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Fire Temperature - RGB used to highlight fires - 27 May 2022 - 2350 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0000 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0010 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0020 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0030 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0040 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0050 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0100 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0110 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0120 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0130 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0140 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.
