2 Jul 2022 - 17:25 EDT
2 Jul 2022 - 21:25 UTC

GOES-West Mesoscale Images for Daggett County, UT - 41°N - 110°W*

Images updated every 1 minute(s).

Day Land Cloud RGB

EUMETSAT Natural Color
23 Jun 2022 - 17:59 UTC

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Flash Extent Density over Band 13

Lightning flash extent density over IR Band 13
23 Jun 2022 - 17:58 UTC

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Day Cloud Phase RGB

RGB for evaluating phase of cooling cloud tops
23 Jun 2022 - 17:59 UTC

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Fire Temperature RGB

RGB used to highlight fires
23 Jun 2022 - 17:59 UTC

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Sandwich RGB

Blend combines IR band 13 with visual band 3
23 Jun 2022 - 17:59 UTC

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Dust RGB

RGB for identifying tropospheric dust
23 Jun 2022 - 17:59 UTC

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Band 1

0.47 µm
Blue - Visible
23 Jun 2022 - 17:59 UTC

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Band 2

0.64 µm
Red - Visible
23 Jun 2022 - 17:59 UTC

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Band 3

0.86 µm
Veggie - Near IR
23 Jun 2022 - 17:59 UTC

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Band 4

1.37 µm
Cirrus - Near IR
23 Jun 2022 - 17:59 UTC

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Band 5

1.6 µm
Snow/Ice - Near IR
23 Jun 2022 - 17:59 UTC

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Band 6

2.2 µm
Cloud Particle - Near IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 7

3.9 µm
Shortwave Window - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 8

6.2 µm
Upper-Level Water Vapor - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 9

6.9 µm
Mid-Level Water Vapor - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 10

7.3 µm
Lower-level Water Vapor - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 11

8.4 µm
Cloud Top - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 12

9.6 µm
Ozone - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 13

10.3 µm
Clean Longwave Window - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 14

11.2 µm
Longwave Window - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 15

12.3 µm
Dirty Longwave Window - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

Band 16

13.3 µm
CO₂ Longwave - IR
23 Jun 2022 - 17:59 UTC

Last update > 1 hour

*GOES-17 Infrared Image Quality

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.