Analysis of Magma Activity during the Cerro Azul Volcanic Unrest in March 2017 Using Sentinel-1 DInSAR Observations
Year: 2024
Type: article
Abstract: Cerro Azul volcano, one of the most active volcanoes in the Galápagos Archipelago, exhibited significant unrest in March 2017, marked by dramatic displacement around the caldera and on the southeastern plain.This study applied differential interferometric synthetic aperture radar (DInSAR) technique to SAR image pairs acquired from the Sentinel-1A satellite's ascending and descending nodes to measure the line-of-sight (LOS) and two-dimensional (up-down and east-west) displacements during the 2017 unrest of the volcano.Extensive concentric fringe patterns were observed around the caldera and on the southeastern plain of Cerro Azul volcano, indicating LOS displacements away from and toward the satellite, respectively.Two-dimensional displacements revealed that the volcanic body around the caldera contracted, while the southeastern plain uplifted and expanded.To further characterize magmatic activity during the unrest, we inverted LOS displacements from both ascending and descending observations using Mogi and Sill source models.The surface displacements simulated from the optimal magma source parameters obtained through inversion showed a normalized root mean square error of less than 5% compared to the DInSAR-observed displacements, confirming the reliability of the inversion results.The Mogi source was located approximately 4.7 km beneath the northeastern caldera rim of Cerro Azul and exhibited a volume change of -31 × 10 6 m 3 .The Sill source, characterized by a long rectangular shape approximately 10 km in length and 1 km in width, was situated about 7 km beneath the southeastern plain and showed a volume change of 68 × 10 6 m 3 .The volume increase of the Sill source was approximately twice that of the volume decrease of the Mogi source.Results of this study suggest that magma intrusion into the southeastern plain, originating from the Mogi source and deeper magma reservoirs, likely drove 피 변화 등의 마그마 특성을 추정할 수 있으며, 이는 화산 활동의 기
Source: 대한원격탐사학회지
Authors: Seohyeon Kim, Hyangsun Han, Jin-Woo Kim, Yeong-Beom Jeon, Seung Chul Lee
Institution: Kangwon National University
Language: English
Subfield: Aerospace Engineering
Field: Engineering
Domain: Physical Sciences
Open Access status: diamond
Awards: G3669908250, G6428614541
OpenAlex ID: W4406077759