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Large-Scale Fog over Lake Superior

An intriguing fog event took place over Lake Superior on Sunday, 15 February. On a day that was otherwise clear and unseasonably warm, fog crept westward as though it was trying to cover the entire lake. The following animation shows the entire day of GOES-19 true color imagery as viewed... Read More

An intriguing fog event took place over Lake Superior on Sunday, 15 February. On a day that was otherwise clear and unseasonably warm, fog crept westward as though it was trying to cover the entire lake. The following animation shows the entire day of GOES-19 true color imagery as viewed by SSEC’s Real Earth. There even appears to be a hint of rotation evident as the fog against the north shore appears to rap around the center of the open water.

It’s worth looking at what might have caused this event. First, let’s look at the Day Cloud Phase Distinction RGB for a portion of this period. In this product, low-level liquid clouds (like fog) appear blue/cyan while surface water is black and surface snow and ice are green. The surface observations for this time have also been overlaid on this image.

This is a challenging time of the year to discern what conditions are like over the Great Lakes thanks to freezing conditions. Buoys have generally been removed to protect them from damage from the ice, and satellite-based wind observations are also inhibited by the ice. Thus, we are largely flying blind over the lake itself. Still, we can put some things together. First, note how cold air is pooling within the lake basin. This is especially evident when looking at the western tip of Superior. There are three ASOS stations in greater Duluth, Minnesota. The Duluth International Airport is located on the continental crust at an elevation of 1428 feet above sea level. The Richard Bong Airport in Superior is located on the mid-continental rift at a much lower elevation of 674 feet. However, Sky Harbor airport is located on a sand bar in the lake and has a much lower elevation of 609 feet. At 1926 UTC (1:26 PM local time), that lower elevation is at least 10 degrees colder than the surrounding, higher elevations. We know that the lake surface temperature is near freezing given the presence of the ice. From all of this, we can infer that there is a decently strong inversion present over the lake. Note also that the near-lake air is already close to saturation, as the Sky Harbor dew point is just 2 degrees F less than the air temperature.

A similar dynamic can be seen further up the coast at Grand Marais, Minnesota. Here, the airport is 8 miles inland and over 1,000 feet above the lake surface, where an additional set of observations is available. Note how the lake air is a full 11 degrees colder than the airport location, while both sites have the same dew point.

Next, there appears to be a weak low pressure system near the border of Wisconsin and Michigan’s Upper Peninsula, as seen in the following NOAA Weather Prediction Center surface analysis. With the low to the south of Lake Superior, we would expect weak easterly flow over the lake, which is more or less backed up by the surface wind observations above.

The fog itself is quite shallow, which we can determine by looking at the brightness temperature of the top of the fog. Since fog acts as a near-blackbody in the infrared window, the brightness temperature of the fog in Band 13 is a reasonable estimate of the temperature of the top of the fog. The AWIPS readout tool says that the IR brightness temperature in the middle of the fog is -5 C, or about 23 F. The IR brightness temperature of the clear lake is only slightly warmer at -2.6 C (27 F ,not shown).

Putting it all together, we have easterly flow, a strong inversion, and a shallow fog layer that is both thick and uniform. Based on this, it’s likely that this is an advection fog. Warmer air from the non-lake regions moved into the cold lake basin, where it cooled and reached saturation. Since air is a poor conductor of heat, the air above the surface stayed warm which was reflected in the higher temperatures of the more elevated locations.

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Satellite signatures of the NASA/SpaceX Crew-12 launch

The NASA/SpaceX Crew-12 Mission to the International Space Station was launched from Kennedy Space Center in Florida at 1015 UTC on 13 February 2026 — and overlapping 1-minute Mesoscale Domain Sectors from GOES-19 (GOES-East) provided 30-second images from all 16 ABI spectral bands (above). Since this was a nighttime launch, varying shades of white... Read More

16-panel display of 30-second GOES-19 images from all 16 ABI spectral bands, from 1014-1020 UTC on 13 February [click to play animated GIF]

The NASA/SpaceX Crew-12 Mission to the International Space Station was launched from Kennedy Space Center in Florida at 1015 UTC on 13 February 2026 — and overlapping 1-minute Mesoscale Domain Sectors from GOES-19 (GOES-East) provided 30-second images from all 16 ABI spectral bands (above). Since this was a nighttime launch, varying shades of white signatures of the Falcon 9 rocket booster were seen in the Visible (02) and Near-Infrared (03-06) spectral bands as the rocket ascended to the northeast — while warmer rocket booster thermal signatures were apparent in many of the Infrared spectral bands (07-16) [10:17:25 UTC 16-panel images]. In addition, a cooler signature of the rocket’s condensation cloud was evident in many of the Infrared spectral bands, as that cloud drifted southeastward just offshore.

In spite of an oblique satellite viewing angle, many of the same Falcon 9 rocket booster signatures were seen in 1-minute GOES-18 (GOES-West) imagery (below) [1016 UTC 16-panel images]. (The 16-panel GOES-19 and GOES-18 images were displayed in their respective native satellite projections.)

16-panel display of 1-minute GOES-18 images from all 16 ABI spectral bands, from 1014-1020 UTC on 13 February [click to play animated GIF]

A slightly longer animation of 30-second GOES-19 Nighttime Microphysics RGB images from the CSPP GeoSphere site (below) showed the aforementioned rocket booster condensation cloud (darker shades of blue) drifting southeast just offshore — along with the hot thermal signature (darker purple pixel) of the rocket booster landing burn as it returned to the launch site at 1023 UTC.

30-second GOES-19 Nighttime Microphysics RGB images (with/without a map overlay), from 1014-1023 UTC on 13 February [click to play animated GIF]

30-second GOES-19 Rocket Plume RGB images created using Geo2Grid (below) provided a larger-scale view of the rocket booster signature as the Falcon 9 traveled northeast away from the launch site.

30-second GOES-19 Rocket Plume RGB images, from 1014-1020 UTC on 13 February [click to play animated GIF | MP4]

A comparison of 1-minute Rocket Plume RGB images from both GOES-18 and GOES-19 (below) nicely demonstrated the effect of parallax — since the satellite viewing angle from GOES-18 was 68.98 degrees from the southwest (compared to only 33.56 degrees from the south-southeast from GOES-19), the apparent location of the high-altitude Rocket Plume RGB signature was displaced much farther to the east as viewed from GOES-18 (1018 UTC images). (The GOES-18/GOES-19 Rocket Plume RGB images were re-mapped to a common projection.)

1-minute Rocket Plume RGB images from GOES-18 (left) and GOES-19 (right), from 1014-1020 UTC on 13 February [click to play animated GIF | MP4]

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Ice leads in the Beaufort Sea

VIIRS Infrared images from Suomi-NPP and NOAA-21 (above) showed widespread ice leads (brighter shades of cyan) in the Beaufort Sea during the 3-day period from 10-12 February 2026 — with a notable increase in ice leads across the eastern Beaufort Sea.Surface wind stress was the primary influence affecting the motion... Read More

Suomi-NPP and NOAA-21 VIIRS Infrared Window (11.45 µm) images, from 1636 UTC on 10 February to 2053 UTC on 12 February [click to play animated GIF]

VIIRS Infrared images from Suomi-NPP and NOAA-21 (above) showed widespread ice leads (brighter shades of cyan) in the Beaufort Sea during the 3-day period from 10-12 February 2026 — with a notable increase in ice leads across the eastern Beaufort Sea.

Surface wind stress was the primary influence affecting the motion and evolution of these ice leads. Surface analyses (below) showed that a tighter pressure gradient developed across the Beaufort Sea during the 3-day period — between high pressure centered over the Siberian Sea and broad cyclonic flow across the Bering Sea and interior/northern Alaska — which would have induced a stronger easterly flow across much of the VIIRS image domain displayed above.

6-hourly surface analyses, from 1200 UTC on 10 February to 1800 UTC on 12 February [click to play animated GIF]

Daily results using an AI-based sea ice lead detection method covering the entire Arctic Ocean are shown below; the Beaufort Sea is located within the bottom right portion of the images.

Daily VIIRS Sea Ice Lead Detections, from 10-12 February [click to enlarge]

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Cyclone Gezani makes landfall on Madagascar as a Category 3 storm

EUMETSAT Meteosat-9 Infrared images (above) showed Cyclone Gezani as it made landfall along the east coast of Madagascar (near the city of Toamasina, station identifier FMMT) around 1645 UTC on 10 February 2026 — as a 110-kt Category 3 storm (JTWC discussion). Gezani had been rapidly intensifying on 10 February prior... Read More

Meteosat-9 Infrared Window (10.8 µm) images, from 0600-1900 UTC on 10 February [click to play animated GIF]

EUMETSAT Meteosat-9 Infrared images (above) showed Cyclone Gezani as it made landfall along the east coast of Madagascar (near the city of Toamasina, station identifier FMMT) around 1645 UTC on 10 February 2026 — as a 110-kt Category 3 storm (JTWC discussion). Gezani had been rapidly intensifying on 10 February prior to landfall (ADT | SATCON). After landfall, the eye of Gezani quickly became cloud-filled as the storm interacted with the topography of the island. Gezani was responsible for at least 41 fatalities, and displaced more than 16000 residents.

A time series of surface data from Toamasina (below) depicted a wind gust of 73 kts at 1500 UTC — their final report before apparently abandoning the airport, or stronger winds subsequently causing power outages.

Time series of surface data from Toamasina, Madagascar [click to enlarge]

An ATMS Microwave image (below) displayed the eyewall of Gezani at 1034 UTC, about 1.5 hours prior to the storm reaching Category 3 intensity.

ATMS Microwave (183 GHz) image at 1034 UTC on 10 February

Meteosat-9 Infrared images with an analysis of deep-layer wind shear (below) indicated that Gezani was moving through an environment of very low shear — a factor that was favorable for the tropical cyclone reaching Category 3 intensity several hours prior to making landfall.

Meteosat-9 Infrared Window images, with contours and streamlines of deep-layer wind shear at 1200 UTC on 10 February

An analysis of Sea Surface Temperature (below) showed that Gezani had been traversing relatively warm water, with SST values of 28C.

Sea Surface Temperature (SST) analysis, with the track of Gezani ending at 1200 UTC on 10 February

ADT, SATCON, ATMS, Wind Shear and SST imagery were sourced from the CIMSS Tropical Cyclones site.

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