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.
10 Jun 2023 - 21:52 EDT
11 Jun 2023 - 01:52 UTC
GOES-West CONUS - Fire Temperature
1 hour loop - 12 images - 5 minute update
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Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0031 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0036 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0041 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0046 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0051 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0056 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0101 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0106 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0111 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0121 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0131 UTC
Fire Temperature - RGB used to highlight fires - 11 Jun 2023 - 0136 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.
