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Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1906 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1911 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1916 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1921 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1926 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1931 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1936 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1941 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1946 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1951 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 1956 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2001 UTC
About Fire Temperature
Fire Temperature RGB allows the user to identify where the most intense fires are occurring and differentiate these from "cooler" fires. The RGB takes advantage of the fact that from 3.9µm to shorter wavelengths, background solar radiation and surface reflectance increases. This means that fires need to be more intense in order to be detected by the 2.2 and 1.6µm bands, as more intense fires emit more radiation at these wavelengths. Therefore, small/"cool" fires will only show up at 3.9µm and appear red while increases in fire intensity cause greater contributions of the other channels resulting in white very intense fires.
