal into seismic and environmental contributions. Atmospheric pressure and wind fluctuations are shown to exhibit temporal cross-frequency coupling across multiple bands, injecting noise that is neither random nor coherent. We investigate this through comodulation, quantifying the synchrony of the seismic motion, wind and pressure signals. By working in the time-frequency domain, we discriminate between the different origins of underlying processes and determine the site's environmental sensitivity. Our method aims to create a virtual vault at InSight's landing site on Mars, shielding the seismometers with effective postprocessing in lieu of a physical vault. This allows us to describe the environmental and seismic signals over a sequence of sols, to quantify the wind and pressure injection and estimate the seismic content of possible marsquakes with a signal-to-noise ratio that can be quantified in terms of environmental independence. Finally, we exploit the relationship between the comodulated signals to identify their sources.

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