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Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1330 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1331 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1332 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1333 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1334 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1335 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1336 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1337 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1338 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1339 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1340 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1341 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1342 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1343 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1344 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1345 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1346 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1347 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1348 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1349 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1350 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1351 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1352 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1353 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1354 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1355 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1356 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1357 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1358 UTC
Band 12 - 9.6 µm - Ozone - IR - 28 Jun 2022 - 1359 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.