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Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0051 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0056 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0101 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0106 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0111 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0116 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0121 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0126 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0131 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0136 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0141 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2022 - 0146 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.
