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VIIRS Infrared images from Suomi-NPP and NOAA-21 (above) showed widespread ice leads in the Chukchi Sea during the 3-day period from 06-08 January 2026. A combination of surface wind stress and ocean currents influenced the motion and evolution of these ice leads.Surface analyses (below) showed a tighter pressure gradient across the... Read More
Suomi-NPP and NOAA-21 VIIRS Infrared images, from 0028 UTC on 06 January to 2332 UTC on 08 January [click to play animated GIF | MP4]
VIIRS Infrared images from Suomi-NPP and NOAA-21 (above) showed widespread ice leads in the Chukchi Sea during the 3-day period from 06-08 January 2026. A combination of surface wind stress and ocean currents influenced the motion and evolution of these ice leads.
Surface analyses (below) showed a tighter pressure gradient across the Chukchi Sea early in the 3-day period, as high pressure was approaching from the Siberian Sea — which would have induced a stronger northerly flow across the VIIRS image domain displayed above. As the core of this high pressure settled over eastern Siberia on 08 January, the pressure gradient relaxed across much of the Chukchi Sea, with a lighter westerly flow likely becoming more prominent toward the end of the 3-day period.
6-hourlty surface analyses, from 0000 UTC on 06 January to 0000 UTC on 09 January [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 Chukchi Sea is located near the bottom center of the images.
AI-based VIIRS sea ice lead detection from 06-08 January [click to enlarge]
1-minute Mesoscale Domain Sector GOES-19 (GOES-East) Water Vapor and Visible images (above) included plots of Pilot Reports (PIREPs) of Moderate to occasionally Severe turbulence — several of which were in the vicinity of mountain waves over parts of eastern Colorado on 05 January 2026. It was notable that in the area where mountain... Read More
1-minute GOES-19 Water Vapor images (6.9 µm, left) and Visible images (0.64 µm, right) with plots of Pilot Reports of turbulence, from 1811-2310 UTC on 05 January [click to play MP4 animation]
1-minute Mesoscale Domain Sector GOES-19 (GOES-East) Water Vapor and Visible images (above) included plots of Pilot Reports (PIREPs) of Moderate to occasionally Severe turbulence — several of which were in the vicinity of mountain waves over parts of eastern Colorado on 05 January 2026. It was notable that in the area where mountain waves were very apparent in Water Vapor images (immediately downwind of the high terrain of the Rocky Mountains), there were no clouds seen in the corresponding Visible images.
Cursor samples of 2 PIREPs of Moderate to Severe turbulence are shown below. In the immediate vicinity of the earlier 1939 UTC PIREP, the distinct signature of mountain waves — adjacent bands of warm/dry subsiding air (shades of yellow) and cool/moist rising air (shades of blue) — was evident in the Water Vapor image.
GOES-19 Water Vapor image (6.9 µm, left) and Visible image (0.64 µm, right) at 1939 UTC on 05 January, with a cursor sample of a PIREP of Moderate to Severe turbulence between the altitudes of 12500-13500 ft [click to enlarge]
GOES-19 Water Vapor image (6.9 µm, left) and Visible image (0.64 µm, right) at 2310 UTC on 05 January, with a cursor sample of a PIREP of Moderate to Severe turbulence at an altitude of 11000 ft [click to enlarge]
A common sight on calm nights and early mornings is radiation fog: as the surface cools at night, the air above the ground cools as well. The absolute moisture content of the air remains the same, but since the temperature is dropping less water vapor can be contained in equilibrium... Read More
A common sight on calm nights and early mornings is radiation fog: as the surface cools at night, the air above the ground cools as well. The absolute moisture content of the air remains the same, but since the temperature is dropping less water vapor can be contained in equilibrium and thus the relative humidity goes up. If the temperature cools enough, it will reach the dew point and fog will form.
But what happens when you throw a dense city into the mix? Cities are warmer than the surrounding land for a number of reasons. First and foremost, the building materials like concrete and asphalt that are prevalent in cities are better at absorbing the sun’s energy than vegetation is. The vertical dimension of cities also matters: the perpendicular surfaces of tall buildings strongly absorb the sun’s rays when the sun is low in the sky and the rest of the landscape is absorbing very little, and the infrared radiation that is emitted outward by one building is often absorbed by a different building right next door. Thus, cities retain their heat at night in a phenomenon known as the urban heat island, or UHI.
On the morning of 5 January 2026, widespread areas of radiation fog were visible over the southeastern continental United States, as large scale nocturnal cooling took place over the Carolinas and Georgia. This can be seen in the Day Cloud Phase Distinction RGB from the GOES-19 geostationary satellite as large regions of cyan clouds. Note how the clouds seem to follow terrain, which is expected for fogs. This particular loop spans the period from before to after sunrise, and (as one can guess from the name) the Day Cloud Phase Distinction product is a daytime only product, so it really only the end of the loop that can be interpreted in this way.
However, something interesting happens when you zoom in on Atlanta, Georgia. While the population of the city of Atlanta proper is relatively small (fewer than 500,000 people), it is the heart of the nation’s 8th largest metropolitan area, ranking it ahead of the Philadelphia, Phoenix, or Boston metros. With so much development, it has a well-pronounced UHI. Let’s look at the same product, zoomed into the Atlanta metro. This map shows the Interstate highways, and the center of the image where the highways all converge is the heart of Atlanta.
Note the gap in the fog right in the heart of the city. This is because the urban heat island kept the temperature of the central core of the city from cooling enough to allow fog to form. In the regions further out, however, the UHI was weaker. Out there, the air cooled more and condensation was able to take place. Sometimes, if you want to avoid the fog, all you have to do is head downtown.
10-minute Full Disk scan GOES-19 (GOES-East) True Color RGB images along with the Aerosol Optical Depth derived product from the CSPP GeoSphere site (above) showed a pulse of blowing dust that was moving northward and westward across the northern Patagonia region of Argentina on 01 January 2026.Surface analyses (below) depicted a cold front that was... Read More
10-minute GOES-19 True Color RGB images (left) and Aerosol Optical Depth derived product (right), from 1500-2300 UTC on 01 January 2026 [click to play MP4 animation]
10-minute Full Disk scan GOES-19 (GOES-East) True Color RGB images along with the Aerosol Optical Depth derived product from the CSPP GeoSphere site (above) showed a pulse of blowing dust that was moving northward and westward across the northern Patagonia region of Argentina on 01 January 2026.
Surface analyses (below) depicted a cold front that was moving northward across that area during the day — a narrow cloud band denoted part of the leading edge of this cold front. The circulation around a compact area of high pressure that developed along the coast (south of the cold front, at 0000 UTC) acted to transport some of the blowing dust farther inland (westward).
Surface analyses at 1200 UTC on 01 January and 0000 UTC on 02 January [click to enlarge]