Popocatépetl, Mexico’s most active volcano and one of the world’s strongest volcanic SO2 emitters, poses a major hazard to more than 20 million people. This study presents a comprehensive space-based investigation of its activity from 2019 to 2024, integrating thermal IR, UV gas absorption, radar, and VNIR satellite imagery. We analyzed Volcanic Radiative Power (VRP), SO2 flux, crater depth, and thermal anomalies to characterize recent eruptive behavior. TROPOMI data reveal three distinct degassing regimes, from $∼$1100,t/d in 2019 to $∼$3000,t/d after 2023, with a mean of $∼$1600,t/d, among the lowest since persistent activity began in 1994. VRP ranged between 0.01 and 1000,MW, declining until mid-2022 and rising before the May–June 2023 explosive phase. Popocatṕetl ceased producing its characteristic pancake-shaped lava domes after 2020, marking a transition from dome-building cycles to a new activity regime characterized by small-scale, short-lived extruded lava bodies, with almost no associated morphological change. Variations in the VRP/SO2 ratio suggest changes in conduit permeability associated with long-term crater deepening, with elevated ratios preceding the 2023 explosions, consistent with reduced gas escape and overpressure buildup. Following the 2023 paroxysm, high degassing decoupled from thermal emissions, indicating renewed magma input and sustained open-vent degassing. Due to limited extrusion, excess degassing and thermal output, calculated as volumetric fluxes responsible for degassing (Qdegas) and radiation (Qrad), point to shallow magma convection. These findings underscore the importance of multiparametric satellite observations to detect transitions in eruptive style, conduit permeability, and degassing dynamics at open-system volcanoes such as Popocat’étl.
Add the full text or supplementary notes for the publication here using Markdown formatting.