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Nighttime Microphysics - RGB to distinguish clouds from fog - 23 Jan 2022 - 2340 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 23 Jan 2022 - 2350 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0000 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0010 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0020 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0030 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0040 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0050 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0100 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0110 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0120 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0130 UTC
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.
