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Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0026 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0031 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0036 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0041 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0046 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0051 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0056 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0101 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0106 UTC
Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0111 UTC
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Nighttime Microphysics - RGB to distinguish clouds from fog - 24 Jan 2022 - 0121 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.
