Mesoscale Convective System in Argentina

November 13th, 2018 |

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images, with GLM Groups plotted in cyan/green [click to play MP4 animation]

In support of the RELAMPAGO-CACTI field experiment, GOES-16 (GOES-East) had a Mesoscale Domain Sector centered over northeastern Argentina on 13 November 2018 — and 1-minute “Clean” Infrared Window (10.3 µm) images with plots of GLM Groups (above) showed a large and long-lived Mesoscale Convective System moving eastward across far northeastern Argentina and expanding into southern Paraguay and southeastern Brazil. Note the large amount of lightning in the anvil region far southeast of the core of the convection.

The corresponding GOES-16 Infrared animation without lightning data is shown below. Minimum cloud-top infrared brightness temperatures often reached -90ºC and colder (yellow pixels embedded within darker violet regions).

GOES-16 "Clean" Infrared Window (10.3 µm) images [click to play MP4 animation]

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

A comparison of NOAA-20 VIIRS True Color Red-Green-Blue (RGB) and Infrared Window (11.45 µm) images using RealEarth (below) provided a very detailed view of the MCS at 1703 UTC. On the Infrared image, storm-top signatures often associated with severe thunderstorms included a well-defined enhanced-V (with a pronounced cold/warm couplet) situated over the Paraguay/Argentina border, and a “warm trench” surrounding the cold overshooting top at the vertex of the enhanced-V over extreme southern Paraguay.

NOAA-20 VIIRS True Color Red-Green-Blue (RGB) and Infrared Window (11.45 µm) images at 1703 UTC [click to enlarge]

NOAA-20 VIIRS True Color Red-Green-Blue (RGB) and Infrared Window (11.45 µm) images at 1703 UTC [click to enlarge]

The warm trench signature was also evident on 2-km resolution GOES-16 Infrared imagery at that same time (below), just west of Posadas, Argentina SARP. However, the warm trench surrounding the small overshooting top was only apparent from 1700 to 1705 UTC — so it was remarkable timing to have an overpass of the NOAA-20 satellite capture the brief signature in greater detail (at 375-meter resolution). A similar short-lived small overshooting top was seen at the vertex of the enhanced-V signature for the 6-minute period centered at 1652 UTC.

GOES-16 "Clean" Infrared Window (10.3 µm) image at 1703 UTC, with and without GLM Groups plotted in cyan/green [click to enlarge]

GOES-16 “Clean” Infrared Window (10.3 µm) image at 1703 UTC, with and without GLM Groups plotted in cyan/green [click to enlarge]

Category 4 Hurricane Michael makes landfall along the Florida coast

October 10th, 2018 |

Sequence of Infrared Window images from Terra/Aqua MODIS (11.0 µm) and Suomi NPP VIIRS (11.45 µm) [click to enlarge]

Infrared Window images from Terra/Aqua MODIS (11.0 µm) and NOAA-20/Suomi NPP VIIRS (11.45 µm) [click to enlarge]

A sequence of Infrared Window images from Terra/Aqua MODIS (11.0 µm) and NOAA-20/Suomi NPP VIIRS (11.45 µm) (above) showed Category 4 Hurricane Michael as it was making its approach toward the Florida coast during the nighttime hours preceding sunrise on 10 October 2018. The yellow pixels east of the eye on the 0724 UTC VIIRS image highlighted cloud-top infrared brightness temperatures of -90ºC and colder (with a minimum of -92ºC).

Toggles between VIIRS Day/Night Band (0.7 µm) and Infrared Window (11.45 µm) images from NOAA-20 and Suomi NPP (below; courtesy of William Straka, CIMSS) revealed convectively-generated mesospheric airglow waves propagating away from the hurricane.

NOAA-20 VIIRS Day/Night Band (0.7 µm) and Infrared Window (11.45 µm) images [click to enlarge]

NOAA-20 VIIRS Day/Night Band (0.7 µm) and Infrared Window (11.45 µm) images [click to enlarge]

Suomi NPP VIIRS Day/Night Band (0.7 µm) and Infrared Window (11.45 µm) images [click to enlarge]

Suomi NPP VIIRS Day/Night Band (0.7 µm) and Infrared Window (11.45 µm) images [click to enlarge]

Overlapping GOES-16 (GOES-East) Mesoscale Domain Sectors provided 30-second interval  “Clean” Infrared Window (10.3 µm) and “Red” Visible (0.64 µm) images of Michael after sunrise (below).

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

GOES-16 "Red" Visible (0.64 µm) images [click to play MP4 animation]

GOES-16 “Red” Visible (0.64 µm) images [click to play MP4 animation]

Closer views of GOES-16 Visible and Infrared images (below) showed Hurricane Michael making landfall around 1730-1745 UTC near Mexico Beach, Florida as a high-end Category 4 storm with maximum sustained winds of 135 knots (155 mph) and a minimum central pressure of 919 hPa (27.41 inches). During the 24-hour period prior to landfall, Michael had been moving over water having moderate Ocean Heat Content and warm Sea Surface Temperatures; and as had been the case during much of Michael’s time as a hurricane, in spite of the fact that deep-layer wind shear was somewhat unfavorable (09 October | 10 October landfall), the storm was still able to maintain a trend of intensification (ADT | SATCON). Additional information regarding the landfall of Michael (and its historical significance) is available here.

GOES-16 "Red" Visible (0.64 µm) images [click to play MP4 animation]

GOES-16 “Red” Visible (0.64 µm) images [click to play MP4 animation]

GOES-16 "Clean" Infrared Window (10.3 µm) images [click to play MP4 animation]

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

GOES-16 Geostationary Lightning Mapper (GLM) Groups — aggregates of individual lightning Events — are plotted on 30-second GOES-16 Visible images (below). The red symbols denote lightning Groups within the 1-minute period immediately preceding the Visible image time, with the yellow symbols being Groups for the 1-minute time period before that. The native GLM parallax correction is turned off — so the lightning locations correspond to where the satellite viewed the lightning signatures at the tops of the clouds.

GOES-16

GOES-16 “Red” Visible (0.64 µm) images, with GLM lightning Groups plotted in red and yellow [click to play MP4 animation]

As pointed out on Twitter by the SOO at NWS Nashville, GOES-16 Visible imagery (below) revealed the bright white sandy beaches of Saint Andrew Sound (Google Maps) as the eye of Michael passed overhead. Surface observations from Panama City (KECP), Tyndall AFB (KPAM) and Apalachicola (KAAF) are plotted on the images — all 3 sites stopped reporting after landfall, presumably due to power outages (the peak wind gust at Tyndall AFB was 129 mph). A longer animation (from 1300-1959 UTC) of 30-second GOES-16 Visible images is available here (courtesy of Pete Pokrandt, UW-AOS).

GOES-16

GOES-16 “Red” Visible (0.64 µm) images, with surface observations and with/without a map overlay [click to play animation | MP4]

The signature of the beaches was also evident on GOES-17 Visible imagery (below) —  but since that satellite was scanning at the standard 5-minute interval, they were only seen on 2 consecutive images. Note that GOES-17 imagery shown here  is preliminary and non-operational.

GOES-17 "Red" Visible (0.64 µm) images, with surface observations and with/without a map overlay [click to enlarge]

GOES-17 “Red” Visible (0.64 µm) images, with surface observations and with/without a map overlay [click to enlarge]

One item of local curiosity that was observed on GOES-16 Visible imagery: a darker shadow-like feature within the eye, which slowly migrated from the northern to the western portion during the 1613-1642 UTC period (1625 UTC still image | MP4 animation). Closer inspection of the GOES-16 ABI Near-Infrared and Infrared spectral bands (below) indicated that this was indeed a cloud shadow, from a cirrus filament that became detached from the southeastern edge of the eyewall and then rotated cyclonically within the eye to cast a shadow against the brightly-illuminated quasi-vertical edges of the eyewall.

16-panel images of all GOES-16 ABI spectral bands [click to play animation | MP4]

All 16 spectral bands of the GOES-16 ABI [click to play animation | MP4]

A sequence of Infrared Window images from Aqua MODIS (11.0 µm) and NOAA-20/Suomi NPP VIIRS (11.45 µm) (below) provided a high-resolution view of the cold cloud tops associated with Michael during and shortly after landfall.

Infrared Window images from Aqua MODIS (11.0 µm) and NOAA-20/Suomi NPP VIIRS (11.45 µm) [click to enlarge]

Infrared Window images from Aqua MODIS (11.0 µm) and NOAA-20/Suomi NPP VIIRS (11.45 µm) [click to enlarge]

On a larger scale, GOES-16 mid/upper-level Derived Motion Winds from the CIMSS Tropical Cyclones site (below) revealed the development of a well-defined outflow channel to the north of the storm, especially during the 12 hours prior to landfall — this enhanced poleward outflow (aided by the approach of an upper-level trough from the central US) may have been a contributing factor in Michael’s continued intensification leading up to landfall.

GOES-16 Mid/Upper-level winds, 21 UTC on 09 October to 21 UTC on 10 October [click to enlarge]

GOES-16 Mid-level (6.9 µm) Water Vapor images with Mid/Upper-level winds, from 21 UTC on 09 October to 21 UTC on 10 October [click to enlarge]

Aqua MODIS Near-Infrared “Cirrus” (1.37 µm) and Water Vapor (6.7 µm) images (below) showed that clouds and moisture were being transported by this outflow channel as far northward as the Ohio River Valley shortly after the time of landfall.

Aqua MODIS Near-Infrared

Aqua MODIS Near-Infrared “Cirrus” (1.37 µm) and Water Vapor (6.7 µm) images [click to enlarge]

A GOES-16 Red-Green-Blue (RGB) animation (below; courtesy of Rick Kohrs, SSEC) showed the landfall of Michael.

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

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

A stereoscopic animation using GOES-16 and GOES-17 Visible imagery is provided below; to view the animation in 3-D, cross your eyes until 3 images appear — then focus on the image in the middle. Note that GOES-17 images shown here are preliminary and non-operational.

“Red” Visible (0.64 µm) images from GOES-16 (left) and GOES-17 (right) [click to play animation]

===== 11 October Update =====

Aqua MODIS True Color RGB images from 06 October and 11 October [click to enlarge]

Aqua MODIS True Color RGB images from 06 October and 11 October [click to enlarge]

A before/after comparison of Aqua MODIS True Color RGB images (source) from 06 October and 11 October (above) showed a dramatic increase in turbidity of the water off the “Emerald Coast” portion of the Florida Panhandle — this turbidity was the result of turbulent mixing of the relatively shallow continental shelf water by the strong winds of the hurricane. The close-up images above are centered off the coast near the landfall location; the large-scale images below show more of the Gulf Coast, from Texas to the Florida Peninsula.

Aqua MODIS True Color RGB images from 06 October and 11 October [click to enlarge]

Aqua MODIS True Color RGB images from 06 October and 11 October [click to enlarge]

Hourly images of the MIMIC Total Precipitable Water product during the 5-day period from 07-11 October (below) showed the transport of tropical moisture from the Caribbean Sea across the Gulf of Mexico and over the southeastern US — heavy rainfall and flooding occurred from Florida and Alabama to the Mid-Atlantic states (WPC summary).

MIMIC Total Precipitable Water images, 07-11 October [click to play animation | MP4]

MIMIC Total Precipitable Water images, 07-11 October [click to play animation | MP4]

The entire life cycle of Michael can be viewed in a compilation of GOES-16 Infrared 1-minute (or 30-second, when available) Mesoscale Sector images from 07-11 October, available here  — with a zoomed-in version of the images from 08-11 October available here or on YouTube (courtesy of Pete Pokandt, UW-AOS).

===== 18 October Update =====

Terra MODIS True Color RGB images from 04 October and 18 October [click to enlarge]

Terra MODIS True Color RGB images from 04 October and 18 October [click to enlarge]

A comparison of before/after Terra MODIS True Color RGB images from 04 October and 18 October (above) revealed a broad swath of damaged/dead vegetation (lighter shades of brown) along the path of strongest winds associated with the eyewall of Hurricane Michael.

Larger-scale versions of those same before/after Terra MODIS True Color RGB images from the SSEC MODIS Direct Broadcast site (below) showed that the path of damaged vegetation extended far northeastward across Georgia — Michael was still at Category 3 intensity when its center moved into the southwestern corner of the state.

Terra MODIS True Color RGB images from 04 October and 18 October [click to enlarge]

Terra MODIS True Color RGB images from 04 October and 18 October [click to enlarge]

A before/after comparison of Terra MODIS False Color RGB images (using Bands 7-2-1) from 04 October and 12 October (below) showed the area rivers that were in varying stages of flooding (darker shades of blue) following the heavy rainfall from Michael (the total precipitation was 8 inches above normal or 600% of normal for the 14-day period of 04-18 October). Most obvious was the Chipola River, which was at Moderate flood stage on 14 October.

Terra MODIS False Color RGB images from 04 October and 12 October [click to enlarge]

Terra MODIS False Color RGB images from 04 October and 12 October [click to enlarge]

Hurricane Florence

September 9th, 2018 |

GOES-16

GOES-16 “Red” Visible (0.64 µm) iimages [click to play MP4 animation]

After previously weakening from a Category 4 hurricane (on 04 September) to a tropical storm on 07 September (track/intensity), Florence re-intensified to become a Category 1 hurricane at 15 UTC on 09 September 2018. 1-minute Mesoscale Domain Sector GOES-16 (GOES-East) “Red” Visible (0.63 µm) are shown above, with the corresponding “Clean” Infrared Window (10.3 µm) images shown below. An eye structure appeared for brief intervals during the day, but was often masked by cloud debris from a series of convective bursts within the surrounding eyewall.

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

GPM GMI Microwave (85 GHz) image at 1811 UTC [click to enlarge]

GPM GMI Microwave (85 GHz) image at 1811 UTC [click to enlarge]

GPM GMI (above) and DMSP-16 SSMIS (below) Microwave (85 GHz) images from the CIMSS Tropical Cyclones site revealed that the eye was still partially open at 1811 UTC and 1945 UTC.

DMSP-16 SSMIS Microwave (85 GHz) image at 1845 UTC [click to enlarge]

DMSP-16 SSMIS Microwave (85 GHz) image at 1845 UTC [click to enlarge]

===== 10 September Update =====

GOES-16

GOES-16 “Red” Visible (0.64 µm) images, with GLM Group lightning [click to enlarge]

GOES-16 GLM lightning Groups (aggregates of GLM lightning Events) are plotted on “Red” Visible (0.64 µm) images (above) and “Clean” Infrared Window (10.3 µm) images (below), courtesy of Dave Santek, SSEC.

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images, with GLM Group lightning [click to enlarge]

Overlapping GOES-16 and GOES-17 Mesoscale Domain Sectors were positioned over Hurricane Florence beginning at 1200 UTC (providing imagery at 30-second intervals) — Visible animations are shown below.

* GOES-17 images shown here are preliminary and non-operational *

GOES-16

GOES-16 “Red” Visible (0.64 µm) images [click to play MP4 animation]

GOES-17

GOES-17 “Red” Visible (0.64 µm) images [click to play MP4 animation]

Longer animations of 30-second GOES-16 Visible and Infrared images viewed using AWIPS (below) provided a better view of  the mesovortices within the eye. Florence rapidly intensified (ADT | SATCON) to a Category 4 hurricane during this period.

GOES-16

GOES-16 “Red” Visible (0.64 µm) images [click to play MP4 animation]

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

One particularly large mesovortex rotated around the eastern edge of the eye after 2100 UTC, significantly eroding the eyewall (below).

GOES-16

GOES-16 “Red” Visible (0.64 µm) images [click to play MP4 animation]

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

Later in the early evening hours, GOES-16 Infrared imagery (below) showed an area of pronounced cloud-top warming and a thinning of cloud material just south of the eyewall, as Florence began to undergo an eyewall replacement cycle.

GOES-16

GOES-16 “Clean” Infrared Window (10.3 µm) images [click to play MP4 animation]

Cranston Fire pyrocumulonimbus

July 25th, 2018 |

GOES-16

GOES-16 “Red” Visible (0.64 µm, left) and Shortwave Infrared (3.9 µm, right) images, with hourly plots of surface reports [click to play animation | MP4]

GOES-16 (GOES-East) “Red” Visible (0.64 µm) and Shortwave Infrared (3.9 µm) images (above) showed the smoke and pyrocumulus clouds as well as the thermal anomaly or “hot spot” (red pixels) associated with the Cranston Fire — located in the center of the images — which started southwest of Palm Springs, California (KPSP) around 1852 UTC or 11:52 am PDT on 25 July 2018. The large areas of red seen on the Shortwave Infrared images early in the animation were signatures of very hot sandy soil surfaces of the southern California deserts. Note the very warm air temperatures seen across the region; Palm Springs had an afternoon high of 116ºF, and Thermal KTRM had a high of 119ºF (farther inland, Death Valley had a high of 127ºF).

A slightly different view — with the fire located in the lower left corner, southwest of KPSP — using GOES-16 “Red” Visible (0.64 µm), Shortwave Infrared (3.9 µm) and “Clean” Infrared Window (10.3 µm) images (below) revealed that the fire actually produced 3 distinct pulses of pyroCumulonimbus (pyroCb) cloud, where the 10.3 µm cloud-top infrared brightness temperature reached or exceeded the -40ºC threshold (lime green enhancement). Three specific times that these separate pyroCb clouds were evident were 2102 UTC, 2147 UTC and 2312 UTC.

GOES-16 "Red" Visible (0.64 µm, left), Shortwave Infrared (3.9 µm, center) and "Clean" Infrared Window (10.3) images, with 4-letter airport identifiers plotted in yellow [click to play animation | MP4]

GOES-16 “Red” Visible (0.64 µm, left), Shortwave Infrared (3.9 µm, center) and “Clean” Infrared Window (10.3 µm, right) images, with 4-letter airport identifiers plotted in yellow [click to play animation | MP4]

Another view of the pyroCb pulses was provided by a 4-panel view of GOES-16 “Red” Visible (0.64 µm), Shortwave Infrared (3.9 µm), “Clean” Infrared Window (10.3 µm) and Cloud Top Phase (below). The coldest 10.3 µm cloud-top infrared brightness temperatures were -55ºC as the primary pyroCb anvil drifted northeastward toward the California/Nevada border.

GOES-16 "Red" Visible (0.64 µm, top left), Shortwave Infrared (3.9 µm, top right), "Clean" Infrared Window (10.3 µm, bottom left) and Cloud Top Phase (bottom right) images [click to play animation | MP4]

GOES-16 “Red” Visible (0.64 µm, top left), Shortwave Infrared (3.9 µm, top right), “Clean” Infrared Window (10.3 µm, bottom left) and Cloud Top Phase (bottom right) images [click to play animation | MP4]

There was also substantial lightning observed with these pyroCb clouds:


Below is a timelapse video of the first 8 hours of the fire, which shows the pyroCb evolution at the end.

Timelapse of Cranston Fire [click to play YouTube video]

Timelapse of Cranston Fire [click to play YouTube video]

===== 26 July Update =====

GOES-16 "Red" Visible (0.64 µm, top left), Shortwave Infrared (3.9 µm, top right), "Clean" Infrared Window (10.3 µm, bottom left) and Fire Temperature (bottom right) images [click to play animation | MP4]

GOES-16 “Red” Visible (0.64 µm, top left), Shortwave Infrared (3.9 µm, top right), “Clean” Infrared Window (10.3 µm, bottom left) and Fire Temperature (bottom right) images [click to play animation | MP4]

Another pyroCb was produced by the Cranston Fire on 26 July, as shown by GOES-16 “Red” Visible (0.64 µm), Shortwave Infrared (3.9 µm), “Clean” Infrared Window (10.3 µm) and Fire Temperature images (above). Similar to the previous day, there appeared to be 2 pulses of pyroCb formation — with cloud-top infrared brightness temperatures cooling to -44ºC. Pyrocumulus from the smaller Ribbon Fire (just southeast of the Cranston Fire) could also be seen.