While GOES animation code will not run on older Internet Explorer browsers,
they work in the newest versions of Microsoft Edge. If you are using
Internet Explorer, please try a different browser: Chrome, Firefox, Safari, or
MS Edge are all supported.
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2221 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2226 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2231 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2236 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2241 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2246 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2251 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2256 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2301 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2306 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2311 UTC
Fire Temperature - RGB used to highlight fires - 02 Oct 2022 - 2316 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.
