Notice:
This site has successfully transitioned the image data source from GOES-16 to
GOES-19. There are some remaining anomalies in the production of mesoscale
geocolor images which are being investigated. Everything else should be operating
as expected. Please contact:
NESDIS.STAR.webmaster@noaa.gov if you have any questions.
30 Apr 2025 - 08:10 EDT
30 Apr 2025 - 12:10 UTC
Post-tropical Cyclone Epsilon - Nighttime Microphysics at 48.6°N - 38.8°W
To enlarge, pause animation & click the image. Hover over popups to zoom. Use slider to navigate. Apparent 'jumps' in the animation occur due to adjustments to reflect storm movement.
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 used to distinguish clouds from fog - 26 Oct 2020 - 0530 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0540 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0550 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0600 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0610 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0630 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0640 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0650 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0700 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0710 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0720 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0800 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0810 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0830 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0900 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0920 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0930 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 0950 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 1000 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 1010 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 1040 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 1050 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 1100 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 26 Oct 2020 - 1110 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.