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Ring Structures in GOES-17 infrared imagery over the Hawai’ian peaks

An animation of GOES-17 Band 13 10.3 µm infrared imagery, above, shows the development of concentric circles of cold, warm, cold and warm surrounding the high peaks of the island of Hawai’i (Click here to see a topographic view). The warmth apparent around the peaks at the start of the... Read More

GOES-17 Clean Window Infrared (10.3 µm) imagery, 0301 – 1601 UTC 27 May 2022 (click to enlarge)

An animation of GOES-17 Band 13 10.3 µm infrared imagery, above, shows the development of concentric circles of cold, warm, cold and warm surrounding the high peaks of the island of Hawai’i (Click here to see a topographic view). The warmth apparent around the peaks at the start of the animation above (dark in the enhancement chosen) suggests that the peaks are peeking through a stratus deck; the toggle below between sunset and sunrise imagery (the sunrise imagery has been brightened considerably) shows that clouds dissipated overnight.

GOES-17 Band 2 (0.64 µm) visible imagery at 0401 UTC and 1601 UTC on 27 May 2022 (Click to enlarge)

The animation below shows brightness temperatures sampled through the rings at 1121 UTC surrounding Mauna Kea. Mountain-top temperatures are sub-freezing, warming to around 5oC/41oF just off the peak, before cooling again to 2oC/36oF and then warming to 5+oC/41+oF farther down the slope. This interesting behavior results from a combination of cooling in the presence of an inversion, and cooling interrupted by the presence of cloudiness. The 1200 UTC sounding from Hilo, on the eastern part of the north coast of Hawai’i, is shown here (courtesy K. Kodama, WFO HNL).

GOES-17 Infrared Band 13 imagery (10.3 µm) at 1121 UTC on 27 May 2022, with brightness temperatures sampled at select points (Click to enlarge)

The toggle below compares GOES-17 Bands 13, 10 and 8 (10.3 µm, 7.3 µm and 6.19 µm, respectively) at 1121 UTC. The ringing is obvious in Band 13; it is not obvious in Bands 10 and 8: in those two bands any surface cooling differences are masked by water vapor emissions higher in the atmosphere, even at the high altitudes along the slopes of Mauna Kea and Mauna Loa.

GOES-17 Bands 13, 10 and 8 (Clean Window, Low-Level Water Vapor and Upper-Level Water Vapor, i.e., 10.3 µm, 7.3 µm and 6.19 µm, respectively) at 1121 UTC on 27 May 2022 (click to enlarge)

Weighting Functions for the three water vapor bands (taken from this website) underscore why ringing around the peaks is far less likely to be observed in the water vapor channels on this day. The sounding shown below (or here) shows a moist layer above 500 mb, between 6 and 8 km above ground; Mauna Loa and Mauna Kea peak at about 4.2 km. The surface-based infrared signal at wavelengths between 6.2 and 7.3 µm will be obscured by water vapor emissions from higher up in the atmosphere. If that high-altitude moist layer were missing, the cold-warm-cold-warm signal would have a better chance of appearing in the water vapor imagery.


Because skies are clearing, one might expect these ring features to appear in the Land Surface Temperature field. However, a toggle that field at 1201 UTC, along with the Clear Sky Mask, shows that is not the case. Land Surface Temperature is computed in regions where skies are “Clear” or “Probably Clear”, but not where skies are “Cloudy” or “Probably Cloudy” (the four possible states in the Clear Sky Mask; note however that AWIPS displays on “Cloudy” skies as white, and all other states are transparent). Thus, the ‘warm’ parts of the rings are displayed; the cold parts are not.

GOES-16 Land Surface Temperature display with/over, Band 13 infrared (10.3 µm) imagery, Topography, and Clear Sky Mask at 1201 UTC on 27 May 2022 (click to enlarge)

Thanks very much to Kevin Kodama, WFO HNL, and Jordan Gerth, NWS/OBS, for bringing this interesting case to our attention!

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High-altitude turbulence over the Southern Plains

GOES-16 (GOES-East) Upper-level Water Vapor (6.2 µm) images with pilot reports of turbulence — with and without contours of RAP40 model Maximum Wind Speed (above) showed an anomalously-deep 500 hPa trough over the Southern Plains, where there was an anomalously-strong 250 hPa jet streak developing along its forward (eastern) edge. A number of pilot reports of moderate to... Read More

GOES-16 Upper-level Water Vapor (6.2 µm) images, with pilot reports of turbulence (cyan) — with and without contours of RAP40 model Maximum Wind Speed (yellow) [click to play animated GIF | MP4]

GOES-16 (GOES-East) Upper-level Water Vapor (6.2 µm) images with pilot reports of turbulence — with and without contours of RAP40 model Maximum Wind Speed (above) showed an anomalously-deep 500 hPa trough over the Southern Plains, where there was an anomalously-strong 250 hPa jet streak developing along its forward (eastern) edge. A number of pilot reports of moderate to severe turbulence were seen within the exit region of this jet streak.

In GOES-16 Upper-level Water Vapor images with and without an overlay of a Turbulence Probability product (below), higher probability values were apparent in the area near/along the axis of the 250 hPa jet streak (and the related pilot reports of turbulence).

GOES-16 Upper-level Water Vapor (6.2 µm) images, with pilot reports of turbulence (cyan) — with and without an overlay of Turbulence Probability [click to play animated GIF | MP4]

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View and animate GOES-16 and GOES-17 Full-Disk IFR/Low IFR Probability fields in RealEarth

GOES-16 and GOES-17 Full-Disk IFR and Low IFR Probability fields are now available in RealEarth. IFR (Instrument Flight Rules) Probability estimates the likelihood that IFR conditions are occurring. You can view and animate real-time satellite IFR probability in RealEarth. ... Read More

GOES-16 and GOES-17 Full-Disk IFR and Low IFR Probability fields are now available in RealEarth. IFR (Instrument Flight Rules) Probability estimates the likelihood that IFR conditions are occurring. You can view and animate real-time satellite IFR probability in RealEarth.

Finding IFR and Low IFR fields in RealEarth for GOES-16 and GOES-17 full disk.
Comparing GOES-17 IFR and Low IFR for 05-25-2022 at 15:10UTC, and animating GOES-17 IFR fields in RealEarth over Hawai’i for the last 12 available GOES-17 time steps (10-minute resolution from 13:10 to 15:20UTC).

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Severe thunderstorms in Texas

1-minute Mesoscale Domain Sector GOES-16 (GOES-East) “Red” Visible (0.64 µm) images (above) include time-matched SPC Storm Reports — and showed the development severe thunderstorms across parts of Texas (and far southeastern New Mexico) during the afternoon and early evening hours on 24 May 2022. These storms produced hail as large as 4.00 inches in diameter, a tornado and damaging winds as... Read More

GOES-16 “Red” Visible (0.64 µm) images, with time-matched SPC Storm Reports plotted in red [click to play animated GIF | MP4]

1-minute Mesoscale Domain Sector GOES-16 (GOES-East) “Red” Visible (0.64 µm) images (above) include time-matched SPC Storm Reports — and showed the development severe thunderstorms across parts of Texas (and far southeastern New Mexico) during the afternoon and early evening hours on 24 May 2022. These storms produced hail as large as 4.00 inches in diameter, a tornado and damaging winds as strong as 78 mph. Signatures of Above-Anvil Cirrus Plumes (reference | VISIT training) were also evident .

In the corresponding 1-minute GOES-16 “Clean” Infrared Window (10.35 µm) images (below), pulsing overshooting tops exhibited infrared brightness temperatures in the -70 to -79ºC range.

GOES-16 “Clean” Infrared Window (10.35 µm) images, with time-matched SPC Storm Reports plotted in blue [click to play animated GIF | MP4]

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