For the first time since the early 1970s, humans are on their way to the moon. A partly cloudy sky over Cape Canaveral and Florida’s Space Coast provided a perfect backdrop for GOES-19 mesoscale imagery. Watch the True Color RGB imagery as the most powerful rocket that NASA has ever built shoots eastward across the Atlantic and towards its lunar destination.

The 3.9 micron channel, normally used for fires, can also be used to track the rocket in flight as long the solid rocket boosters and main engines are firing. This loop is the same time and area as the true color image above, but the rocket is shown as the large, rapidly moving dark (hot) spot.

This is also an interesting application for GOES CSPP Level 2 products. Here’s the cloud height product for shortly after launch. The plume is easily over 10000 m right after launch according to this algorithm.

On 6 April 2026, the astronauts will fly around the moon and be further from Earth than any humans have ever been.

View only this post Read Less

Overlapping 1-minute Mesoscale Domain Sectors provided 30-second imagery from GOES-19 (GOES-East) to support the launch of Artemis II — and Rocket Plume RGB images created using Geo2Grid (above) displayed both the hot thermal signature of the NASA Space Launch System (SLS) Core Stage rocket booster near the Kennedy Space Center launch site (brighter red pixels: 2235 UTC) in addition to the high-altitude thermal signature of moisture-laden rocket exhaust (brighter shades of green: 2239 UTC) as the spacecraft moved quickly eastward away from Florida after launch at 2235 UTC on 01 April 2026.

Multi-panel displays of GOES-19 imagery (below) revealed that reflectance and/or thermal signatures of the SLS rocket booster and its condensation plume were apparent in all 16 ABI spectral bands.

A GOES-18 (GOES-West) Mesoscale Domain Sector was also positioned over the launch area — and in spite of a much of a much larger satellite viewing angle, reflectance and/or thermal signatures of the SLS rocket booster and its condensation plume were also seen in all 16 of the GOES-18 ABI spectral bands (below).

A larger-scale view of 1-minute GOES-18 Water Vapor imagery (below) tracked the thermal signature of the SLS Core Stage booster as it approached the eastern limb of the satellite view at 2341 UTC.

30-second GOES-19 True Color RGB images (below) showed the SLS rocket booster’s condensation cloud as it initially arched northeast away from the Florida coast — but wind shear soon began to deform the cloud feature.

View only this post Read Less

1-minute Mesoscale Domain Sector GOES-19 (GOES-East) Visible, Water Vapor and Infrared images (above) showed the development of vertically-propagating standing wave clouds over far northeastern South Dakota on 28 March 2026 — initiated by strong SW winds interacting with the topography of the Coteau des Prairies.

The coldest cloud-top infrared brightness temperatures of the standing wave cloud features were around -45ºC — which roughly corresponded to the 300 hPa pressure level (or an altitude just below 9 km), according to rawinsonde data from Aberdeen SD (below).

A toggle between the GOES-19 images at 1600 UTC and topography (below) included plots of surface wind barbs (white) and RAP model 850 hPa wind barbs (beige) at that time. This helped to visualize the strong flow across the higher terrain that was responsible for generating the standing wave clouds immediately downwind of the Coteau des Prairies (the terrain elevation along the eastern edge abruptly drops from about 2.0 kft to around 1.1 kft — making the formation mechanism of these cloud features similar to those that develop along the coast of northeastern Minnesota).

Wind gusts across and to the lee of the Coteau reached the 60-70 mph range (below).

1-minute GOES-19 True Color RGB images from the CSPP GeoSphere site (below) revealed the quasi-stationary nature of the orographically-forced wave clouds.

View only this post Read Less

During the day of 27 March 2026, a band of strong strorms propagated from north of the Samoan islands southward to the island themselves. These storm were notable for deep convection and strong environmental instability and were the cause of flood warnings across American Samoa.

A good first look at the environment supporting these storm comes from the NUCAPS vertical profile retrievals. Here’s a profile from the NOAA-20 satellite from just south of the area where convection formed. This is from 13:23 UTC, which corresponds to 2:23 AM in American Samoa Standard Time. Even though it’s the middle of the night, 4822 J/kg of surface-based CAPE is present. The downdraft CAPE is also significant at 895 J/kg, and the sounding is moist (although not atypically high for this region) at 1.87 inches of precipitable water. Together, these values indicate a strong possibility of deep convection and significant rainfall.

The CIMSS MIMIC-TWP2 brings some larger-scale context to the high amounts of water vapor. This loop spans from 0400 UTC on the 27th to 0500 UTC on the 28th. Looking at the Samoan Islands (southwest of the intersection of 10 S and 170 W), it’s clear that they lie in the heart of a strong plume of atmospheric moisture.

The Band 13 (10.3 micron) imagery from GOES-18 also helps show the intensity of the convection, with numerous overshooting tops seen throughout this field of view. These are seen as the grey regions embedded in the darker black areas in the enhanced color scale on the Band 13 imagrey.

It may be easier to recognize the areas of intense convection using the Day Convection RGB. Here, the most vigorous updrafts are visible as bright yellows. Note that the colors seem to fade to a more pastel tone as the loop continues. This is because this particular loop runs between 0100 to 0450 UTC on the 28th. That’s 2:00 to 5:50 PM in local time, and sunset is at 6:28 PM. This product depends on several different shortwave channels (0.64, 1.6, and 3.9 microns) and thus the fading daylight at the end of this loop makes this product increasingly unreliable.

An interesting phenomenon can be seen in the visible imagery during the morning. Lots of outflow boundaries are seen propagating southward of the main convection located to the north of the Samoan islands; note the thin bands of clouds that form in the middle of the image at the end of the loop. Here is where we are seeing the impact of the strong downdraft CAPE (DCAPE) from the NUCAPS sounding at the top of this post. DCAPE represents the tendency of a parcel that is perturbed downwards to keep going down. Areas with high DCAPE are prone to strong evaporatively-cooled downdrafts which force strong winds when they collide with the surface and propagate outward. These downbursts fizzled out before they reached land which makes it hard to determine just how strong they are given the lack of surface observations in the ocean.

View only this post Read Less