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• W2023698819 endingPage "9485" @default.
• W2023698819 startingPage "9477" @default.
• W2023698819 abstract "The use of Landsat thermal infrared imagery gives a direct way of quantitatively monitoring the evolution of low‐amplitude thermal anomalies. Using nighttime Landsat thematic mapper images of Vulcano and Stromboli volcanoes on October 23, 1986, we have developed a simplified method for correcting atmospheric effects. We were then able to identify thermal anomalies around the craters. Part of the Stromboli lava flow, formed 1 year earlier, was also still warm enough to be detected. We obtained fairly accurate estimates of relative surface anomaly radiative heat fluxes: 29±5 W m −2 , 21±4 W m −2 , and 37±5 W m −2 for the Stromboli craters, Stromboli lava flow, and Vulcano crater, respectively. Accounting for the convective heat loss significantly increases the estimates of the relative internal heat flux of geothermal origin; we found values of 370±60 W m −2 for the Stromboli crater region, 220±50 W m −2 for the Stromboli lava flow, and 270±60 W m −2 for the Vulcano crater. Despite the low precision, these values are much higher than the 53–62 W m −2 limit (defined by Cassinis and Lechi, 1974) as the threshold where the geothermal flux can affect ground temperatures. Our study provides a unique systematic definition of thermal volcanic features found on Stromboli and Vulcano, the spatial extents of the anomalies, and their fluxes and associated errors." @default.
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• W2023698819 date "1994-05-10" @default.
• W2023698819 modified "2023-09-27" @default.
• W2023698819 title "Thermal infrared satellite measurements of volcanic activity at Stromboli and Vulcano" @default.
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• W2023698819 doi "https://doi.org/10.1029/93jb02392" @default.
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