NOAA GOES Image Viewer website
13 Jun 2021 - 16:58 EDT
13 Jun 2021 - 20:58 UTC

GOES-West - Latest Full Disk Images*

Images updated every 10 minutes. GLM images updated every minute.

GeoColor

True Color daytime, multispectral IR at night
13 Jun 2021 - 20:30 UTC

GLM FED+GeoColor

Geostationary Lightning Mapper
13 Jun 2021 - 20:40 UTC

AirMass RGB

RGB composite based on the data from IR and WV
13 Jun 2021 - 20:30 UTC

Sandwich RGB

Multi-spectral blend combines IR band 13 with visual band 3
13 Jun 2021 - 20:30 UTC

Derived Motion Winds

Derived Motion Winds
13 Jun 2021 - 20:00 UTC

Day Cloud Phase RGB

RGB used to evaluate the phase of cooling cloud tops
13 Jun 2021 - 20:30 UTC

Nighttime Microphysics

RGB used to distinguish clouds from fog
13 Jun 2021 - 20:30 UTC

Band 1

0.47 µm
Blue - Visible
13 Jun 2021 - 20:40 UTC

Band 2

0.64 µm
Red - Visible
13 Jun 2021 - 20:30 UTC

Band 3

0.86 µm
Veggie - Near IR
13 Jun 2021 - 20:40 UTC

Band 4

1.37 µm
Cirrus - Near IR
13 Jun 2021 - 20:40 UTC

Band 5

1.6 µm
Snow/Ice - Near IR
13 Jun 2021 - 20:40 UTC

Band 6

2.2 µm
Cloud Particle - Near IR
13 Jun 2021 - 20:40 UTC

Band 7

3.9 µm
Shortwave Window - IR
13 Jun 2021 - 20:40 UTC

Band 8

6.2 µm
Upper-Level Water Vapor - IR
13 Jun 2021 - 20:40 UTC

Band 9

6.9 µm
Mid-Level Water Vapor - IR
13 Jun 2021 - 20:40 UTC

Band 10

7.3 µm
Lower-level Water Vapor - IR
13 Jun 2021 - 20:40 UTC

Band 11

8.4 µm
Cloud Top - IR
13 Jun 2021 - 20:40 UTC

Band 12

9.6 µm
Ozone - IR
13 Jun 2021 - 20:40 UTC

Band 13

10.3 µm
Clean Longwave Window - IR
13 Jun 2021 - 20:40 UTC

Band 14

11.2 µm
Longwave Window - IR
13 Jun 2021 - 20:40 UTC

Band 15

12.3 µm
Dirty Longwave Window - IR
13 Jun 2021 - 20:40 UTC

Band 16

13.3 µm
CO₂ Longwave - IR
13 Jun 2021 - 20:40 UTC


*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.