Notice:
Starting December 3, 2024, visitors to GOES.NOAA.GOV will be redirected
to the STAR
GOES Imagery site. If you have any questions about this change
or need assistance, please contact OSPO
User Services.
7 Dec 2024 - 16:35 EST
7 Dec 2024 - 21:35 UTC
GOES-West Full Disk - Fire Temperature
2 hour loop - 12 images - 10 minute update
To enlarge, pause animation & click the image. Hover over popups to zoom. Use slider to navigate.
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 - 07 Dec 2024 - 1930 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 1940 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 1950 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2000 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2010 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2020 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2030 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2040 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2050 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2100 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2110 UTC
Fire Temperature - RGB used to highlight fires - 07 Dec 2024 - 2120 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.