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10-minute Full Disk scan GOES-19 (GOES-East) Water Vapor images centered over the southern Great Lakes (above) included contours of Moderate Or Greater (MOG) Turbulence Probability (yellow contour = 40%) and Pilot Reports of Turbulence on 20 November 2025. The yellow 40% MOG contour progressed eastward across the southern Great Lakes and toward the... Read More
GOES-19 Water Vapor imagery with contours of Moderate Or Greater (MOG) Turbulence Probability and plots of Pilot Reports of turbulence, from 1150-1900 UTC on 20 November [click to play MP4 animation]
10-minute Full Disk scan GOES-19 (GOES-East) Water Vapor images centered over the southern Great Lakes (above) included contours of Moderate Or Greater (MOG) Turbulence Probability (yellow contour = 40%) and Pilot Reports of Turbulence on 20 November 2025. The yellow 40% MOG contour progressed eastward across the southern Great Lakes and toward the Northeast US during the day — note the appearance of one report of Extreme Turbulence over the southwest portion of Lower Michigan around 1500 UTC.
Products from the Aviation Weather Center allowed cursor samples of two closely-spaced Pilot Reports of Extreme Turbulence — apparently from the same aircraft, as it was flying southeast (below).
Cursor sample of a Pilot Report of Extreme Turbulence at 1450 UTC on 20 November [click to enlarge]
The second encounter of Extreme Turbulence occurred at 1505 UTC, causing minor injuries (below).
Cursor sample of a Pilot Report of Extreme Turbulence (causing minor injuries) at 1505 UTC on 20 November [click to enlarge]
A toggle between the 1501 UTC GOES-19 Water Vapor image and a 3-hour NAM40 model forecast of 250 hPa winds valid at 1500 UTC (below) indicated that the initial 1450 UTC Pilot Report of Extreme Turbulence (red symbol) occurred in an area of strong speed shear just north of the axis of a 150-knot jet streak (shades of orange). There was also the characteristic dry/moist gradient in Water Vapor imagery along the axis of the upper-tropospheric jet streak.
Toggle between the GOES-19 Water Vapor image at 1501 UTC and a 3-hour NAM40 model forecast of 250 hPa Wind Speed valid at 1500 UTC on 20 November; the 1450 UTC Pilot Report of Extreme Turbulence is plotted in red [click to enlarge]
An animation of 5-minute CONUS Sector GOES-19 Water Vapor images with Pilot Reports of Turbulence is shown below.
5-minute GOES-19 Water Vapor images with plots of Pilot Reports of turbulence, from 1121-2001 UTC on 20 November [click to play MP4 animation]
Thanks to Rick DiMaio for alerting us to this case!
10-minute Full Disk scan GOES-19 (GOES-East) daytime True Color RGB + nighttime Dust RGB images — created using Geo2Grid (above) showed the offshore transport of significant amounts of blowing dust from the Patagonia region of southern Argentina on 17-18 November 2025.A slightly longer period of GOES-19 Dust RGB images (below) displayed the... Read More
10-minute GOES-19 daytime True Color RGB and nighttime Dust RGB images, from 1200 UTC on 17 November to 0710 UTC on 18 November [click to play animated GIF]
10-minute Full Disk scan GOES-19 (GOES-East) daytime True Color RGB + nighttime Dust RGB images — created using Geo2Grid(above) showed the offshore transport of significant amounts of blowing dust from the Patagonia region of southern Argentina on 17-18 November 2025.
A slightly longer period of GOES-19 Dust RGB images (below) displayed the plume of airborne dust (brighter shades of magenta) as it arced eastward then southward across the southern Atlantic Ocean.
10-minute GOES-19 Dust RGB images, from 1100 UTC on 17 November to 1500 UTC on 18 November [click to play animated GIF]
10-minute GOES-19 daytime True Color RGB and Nighttime Microphysics RGB images, from 1200 UTC on 17 November to 0700 UTC on 18 November [click to play MP4 animation]
Strong boundary layer winds — which lofted the areas of blowing dust — developed in the wake of a cold front associated with a low pressure system that was deepening off the coast of Argentina (below).
12-hour surface analyses, from 0000 UTC on 17 November to 1200 UTC on 18 November [click to play animated GIF]
There was a wind gust to 75 kts (86 mph) at METAR site SAVC at 1500 UTC — and for several hours leading up to that time, blowing dust had reduced the surface visibility to less than 1 mile at that airport (below).
Cursor sample of the Comodoro, Argentina (SAVC) METAR at 1500 UTC on 17 November [click to enlarge]
Time series of surface observation data at Comodoro, Argentina (SAVC) from 1000-2200 UTC on 17 November [click to enlarge]
5 hours later there was a wind gust to 61 kts (70 mph) at METAR site SAVT at 2000 UTC — and just before that time, blowing dust reduced the surface visibility to about 1 mile at that airport (below).
Cursor sample of the Trelew Almirante, Argentina (SAVT) METAR at 2000 UTC on 17 November [click to enlarge]
Time series of surface observation data at Trelew Almirante, Argentina (SAVT) from 0600 UTC on 17 November to 0000 UTC on 18 November [click to enlarge]
One of the most popular GOES products is the True Color RGB. There’s a lot to like about it: a constantly updating full color view of the planet, watching clouds swirl above sapphire seas and emerald forests. It can be positively mesmerizing to watch loops of this product, at least... Read More
One of the most popular GOES products is the True Color RGB. There’s a lot to like about it: a constantly updating full color view of the planet, watching clouds swirl above sapphire seas and emerald forests. It can be positively mesmerizing to watch loops of this product, at least until the sun sets, the terminator arrives, and the visible reflectances go away.
There is an important cacceat to remember, though. The GOES true color product isn’t really a true color image of the planet. The GOES ABI instrument is not like a consumer digital camera, in which separate channels record the red, blue, and green reflectance and assemble those into an easily recognizable photograph. Instead, while ABI has a blue channel (Channel 1, 0.47 microns) and a red channel (Channel 2, 0.64 microns), it doesn’t have a green channel. Instead, ground processing does a little trickery. Channel 3, at 0.86 microns, is very sensitive to vegetation. What we can do instead is create an RGB product where red is red, blue is (wait for it…) blue, and green is a channel that is strongly representative of surfaces that are green. Most of the time this works just fine for the majority of users.
However, this all relies on the assumption that vegetation is green. But what happens if you have a lot of vegetation that isn’t green at all? How would that appear on the GOES True Color RGB? This image, taken on 17 November 2025, shows the southeastern United States as seen from GOES-19. Note how lush the forests in this region look. There’s lots of green throughout the region. If you were looking to identify where fall colors weer at their peak, it might be challenging to do so with this image.
VIIRS tells a different story. This image, obtained via direct broadcast, was taken at approximately the same time from the NOAA-21 satellite. The VIIRS instrument has true red, green, and blue channels, so a true color RGB is much closer to what our eyes would perceive if we were looking down from space. Note how the green areas of this image are much smaller in extent. Florida, southern Alabama, and the coastal regions of Georgia and South Carolina still retain much of their verdant colors as before. However, the hardwood forests of Appalachia, including the dense forests along the Tennessee / North Carolina border, are much browner than before.
The following slider allows you to directly compare the two images to see how they differ. Check out how the colors along the coasts, where trees are still green, are mostly the same between the two images, but they are very different in the forested regions where leaves have already turned.
This slider also does a good job of illustrating parallax and how cloud height exacerbates it. As you slide the bar back and forth, note that there’s very small displacements in the positions of the low clouds, like the popcorn convection throughout the Florida peninsula. However, the high cirrus (likely aged contrails) over Georgia and Alabama show a much greater horizontal displacement due to the very different scanning positions of the two instruments.
This simple example shows that it’s important to remember that the GOES ABI True Color product is really representing an idealized version of what we think the planet is supposed to look like, rather than a direct capture of what it actually looks like right now. Note that this is not as much of an issue with many other geostationary satellites. The Flexible Combined Imager (FCI) on EUMETSAT’s Meteosat-12, the Advanced Himawari Imager (AHI) on the Himawari series operated by Japan, and the Advanced Meteorological Imager (AMI) on South Korea’s GEOKOMPSAT-2a all have the necessary channels to produce full spectrum true color images. Note that this is not true for SEVIRI, still in operational use over the Indian Ocean on Meteosat-9 and in wide use in central and eastern Asia. EUMETSAT’s Natural Color RGB is a combination of 1.6 (red), 0.8 (green), and 0.6 (blue), which has even fewer visible channels than the GOES True Color.
10-minute Full Disk scan JMA Himawari-8 Visible, Shortwave Infrared and Infrared Window images (above) showed 2 pulses of pyrocumulonimbus (pyroCb) clouds that were spawned by a large bushfire in Western Australia on 17 November 2025. The pyroCb cloud pulses exhibited a cloud-top 10.4 µm infrared brightness temperature (IRBT) of -40ºC... Read More
10-minute Himawari-8 “Red” Visible (0.64 µm, left), Shortwave Infrared (3.9 µm, middle) and “Clean” Infrared Window (10.4 µm, right) images, from 0400-0800 UTC on 17 November [click to play animated GIF]
10-minute Full Disk scan JMA Himawari-8 Visible, Shortwave Infrared and Infrared Window images (above) showed 2 pulses of pyrocumulonimbus (pyroCb) clouds that were spawned by a large bushfire in Western Australia on 17 November 2025. The pyroCb cloud pulses exhibited a cloud-top 10.4 µm infrared brightness temperature (IRBT) of -40ºC or colder (denoted by darker blue pixels) — a necessary condition to be classified as a pyroCb (since that temperature assures that heterogeneous glaciation has occurred at the cloud top). Note that the pyroCb cloud tops appeared as darker shades of gray in the Shortwave Infrared images, due to enhanced solar reflection off the smaller smoky ice crystals.
Himawari-8 Fire Temperature RGB + Infrared Window images viewed using RealEarth(below) indicated that the large bushfire was burning near the Zyotdorp Nature Reserve.
10-minute Himawari-8 Fire Temperature RGB + Infrared Window images, from 0400-0800 UTC on 17 November [click to play MP4 animation]