NOAA GOES Image Viewer website
17 Apr 2021 - 04:52 EDT
17 Apr 2021 - 08:52 UTC

GOES-West - Sector view: Northern Pacific - Nighttime Microphysics*

6 hour loop - 24 images - 15 minute update

To enlarge, pause animation & click the image. Hover over popups to zoom. Use slider to navigate.

  

  
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0350 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0350 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0400 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0400 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0410 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0410 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0420 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0420 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0430 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0430 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0440 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0440 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0450 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0450 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0500 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0500 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0510 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0510 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0520 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0520 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0530 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0530 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0540 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0540 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0550 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0550 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0600 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0600 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0615 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0615 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0630 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0630 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0645 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0645 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0700 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0700 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0715 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0715 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0730 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0730 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0745 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0745 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0800 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0800 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0815 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0815 UTC Latitude / Longitude grid
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0830 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 17 Apr 2021 - 0830 UTC Latitude / Longitude grid
 

About Nighttime Microphysics

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.

• For more details, see the Nighttime Microphysics RGB Quick Guide, (PDF, 1.41 MB)

*GOES-17 Infrared Image Quality

During post-launch testing of the GOES-17 ABI instrument, an issue with the instrument's cooling system was discovered. The loop heat pipe (LHP) subsystem, which transfers heat from the ABI electronics to the radiator, is not operating at its designed capacity. The consequence of this is that the ABI detectors cannot be maintained at their intended temperatures under certain orbital conditions. This is preventing adequate cooling for some of the infrared (IR) channels on the instrument during parts of the night, leading to partial loss of ABI imagery. Learn more.

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