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Tropical Storm Lala becomes a Category 1 Hurricane south of the Big Island of Hawai`i

1-minute Mesoscale Domain Sector GOES-18 (GOES-West) Infrared Window and Visible images (above) showed Tropical Storm Lala as it intensified to become a Category 1 Hurricane at 1900 UTC on 15 August 2026 (GOES-18 images | NHC advisory) south of the Big Island of Hawaii. Lala exhibited a rather ragged eye that remained... Read More

1-minute GOES-18 Infrared Window (left) and Visible images (right) with overlays of GLM Flash Points and surface observation data, from 1610 UTC on 15 August to 0400 UTC on 16 August

1-minute Mesoscale Domain Sector GOES-18 (GOES-West) Infrared Window and Visible images (above) showed Tropical Storm Lala as it intensified to become a Category 1 Hurricane at 1900 UTC on 15 August 2026 (GOES-18 images | NHC advisory) south of the Big Island of Hawaii. Lala exhibited a rather ragged eye that remained generally cloud-filled — and while the hurricane did not make an official landfall, its northern eyewall did pass across the far southern tip of the Big Island. An overlay of 1-minute GOES-18 GLM Flash Points revealed that there was no intermittent satellite-detected lightning activity until 2323 UTC on 15 August. In terms of wind, some RAWS sites on the Big Island reported gusts in the 60-77 mph range, and Kona International Airport reported a peak wind of 64 knots (74 mph) — with a peak gust of 140 mph occurring at the Mauna Kea summit. Highest wind gusts at other islands included 85 mph in Maui County and 74 mph in Honolulu County.

The coldest overshooting tops surrounding the eye of Lala exhibited infrared brightness temperatures in the -75 to -80 C range (brighter white pixels embedded within dark black regions) — according to a plot of rawinsonde data from Hilo on the Big Island (below), those temperatures roughly corresponded to altitudes near or just above the Forecast Surface air parcel’s Equilibrium Level (EL).

Plot of rawnsonde data from Hilo, Hawai`i at 1800 UTC on 15 August [click to enlarge]

It is noteworthy that the Precipitable Water (PW) value on the Hilo sounding was 2.73 inches — which appears to be the highest PW value on record for Hilo, just eclipsing the prior record maximum value of 2.72 inches on 24 August 1961 (below).

Climatology of Precipitable Water (PW) for all Hilo, Hawai`i soundings [click to enlarge]

With an unusually moist atmosphere in place, heavy rainfall amounts in excess of 43 inches occurred on the Big Island. The MIMIC Total Precipitable Water product (below) indicated that Lala was drawing rich tropical moisture northward from the Intertropical Convergence Zone (ITCZ) as the tropical cyclone developed and moved northwestward toward Hawai`i.

MIMIC Total Precipitable Water product, from 0000 UTC on 11 August to 2300 UTC on 16 August

A sequence of storm-centered Rainfall Rate products derived using microwave data from the ATMS and AMSU instruments on a variety of polar-orbiting satellites is shown below — access to these and other Low-Earth Orbiting (LEO) satellite Direct Broadcast ground station products is discussed in this blog post.

Rain Rate derived using AMSU and ATMS microwave data, from 1131 UTC on 15 August to 2008 UTC on 16 August

The ample moisture of Hurricane Lala that was helping to produce the heavy rainfall was also producing snow at the summit of Mauna Kea, as documented by web camera video shortly before 0100 UTC on 16 August:

A sequence of rawinsonde data plots from Hilo (below) showed that the freezing level (labeled FZL, in cyan) was at its lowest height (15174 feet) at 0000 UTC on 16 August — which was only 1371 feet (418 meters) above the Mauna Kea summit elevation of 13803 feet. Larger snowflake aggregates falling from clouds above Mauna Kea would likely not have melted entirely before arriving at the summit.

Plots of rawinsonde data from Hilo at 1800 UTC on 15 August, 0000 UTC on 16 August and 0600 UTC on 16 August

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A 3-day animation of GOES-18 daytime True Color RGB + Nighttime Microphysics RGB images (below) displayed the northwestward trek of Lala from 14-16 August.

It is interesting to note that on 14 August, as Lala was still well southeast of the Big Island, a hazy plume of “vog” (volcanic fog) could be seen southwest of the island — which was emitted by Episode 53 of an ongoing eruption of Kilauea (the hot thermal anomaly of the volcano’s lava flow showed up as a small cluster of dark purple pixels in Nighttime Microphysics RGB imagery).

5-minute GOES-18 daytime True Color RGB + Nighttime Microphysics RGB images, from 0001 UTC on 14 August to 2356 UTC on 16 August

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Tropical Storm Lala develops southeast of Hawai`i

1-minute Mesoscale Domain Sector GOES-18 (GOES-West) Visible images (above) and Infrared Window images (below) showed the slow organization of cloud features associated with Tropical Storm Lala southeast of Hawai’i on 13 August 2026. Overlays of GOES-18 GLM Flash Points indicated that lightning activity was sparse during that time period. Lala was moving... Read More

1-minute GOES-18 Visible images with an overlay of GLM Flash Points, from 1914 UTC on 13 August to 0013 UTC on 14 August

1-minute Mesoscale Domain Sector GOES-18 (GOES-West) Visible images (above) and Infrared Window images (below) showed the slow organization of cloud features associated with Tropical Storm Lala southeast of Hawai’i on 13 August 2026. Overlays of GOES-18 GLM Flash Points indicated that lightning activity was sparse during that time period. Lala was moving through an environment of very low deep-layer wind shear and traversing fairly warm Sea Surface Temperatures — factors which favored further intensification as Lala approached Hawai’i.

1-minute GOES-18 Infrared Window images with an overlay of GLM Flash Points, from 1914 UTC on 13 August to 0013 UTC on 14 August

During the preceding nighttime hours, before Potential Tropical Cyclone One-C had intensified to become Tropical Storm Lala, VIIRS Day/Night Band images from NOAA-20 and NOAA-21 (below) displayed the faint signature of cloud features — faint because the Moon had not yet risen at that location, so the only source of illumination was atmospheric airglow.

NOAA-21 VIIRS Day/Night Band image valid at 1035 UTC on 13 August [click to enlarge]
NOAA-20 VIIRS Day/Night Band image valid at 1131 UTC on 13 August [click to enlarge]

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Day/Night Band Observations of the Total Solar Eclipse

Eyes around the world were turned toward Greenland, Iceland, and Spain as a total solar eclipse tracked across parts of the Northern Hemisphere yesterday, 12 August 2026. If you haven’t already seen the CIMSS Blog post on yesterday’s total solar eclipse from the GOES perspective, be sure to check it out. However, this was a... Read More

Eyes around the world were turned toward Greenland, Iceland, and Spain as a total solar eclipse tracked across parts of the Northern Hemisphere yesterday, 12 August 2026. If you haven’t already seen the CIMSS Blog post on yesterday’s total solar eclipse from the GOES perspective, be sure to check it out. However, this was a high-latitude eclipse and it was difficult to see the lunar shadow from the standard geostationary view. By contrast, the polar-orbiting satellites of the Joint Polar Satellite System (JPSS) are able to view the eclipse from a much more direct angle. Here’s a static true color view from NOAA21’s VIIRS at 1720 UTC. Note the expected coloration over the eastern contiguous United States, but as you look further to the north you see the darkening of the ground due to increasingly obscured sunlight.

VIIRS true color view of the solar eclipse on 12 August 2026.

Even better, the JPSS satellites also feature the VIIRS imager. What better way to view the simultaneous day and night of a solar eclipse than the Day/Night Band? Let’s take a look! These images have been plotted via the excellent polar SLIDER resource from our colleagues and friends at the Cooperative Institute for Research in the Atmosphere. These images are North Pole views, with Alaska at the bottom center and Greenland off to the upper right. You can see much of the contiguous United States in the lower right.

The first hint of a partial eclipse began at 1534 UTC (7:34 AM Alaska time, for context). Therefore, this first image, at 1518 shows the pre-eclipse environment. SLIDER overlays previous swaths on the image, hence the nighttime lights in the United States. However, in general nothing too unusual appears to be going on.

VIIRS DNB view of the North  Pole at 1518 UTC on 12 August 2026.

The next swath is at 1603 UTC. The eclipse is only a few minutes old at this point, and there’s not really much that is easily identifiable as being an effect of the dimming sun. Still, we see lots of clouds over the North Pole and some clear seas between Greenland and Canada.

VIIRS DNB view of the North  Pole at 1603 UTC on 12 August 2026.

By the time we reach 1659 UTC, however, we see a substantial change in the darkness over eastern Siberia. The Day/Night band relies on moonlight when the sun is not available, and when the moon is not present the views are going to be dark. Geometrically, a solar eclipse can only take place during a new moon. Therefore the nighttime parts of the globe are going to be black, and the part of the Earth beneath the moon’s shadow will also be dark. This swath was right at the time the total eclipse first began.

VIIRS DNB view of the North  Pole at 1659 UTC on 12 August 2026.

With the next swath at 1744 UTC, we see that the shadow has moved to far northern Greenland. The eclipse reached it maximum at 1746 UTC, so this view represents the eclipse at effectively its greatest extent. We can see this as a dark hole in upper center-right of the next image, where previously Greenland clearly had snow, clouds, and ice.

VIIRS DNB view of the North  Pole at 1744 UTC on 12 August 2026.

The JPSS satellites are sun-synchronous, moving from east to west so that they feature largely similar solar characteristics from one swath to the next. Because of this, there are no further satellite views of the eclipse as it moved onward to Spain. Regardless, JPSS gave us a unique perspective of one of nature’s most thrilling (and predictable!) natural phenomena. Stay tuned to the CIMSS Satellite Blog on 2 August 2027, when we’ll be discussing the next solar eclipse which will be taking place over Spain, Africa, and the Mediterranean.

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Solar eclipse shadow as viewed by GOES-18 and GOES-19

10-minute Full Disk scan Near-Infrared “Vegetation” images from GOES-18/GOES-West (above) and GOES-19/GOES-East (below) revealed the shadow of a total solar eclipse on 12 August 2026 — which began by moving eastward across far northern Alaska and Arctic Canada, then curved southeast across Greenland, Iceland and far western Europe before fading from view... Read More

10-minute GOES-18 Near-Infrared “Vegetation” images, from 1500-1830 UTC on 12 August

10-minute Full Disk scan Near-Infrared “Vegetation” images from GOES-18/GOES-West (above) and GOES-19/GOES-East (below) revealed the shadow of a total solar eclipse on 12 August 2026 — which began by moving eastward across far northern Alaska and Arctic Canada, then curved southeast across Greenland, Iceland and far western Europe before fading from view with sunset over western Africa.

10-minute GOES-19 Near-Infrared “Vegetation” images, from 1500-1930 UTC on 12 August

A closer view of GOES-19 images (below) showed the solar eclipse shadow as it passed across eastern Greenland and then Iceland.

10-minute GOES-19 Near-Infrared “Vegetation” images, from 1730-1800 UTC on 12 August

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