GOES-18 Interleave Testing - Has ended. GOES-West data now supplied from operational GOES-17 satellite.
GOES-18 expected to become operational GOES-West in January 2023. See GOES-18 Interleave Testing for more information.
28 May 2023 - 03:20 EDT
28 May 2023 - 07:20 UTC
GOES-East CONUS - Fire Temperature
1 hour loop - 12 images - 5 minute update
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Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0611 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0616 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0621 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0626 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0631 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0636 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0641 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0646 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0651 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0656 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0701 UTC
Fire Temperature - RGB used to highlight fires - 28 May 2023 - 0706 UTC
Fire Temperature key:
1 - Warm fire 2 - Very warm fire 3 - Hot fire 4 - Very hot fire 5 - Burn scars 6 - Clear sky: land 7 - Clear sky: water/snow/night 8 - Water clouds 9 - Ice clouds
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.
