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A Foggy Morning for Lake Superior

The Great Lakes have a significant amount of thermal mass, meaning it takes a long time for them to cool down as the seasons change from summer to autumn. Often during this time of year, the air overlying the lakes is warmer than the lakes themselves. As water evaporates from... Read More

The Great Lakes have a significant amount of thermal mass, meaning it takes a long time for them to cool down as the seasons change from summer to autumn. Often during this time of year, the air overlying the lakes is warmer than the lakes themselves. As water evaporates from the lake surface into the cold, dry air above, it quickly condenses into fog. GOES-19 and the NOAA Buoy Network can work together to identify such an event.

NOAA’s buoys are preimarily intended to measure waves and winds, but many of them have air and water temperatures as well. Here’s a time series of the recent air and water temperature observations from NOAA’s West Superior buoy, located in the middle of western Superior about 30 miles northeast of the Apostle Islands. Here, it is clear that since about 0500 UTC (midnight local time) on 10 September, the water temperature has been at or above the air temperature.

This is a clear recipe for fog as the unsaturated air quickly becomes overwhelmed with moisture that has evaporated from the lake. The buoy itself can confirm this, as it has a system of cameras that show an up close and personal view of conditions at that site.

Of course, there are only a handful of buoys in the otherwise vast expanse of Lake Superior. Most of the lake has no in situ information at all. This is yet another case where satellites can be useful. However, satellite observations of fog can be challenging, especially when relying on the infrared band. This is because fog is such a low cloud that its brightness temperature is effectively the same as the land. Take, for example, this view of the Band 13 (10.7 micron) infrared window channel. Clouds are easy to discern over the upper peninsula of Michigan and eastern Wisconsin, but things are much murkier over western Lake Superior. Is the fog uniform across the lake, or are there clearing spots that cannot be seen from this view because the lake and fog temperatures are basically the same?

This is where RGB views can help add significant insight. In the Day Microphysics view (shown here because local time is from 9-10 AM for these loops) it is evident that there is clearing along the Minnesota shore, where the blue of the surface can be clearly discerned by the greyish color of the fog. Such clearing is impossible to discern from the infrared satellite.

SSEC Researcher Kathy Strabala notes that during the portions of the lunar cycle where the moon is providing a lot of illumination, VIIRS can provide visible-like imagery at night that can also aid in fog detection. For this event, the closest full moon was on 7 September, just two days before. The following image from the VIIRS Direct Broadcast antenna at CIMSS Headquarters illustrates the impact of the moon’s light perfectly. Note that even though it is night, it is easy to see where the fog ends. Thanks, Kathy!

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5-minute GOES-19 Day Fog BTD (3.9 µm – 10.3 µm) images with buoy observations plotted in yellow, from 1301-1801 UTC on 10 September (courtesy Scott Bachmeier, CIMSS) [click to play MP4 animation]

GOES-19 Day Fog brightness temperature difference (BTD) images with plots of buoy data (above) revealed that Lake Superior buoy water temperatures were generally in the 52-54 F range, with air temperatures within 1-2 degrees F of the water temperatures.

The corresponding Day Fog BTD images with plots of METAR surface reports (below) helped to explain why the aforementioned gap in the fog off the North Shore of Minnesota began to fill in after about 1501 UTC — this was in response to the development of a lake breeze (note the shoreline-parallel cloud line that formed not far inland, along the leading edge of the lake breeze) as daytime heating progressed across the Arrowhead of Minnesota. This lake breeze then acted to draw the fog edge toward the coast.

5-minute GOES-19 Day Fog BTD (3.9 µm – 10.3 µm) images with METAR surface reports plotted in white, from 1301-1801 UTC on 10 September (courtesy Scott Bachmeier, CIMSS) [click to play MP4 animation]

The GOES-19 Cloud Thickness derived product (below) showed that much of the fog across western Lake Superior was 500-1000 ft thick.

5-minute GOES-19 Cloud Thickness derived product with buoy observations plotted in yellow, from 1401-1801 UTC on 10 September (courtesy Scott Bachmeier, CIMSS) [click to play MP4 animation]

A 30-meter resolution Landsat-8 “Natural Color” RGB image at 1652 UTC (below) displayed the intricate and non-uniform structure of the top of the lake fog layer — and also highlighted the presence of an undular bore east of the Apostle Islands.

Landsat-8 “Natural Color” RGB image at 1652 UTC on 10 September [click to enlarge]

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Severe thunderstorms produce giant hail and isolated tornadoes in the Southern Plains

1-minute Mesoscale Domain Sector GOES-19 (GOES-East) Visible and Infrared images (above) included time-matched (+/- 3 minutes) SPC Storm Reports — which showed discrete supercell thunderstorms that produced giant hail (as large as 4.00 inches in diameter in southwest Kansas at 2215 UTC and 2343 UTC, and 3.50 inches in diameter in the northeast Texas Panhandle... Read More

1-minute GOES-19 “Red” Visible (0.64 µm, left) and “Clean” Infrared Window (10.3 µm, right) images with time-matched (+/- 3 minutes) SPC Storm Reports plotted in red/cyan, from 2130 UTC on 08 September to 0030 UTC on 09 September [click to play animated GIF | MP4]

1-minute Mesoscale Domain Sector GOES-19 (GOES-East) Visible and Infrared images (above) included time-matched (+/- 3 minutes) SPC Storm Reports — which showed discrete supercell thunderstorms that produced giant hail (as large as 4.00 inches in diameter in southwest Kansas at 2215 UTC and 2343 UTC, and 3.50 inches in diameter in the northeast Texas Panhandle at 2352 UTC) on 08 September 2025. There were also tornadoes at 2257 UTC in Oklahoma and at 0005 UTC in Texas.

Pulses of overshooting tops exhibited infrared brightness temperatures as cold as -75ºC — which represented a ~2 km overshoot of the Most Unstable (MU) air parcel’s Equilibrium Level (EL), according to 0000 UTC rawinsonde data from Amarillo, Texas (below).

Plot of rawinsonde data from Amarillo, Texas at 0000 UTC on 09 September [click to enlarge]

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Effects of a lunar eclipse on GOES-18/GOES-19 SUVI imagery

A total lunar eclipse occurred on 07 September 2025 (Space.com) — and as the Moon moved between GOES-18 (GOES-West), GOES-19 (GOES-East) and the Sun, SUVI imagery was totally obscured. The period that the Moon totally blocked the Sun was from 0840-0928 UTC with GOES-18 (above), and from 0434-0522 UTC with... Read More

GOES-18 SUVI Fe171 (171 Å) images, from 0652-1000 UTC on 07 September [click to play MP4 animation]

A total lunar eclipse occurred on 07 September 2025 (Space.com) — and as the Moon moved between GOES-18 (GOES-West), GOES-19 (GOES-East) and the Sun, SUVI imagery was totally obscured. The period that the Moon totally blocked the Sun was from 0840-0928 UTC with GOES-18 (above), and from 0434-0522 UTC with GOES-19 (below).

The times that the Moon’s edge was beginning to move away from the Sun were 0932 UTC as seen from GOES-18, and 0526 UTC as seen from GOES-19. Several solar prominences were apparent as they emanated from the eastern/northeastern limb of the Sun. These SUVI images were sourced from the SSEC Geostationary Satellite Imagery site.

GOES-19 SUVI Fe171 (171 Å) images, from 0326-0602 UTC on 07 September [click to play MP4 animation]

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Lightning causes a delay during the Eagles vs Cowboys football game

Lightning caused a 1-hour delay in the Eagles vs Cowboys football game at Lincoln Financial Field in Philadelphia (NFL.com) during the evening hours on 04 September 2025 (as a pre-frontal squall line was approaching the area) — the delay lasted from 10:25 pm ET (0225 UTC on 05 September) to 11:30... Read More

Plot of LightningCast Probability and GLM Flash Extent Density at/near Lincoln Financial Field in Philadelphia [click to enlarge]

Lightning caused a 1-hour delay in the Eagles vs Cowboys football game at Lincoln Financial Field in Philadelphia (NFL.com) during the evening hours on 04 September 2025 (as a pre-frontal squall line was approaching the area) — the delay lasted from 10:25 pm ET (0225 UTC on 05 September) to 11:30 pm ET (0330 UTC on 05 September). A plot of GOES-19 LightningCast Probability and GOES-19 (GOES-East) GLM Flash Extent Density (above) displayed the increase in LightningCast Probability and Flash Extent Density around the time of the game delay.

An animation of 5-minute CONUS Sector GOES-19 Infrared images with an overlay of Flash Extent Density and contours of LightningCast Probability (below) showed the thunderstorms with satellite-detected lightning activity as they approached Philadelphia and Lincoln Financial Field (the cyan dot just south of Philadelphia).

5-minute GOES-19 Infrared, GLM Flash Extent Density and contours of LightningCast Probability [click to play MP4 animation]

1-minute Mesoscale Domain Sector GOES-19 Infrared images with overlays of GLM Flash Extent Density, parallax-corrected GLM Flash Points and parallax-corrected contours of LightningCast Probability (below) provided a closer view at higher temporal resolution. Lincoln Financial Field is located about 5 miles northeast of Philadelphia International Airport (KPHL).

1-minute GOES-19 Infrared images with overlays of GLM Flash Extent Density, GLM Flash Points and contours of LightningCast Probability, from 0030-0330 UTC on 05 September [click to play MP4 animation]

There was satellite-detected lightning activity just west of the stadium at 0234 UTC, about 10 minutes after the game was initially delayed (below), and very near the stadium at 0240 UTC — close to the time that the Twitter photo of a cloud-to-ground lightning strike was taken (see the bottom of this blog post).

GOES-19 Infrared image with overlays of GLM Flash Extent Density, GLM Flash Points and contours of LightningCast Probability, at 0234 UTC on 05 September [click to enlarge]

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