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13 May 2025 - 08:54 EDT
13 May 2025 - 12:54 UTC

GOES-West CONUS - Fire Temperature

GOES-West - CONUS - FireTemperature - We are working to restore image production as quickly as possible. Please refer to the other GOES imagery sites listed on our resources page. Thank you for your patience.

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Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1011 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1011 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1016 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1016 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1021 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1021 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1026 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1026 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1031 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1031 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1036 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1036 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1041 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1041 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1046 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1046 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1051 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1051 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1056 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1056 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1101 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1101 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1106 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1106 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1111 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1111 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1116 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1116 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1121 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1121 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1126 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1126 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1131 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1131 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1136 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1136 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1141 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1141 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1146 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1146 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1151 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1151 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1156 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1156 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1201 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1201 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1206 UTC
Fire Temperature - RGB used to highlight fires - 13 May 2025 - 1206 UTC
legend for Fire Temperature RBG

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.

• For more details, see the Fire Temperature RGB Quick Guide, (PDF, 1.2 MB)