Physical Detection Limits of Dense GNSS Arrays for Monitoring Prerupture Transient Deformation

ABSTRACT Detectability of prerupture crustal deformation depends on sensor precision, node density, array aperture, spatial covariance, deformation footprint, and causal filtering. We derive a covariance-propagation framework for targeted dense arrays of low-cost dual-band Global Navigation Satellite System sensors. Regional offset and planar fields are fitted as nuisance modes, while independent receiver noise and residual locally correlated noise enter an explicit covariance matrix. For a prescribed spatial template, minimum-variance weighting estimates the same localized amplitude used in the performance figures. The exponential covariance is retained only as a transparent benchmark; other positive-definite kernels can be inserted through their covariance matrix or integrated correlation area. Because the proposed hardware has not been field-calibrated, we use favorable, reference, and conservative design scenarios rather than a universal noise value. For a 20 × 20 km domain and a radial Rc=3 km footprint, the reference scenario gives spatial-search-adjusted thresholds of approximately 2.03, 1.63, 1.41, and 1.19 cm for N = 900, 1,600, 2,500, and 4,900 nodes, respectively; in the conservative scenario, persistent local correlation creates a floor of several centimeters even at larger N. Independently processed records from Global Navigation Satellite System stations PSGA and IQQE during the 2014 Iquique sequence provide filtered amplitudes of 1.54 and 1.02 cm without rescaling. In a counterfactual N = 4096 benchmark, PSGA crosses the favorable and reference thresholds, whereas IQQE crosses only the favorable threshold; this is not a retrospective dense-array detection. Direct matrix inversion, a finite-grid matrix-free solution, and 5000 Monte Carlo realizations agree at the sub-percent level. The framework identifies the density, covariance, footprint, and cost conditions for mechanically grounded prerupture monitoring, together with the field-calibration and false-alarm tests required before operational use.

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Publication Details

Journal
Bulletin of the Seismological Society of America
Published
2026-09-21
DOI
https://doi.org/10.1785/0120260121
Primary Topic
GNSS positioning and interference
Type
article
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Physical Detection Limits of Dense GNSS Arrays for Monitoring Prerupture Transient Deformation

Yi Yang
Bulletin of the Seismological Society of America
GNSS positioning and interference
article

Physical Detection Limits of Dense GNSS Arrays for Monitoring Prerupture Transient Deformation

Yi Yang
article en

Abstract

ABSTRACT Detectability of prerupture crustal deformation depends on sensor precision, node density, array aperture, spatial covariance, deformation footprint, and causal filtering. We derive a covariance-propagation framework for targeted dense arrays of low-cost dual-band Global Navigation Satellite System sensors. Regional offset and planar fields are fitted as nuisance modes, while independent receiver noise and residual locally correlated noise enter an explicit covariance matrix. For a prescribed spatial template, minimum-variance weighting estimates the same localized amplitude used in the performance figures. The exponential covariance is retained only as a transparent benchmark; other positive-definite kernels can be inserted through their covariance matrix or integrated correlation area. Because the proposed hardware has not been field-calibrated, we use favorable, reference, and conservative design scenarios rather than a universal noise value. For a 20 × 20 km domain and a radial Rc=3 km footprint, the reference scenario gives spatial-search-adjusted thresholds of approximately 2.03, 1.63, 1.41, and 1.19 cm for N = 900, 1,600, 2,500, and 4,900 nodes, respectively; in the conservative scenario, persistent local correlation creates a floor of several centimeters even at larger N. Independently processed records from Global Navigation Satellite System stations PSGA and IQQE during the 2014 Iquique sequence provide filtered amplitudes of 1.54 and 1.02 cm without rescaling. In a counterfactual N = 4096 benchmark, PSGA crosses the favorable and reference thresholds, whereas IQQE crosses only the favorable threshold; this is not a retrospective dense-array detection. Direct matrix inversion, a finite-grid matrix-free solution, and 5000 Monte Carlo realizations agree at the sub-percent level. The framework identifies the density, covariance, footprint, and cost conditions for mechanically grounded prerupture monitoring, together with the field-calibration and false-alarm tests required before operational use.

Bulletin of the Seismological Society of America
Institute of Physics, Academia Sinica (TW), National Cheng Kung University (TW)
Openalex Percentile: Top 7%
GNSS positioning and interference
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