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Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2140 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2141 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2142 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2143 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2144 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2145 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2146 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2147 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2148 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2149 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2150 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2151 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2152 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2153 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2154 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2155 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2156 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2157 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2158 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2159 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2200 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2201 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2202 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2203 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2204 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2205 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2206 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2207 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2208 UTC
Band 12 - 9.6 µm - Ozone - IR - 04 Dec 2021 - 2209 UTC
About Band 12
9.6 µm - "Ozone" Band - 2 km resolution - Band 12 will provide information both day and night about the dynamics of the atmosphere near the tropopause with high spatial and temporal resolutions. For clear (cloud-free) scenes of view, this band is cooler than the IR window bands because of absorption due to ozone.
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.
