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Shower initiation over Wisconsin

Showers developed over southern Wisconsin late in the day on 12 June 2020. What satellite products could be used to anticipate where the showers would develop? The animation of visible and radar, above, shows that the storms initiated near a boundary (mostly stationary) that separated Lake Michigan-influenced air with less... Read More

GOES-16 ABI Band 2 (0.64 ) visible imagery (left) and Midwest Composite Radar (right), 1736 – 2100 UTC on 13 June 2020 (Click to animate)

Showers developed over southern Wisconsin late in the day on 12 June 2020. What satellite products could be used to anticipate where the showers would develop? The animation of visible and radar, above, shows that the storms initiated near a boundary (mostly stationary) that separated Lake Michigan-influenced air with less stable air (based on cumuliform cloud development) to the south and west. Showers develop near the lake breeze front starting around 2000 UTC; a parallax shift is obvious between the radar and satellite (2100 UTC example) A parallax correction on the satellite imagery would shift the cloud locations towards the sub-satellite point (0, 75.2 W for GOES-East).

NUCAPS (NOAA-Unique Combined Atmospheric Processing System) soundings combine infrared and microwave information from the high spectral resolution CrIS (Cross-track Infrared Sounder) and ATMS (Advanced Technology Microwave Sounder) instruments on NOAA-20 to yield estimates of the thermodynamic structure of the atmosphere. NOAA-20 overflew the western Great Lakes shortly after 1800 UTC on 12 June, and clear skies at the time means the infrared information was complete. (In cloudy skies, NUCAPS soundings are more typically driven by ATMS data, which has coarser spectral and horizontal resolution).

The Total Totals index shown below was derived from the NUCAPS thermodynamic information. A gradient in stability exists between the most unstable air in western Wisconsin and the more stable lake-influenced air over eastern Wisconsin.

Total Totals index derived from NOAA-20 NUCAPS data, 1840 UTC on 12 June 2020 (Click to enlarge)

The low-level lapse rate, below, (from 900-700 mb), also shows a gradient in stability in the region where shower development occurred. It is not unusual for shower initiation to occur in gradients of stability (Example 1, Example 2,…), so that is a region on which to focus when waiting for convection to start.

900-700 mb Lapse Rates derived from NOAA-20 NUCAPS data, 1840 UTC on 12 June 2020 (Click to enlarge)

Once the shower development occurs, when will lightning occur?  As noted in this blog post, the Day Cloud Phase Distinction Red-Green-Blue imagery that includes the 1.61 µm band (at which wavelength reflectance is greatly affected by the presence of ice) gives a visual clue to when glaciation occurs, and cloud-top glaciation commonly precedes lightning development.  The animation below shows the Day Cloud Phase Distinction on the left, and the Day Cloud Phase Distinction overlain with Geostationary Lightning Mapper (GLM) Flash Extent Density.

There are only two detected lightning flashes in this animation — and in both cases, the Day Cloud Phase Distinction has become more orange/yellow and less green/blue before the lightning strike. This color change occurs as the 1.61 µm imagery becomes darker: ice in the cloud top increases the absorption (and reduces the reflectance) of 1.61 µm solar energy. Compare the 2111, 2116 and 2121 imagery for the lightning strike near Madison in Dane County; Similarly, compare the 2051, 2056, 2101 and 2106 imagery for the 2101 UTC lightning strike in Waukesha county). There are subtle color changes (on other days the changes are more obvious!) in the Day Cloud Phase Distinction RGB that preceded lightning events.

GOES-16 Day Cloud Phase Distinction (left), and Day Cloud Phase Distinction overlain with Geostationary Lightning Mapper (GLM) data (Click to animate)


GOES-16 Level 2 Products include Derived Stability Products (these can be found online here as well), and the mostly clear skies on 12 June meant a good signal.  The Baseline Lifted Index, shown below from 1701 through 2256 UTC,  shows convection developing along the eastern edge of less stable air.

GOES-16 Derived Stability Index (Lifted Index) in clear regions, GOES-16 ABI Band 13 (10.3 µm) infrared imagery in cloud regions, 1701-2256 UTC on 12 June 2020 (Click to animate)

Is there an easily identifiable trigger that spawned these storms? Water Vapor imagery often shows impulses in clear skies. The two RGB products below combine different water vapor channels.  There is a subtle increase in the amount of orange in the Differential Water Vapor before the convection starts.  This increase in the red component is an increase in the brightness temperature difference between upper and lower water vapor channels, a difference that can be associated with upper-tropospheric forcing.  The simple water vapor RGB (that includes the upper and lower water vapor channels, but not the difference between them) on the right shows no obvious signal.

GOES-16 Differential Water Vapor RGB (left) and SImple Water Vapor RGB (right) from 0916 to 2116 UTC on 12 June 2020 (Click to animate).

The Air Mass RGB (described here) also has the split water vapor difference as its red component. The animation below (from this site), shows a subtle change in air mass (cooler, dryer air moving southward from Canada) that could have provided an additional triggering mechanism for the convection.

GOES-16 Air Mass RGB, 1541 to 2141 UTC on 12 June 2020 (Click to enlarge)


Webcams in Madison, WI, that capture the evolution of these storms, and also show the GOES-16 imagery (derived from this site), are available at this tweet from @GOESGuy.

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Mount St. Helens: June 1980

SMS-2The main Mount St. Helens eruption was May 18, 1980 — yet there were also later paroxysmal eruptions. Imagery from NASA’s SMS-2 (Synchronous Meteorological Satellite) monitored two more Mount St. Helens eruptions on June 12th (local time), 1980, as shown above. Note that in “UTC-time”, the eruption took place on June 13th. A... Read More

SMS-2

Vis and IR

Visible and Infrared NASA SMS-2 animation on June 13, 1980 between 02:30 and 07:00 UTC. The red square denotes the  approximate location of Mount St. Helens, and the arrows highlight the plumes of the two separate eruptions.  [Click to play mp4]

The main Mount St. Helens eruption was May 18, 1980 — yet there were also later paroxysmal eruptions. Imagery from NASA’s SMS-2 (Synchronous Meteorological Satellite) monitored two more Mount St. Helens eruptions on June 12th (local time), 1980, as shown above. Note that in “UTC-time”, the eruption took place on June 13th. A similar side-by-side SMS-2 visible and infrared animation (without the arrows) is available here (in addition to one without the red location box).

SMS-2 Visible image

NASA SMS-2 visible animation from June 13th (02:00 to 04:00 UTC), 1980. The red square denotes the  approximate location of Mount St. Helens. [Click to play mp4]

A visible band animation without the red square at the location of Mount St. Helens is shown above. The second plume coated Portland (OR) with ash. For more on this case, see Wikipedia and the USGS. Here’s the same loop and image, but without the red location box.

The volcanic ash plume was also evident in the infrared window band, below, but the imagery has fairly coarse spatial (and temporal) resolution compared to today’s GOES-R series ABI (which allows much improved volcanic cloud monitoring). This longer IR loop shows the 2nd plume as well.

IR image

NASA SMS-2 infrared animation from June 13th (02:45 to 04:00 UTC), 1980. The red square denotes the  approximate location of Mount St. Helens. [Click to play mp4]

Swipe between SMS-2 Visible and Infrared bands. Red square notes Mount St. Helens location.

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Fade between a SMS-2 Visible and Infrared band.

Note that there is a geolocation offset between the two spectral bands. The satellite times listed are the image scan start times.

GOES-3

The experimental SMS series followed the ATS series, and was a precursor to the operational GOES.

GOES -3 also observed both volcanic ash plumes.

GOES-3 IR

GOES-3 Infrared animation from June 13, 1980. [Click to play mp4]

A slightly longer GOES-3 infrared animation is available here. NASA SMS-2 and NOAA GOES-3 data are via the University of Wisconsin-Madison SSEC Satellite Data Services.

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Pyrocumlonimbus cloud spawned by the Bringham Fire in Arizona

1-minute Mesoscale Domain Sector GOES-17 (GOES-West) “Red” Visible (0.64 µm), Shortwave Infrared (3.9 µm) and “Clean” Infrared Window (10.35 µm) images (above) showed the formation of a pyrocumulonimbus (pyroCb) cloud that was spawned by the Bringham Fire in extreme eastern Arizona during the afternoon hours on 11 June 2020. To be classified as a pyroCb, the deep convective... Read More

GOES-17 “Red” Visible (0.64 µm, top), Shortwave Infrared (3.9 µm, center) and “Clean” Infrared Window (10.35 µm, bottom) images, with hourly plots of surface reports [click to play animation | MP4]

GOES-17 “Red” Visible (0.64 µm, top), Shortwave Infrared (3.9 µm, center) and “Clean” Infrared Window (10.35 µm, bottom) images, with hourly plots of surface reports [click to play animation | MP4]

1-minute Mesoscale Domain Sector GOES-17 (GOES-West) “Red” Visible (0.64 µm), Shortwave Infrared (3.9 µm) and “Clean” Infrared Window (10.35 µm) images (above) showed the formation of a pyrocumulonimbus (pyroCb) cloud that was spawned by the Bringham Fire in extreme eastern Arizona during the afternoon hours on 11 June 2020. To be classified as a pyroCb, the deep convective cloud must be generated by a large/hot fire, and eventually exhibit cloud-top 10.35 µm infrared brightness temperatures of -40ºC and colder — assuring the heterogeneous nucleation of all supercooled water droplets to form ice crystals. The pyroCb cloud then moved northeastward across far western New Mexico.

In Shortwave Infrared imagery, the fire’s thermal anomaly or “hot spot” was depicted by the cluster of red pixels — and the pyroCb cloud tops  appear warmer (darker gray) than those of nearby conventional thunderstorms, due to enhanced reflection of solar radiation off the smaller ice crystals found in the pyroCb anvil (reference).

The pyroCb exhibited minimum cloud-top 10.35 µm infrared brightness temperature in the -40 to -49ºC range (shades of blue) — according to rawinsonde data from Tucson, Arizona at 00 UTC on 12 June (below), this roughly corresponded to altitudes of 10-12 km.

Plot of rawinsonde data from Tucson, Arizona [click to enlarge]

Plot of rawinsonde data from Tucson, Arizona [click to enlarge]

 

Suomi NPP VIIRS True Color RGB image, with plots of VIIRS Fire Radiative Power [click to enlarge]

Suomi NPP VIIRS True Color RGB image, with plots of VIIRS Fire Radiative Power [click to enlarge]

A Suomi NPP VIIRS True Color Red-Green-Blue (RGB) image viewed using RealEarth (above) included plots of VIIRS Fire Radiative Power. The hazy signature of smoke drifting northward was apparent in the image. In fact, a plot of surface observation data at Springerville, Arizona (KJTC) (below) indicated that surface visibility was eventually reduced to 7 miles around 23 UTC as strong southerly winds advected smoke northward from the fire.

Plot of surface observation data at Springerville, Arizona [click to enlarge]

Plot of surface observation data at Springerville, Arizona [click to enlarge]

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Blowing dust in the Plains

GOES-16 (GOES-East) Split Cloud Top Phase (11.2-8.4 µm) and Dust Red-Green-Blue (RGB) images (above) displayed signatures of blowing dust plumes — medium shades of blue in the 11.2-8.4 µm product, and brighter shades of magenta to pink in the Dust RGB — caused by strong winds in the wake of cold fronts moving... Read More

GOES-16 Split Cloud Top Phase (11.2-8.4 µm) and Dust RGB images (with and without plots of surface reports) [click to play animation | MP4]

GOES-16 Split Cloud Top Phase (11.2-8.4 µm) and Dust RGB images (with and without plots of surface reports) [click to play animation | MP4]

GOES-16 (GOES-East) Split Cloud Top Phase (11.2-8.4 µm) and Dust Red-Green-Blue (RGB) images (above) displayed signatures of blowing dust plumes — medium shades of blue in the 11.2-8.4 µm product, and brighter shades of magenta to pink in the Dust RGB — caused by strong winds in the wake of cold fronts moving southward and eastward  across the central and southern Plains on 09 June 2020.

A closer view of GOES-16 Dust RGB images over the Texas Panhandle (below) showed a localized pocket of dense blowing dust moving southeastward — it temporarily reduced visibility to 2 miles at Borger KBGD, moved across Interstate 40 east of Amarillo KAMA, and then reduced visibility to 3 miles at Childress KCDS.

GOES-16 Dust RGB images [click to play animation | MP4]

GOES-16 Dust RGB images [click to play animation | MP4]

On a larger scale, a longer animation of GOES-16 Dust RGB images created using Geo2Grid (below) showed the early stages of the initial southward surge of blowing dust over eastern Colorado, where wind gusts to 102 mph were recorded.

GOES-16 Dust RGB images [click to play animation | MP4]

GOES-16 Dust RGB images [click to play animation | MP4]

The corresponding daytime GOES-16 True Color RGB mages (below) showed the tan-colored plumes of blowing dust, in addition to a few smoke plumes (shades of white) from wildfires in Arizona, New Mexico and the Texas Panhandle.

GOES-16 True Color RGB images [click to play animation | MP4]

GOES-16 True Color RGB images [click to play animation | MP4]

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