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Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0030 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0040 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0050 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0100 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0110 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0120 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0130 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0140 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0150 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0200 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0210 UTC
Nighttime Microphysics - RGB used to distinguish clouds from fog - 23 Jan 2021 - 0220 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.