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.
7 Feb 2023 - 09:52 EST
7 Feb 2023 - 14:52 UTC
GOES-East Full Disk - Nighttime Microphysics
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.
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1230 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1240 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1250 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1300 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1310 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1320 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1330 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1340 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1350 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1400 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1410 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 07 Feb 2023 - 1420 UTC
This RGB will be phased out around 1 Feb 2023 and will be replaced by the Day Night Cloud Micro Combo RGB.
Nighttime Microphysics RGB The distinction between low clouds and fog in satellite imagery is challenging. While the difference between the 10.4 and 3.9 μm channels has been a regularly applied product to meet aviation forecast needs, the Nighttime Microphysics (NtMicro) RGB adds another channel difference (12.4- 10.4 μm) as a proxy to cloud thickness and repeats the use of the 10.4 μm thermal channel to enhance areas of warm (i.e. low) clouds where fog is more likely. The NtMicro RGB is also an efficient tool to quickly identify other cloud types in the mid and upper atmosphere.
