{"title":"Mapping of flood inundated areas using earth observation data and cloud computing platform","authors":"Mohit Arora , Raj Setia , Randhir Singh , Sudhir Kumar Singh , Sumit Kumar , Brijendra Pateriya","doi":"10.1016/j.jastp.2025.106567","DOIUrl":null,"url":null,"abstract":"<div><div>Floods pose a significant threat, not only impacting human lives and property, but also causing extensive damage to critical infrastructure. Rapid flood impact assessment methods require comprehensive, updated and accurate flood maps to deliver the dependable information for effective disaster risk management. In this study, the flood-inundated areas were mapped and monitored in Punjab (India) using dual-polarized (VH and VV) Sentinel-1 (A and B) images of July–August 2023 and the impact of flood on cropped area was assessed using Geographic Information System (GIS). The satellite images were processed in Google Earth Engine (GEE) platform to extract the spatial extent of flood-inundated areas. The flooded areas were validated with limited ground truth. The district wise zonal statistics was derived to find the flood inundated areas. Results showed that the backscattering coefficient (σ0) of the flooded area ranged from −4 to −20 dB for VH polarization and from −4 to −30 dB for VV polarization. These threshold limits were used to extract the flood pixels followed by masking of permanent water bodies. The water extent reached its peak from 11 to July 17, 2023 (first flood period) and again from 14 to August 17, 2023 (Second flood period) in Punjab with 5.52 % of the area inundated during first flood period and 2.65 % of the cropped area inundated during the second flood period. The overall accuracy was 91.7 % with Kappa Coefficient of 0.83 in VV polarization and 86.2 % with Kappa Coefficient of 0.73 in VH polarization. Paddy was mostly inundated by flooding in the areas with lower elevation, high runoff and along the river breeches. These results suggest that spatio-temporal mapping of flood inundation is important for policy makers towards flood risk preparedness, raising awareness, designing the mitigation strategies and implementation of flood management planning to protect nature and human life.</div></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"274 ","pages":"Article 106567"},"PeriodicalIF":1.8000,"publicationDate":"2025-06-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682625001518","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
Floods pose a significant threat, not only impacting human lives and property, but also causing extensive damage to critical infrastructure. Rapid flood impact assessment methods require comprehensive, updated and accurate flood maps to deliver the dependable information for effective disaster risk management. In this study, the flood-inundated areas were mapped and monitored in Punjab (India) using dual-polarized (VH and VV) Sentinel-1 (A and B) images of July–August 2023 and the impact of flood on cropped area was assessed using Geographic Information System (GIS). The satellite images were processed in Google Earth Engine (GEE) platform to extract the spatial extent of flood-inundated areas. The flooded areas were validated with limited ground truth. The district wise zonal statistics was derived to find the flood inundated areas. Results showed that the backscattering coefficient (σ0) of the flooded area ranged from −4 to −20 dB for VH polarization and from −4 to −30 dB for VV polarization. These threshold limits were used to extract the flood pixels followed by masking of permanent water bodies. The water extent reached its peak from 11 to July 17, 2023 (first flood period) and again from 14 to August 17, 2023 (Second flood period) in Punjab with 5.52 % of the area inundated during first flood period and 2.65 % of the cropped area inundated during the second flood period. The overall accuracy was 91.7 % with Kappa Coefficient of 0.83 in VV polarization and 86.2 % with Kappa Coefficient of 0.73 in VH polarization. Paddy was mostly inundated by flooding in the areas with lower elevation, high runoff and along the river breeches. These results suggest that spatio-temporal mapping of flood inundation is important for policy makers towards flood risk preparedness, raising awareness, designing the mitigation strategies and implementation of flood management planning to protect nature and human life.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.