- University of Padua, Department of Geosciences, Padova, Italy (filippo.catani@unipd.it)
InSAR time series are widely used to characterize long-term surface deformation, yet coseismic steps can distort displacement histories and bias velocity estimates if they are not explicitly identified and separated. We present a catalog-independent framework to detect and remove multiple coseismic steps from large InSAR time series datasets by exploiting a characteristic earthquake signature: many pixels exhibit near-synchronous displacement steps, while step amplitudes vary spatially. After reducing slowly varying components (e.g., linear trend and seasonal terms), we identify a sparse set of shared changepoint times across displacement histories using a multi-signal shared-changepoint model, enabling recovery of multi-event sequences within a single observation period. For each detected changepoint, we estimate pixel-wise step amplitudes using robust windowed statistics and/or step regression, and then regularize each event’s step-amplitude field on a spatial neighborhood graph using total-variation regularization to enforce spatial consistency, suppress outliers, and preserve sharp gradients expected near faults. Subtracting the regularized steps from the original time series yields de-evented displacement histories and updated long-term deformation rates. The approach is scalable, supports repeated and closely spaced events via joint estimation of multiple steps, and does not require prior event timing information. Applied to multi-year regional InSAR products, the method produces cleaner time series, reduced residual variance, and more stable velocity estimates, improving characterization of gradual deformation in tectonic and volcanic settings.
How to cite: Chen, X., Floris, M., Rosi, A., and Catani, F.: Catalog-independent detection and removal of coseismic steps in InSAR time series using shared changepoints and spatial regularization, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-19196, https://doi.org/10.5194/egusphere-egu26-19196, 2026.