This website works best with a newer web browser such as Chrome, Firefox, Safari or Microsoft Edge. Internet Explorer is not supported by this website.

South Sandwich Islands volcanic and orographic cloud signatures

Even though the South Sandwich Islands are near the limb of the GOES-16 (GOES-East) view, Near-Infrared “Cloud Particle Size” (2.24 µm) images (above) were able to display a long volcanic plume (brighter shades of white) originating from Mount Michael on Saunders Island during the daylight hours on 12 March 2020. In addition, smaller/shorter volcanic... Read More

GOES-16 Near-Infrared

GOES-16 Near-Infrared “Cloud Particle Size” (2.24 µm) images [click to play animation | MP4]

Even though the South Sandwich Islands are near the limb of the GOES-16 (GOES-East) view, Near-Infrared “Cloud Particle Size” (2.24 µm) images (above) were able to display a long volcanic plume (brighter shades of white) originating from Mount Michael on Saunders Island during the daylight hours on 12 March 2020. In addition, smaller/shorter volcanic plumes could also be seen originating from a few of the smaller islands just to the north of Saunders Island. The volcanic plumes were more reflective (brighter white) because they were comprised of smaller droplets compared to the expansive stratus/stratocumulus clouds over the South Atlantic Ocean.

The smaller cloud particles of the volcanic plume were also more efficient reflectors of incoming solar radiation, thus appearing warmer (darker shades of gray) in GOES-16 Shortwave Infrared (3.9 µm) images (below).

GOES-16 Shortwave Infrared (3.9 µm) images [click to play animation | MP4]

GOES-16 Shortwave Infrared (3.9 µm) images [click to play animation | MP4]

2 days later, southerly/southwesterly winds interacting with the rugged terrain of the islands created von Kármán vortex streets downwind (north-northeast) of some of the islands (especially Montagu Island, the largest of the South Sandwich chain) — VIIRS True Color Red-Green-Blue (RGB) images from NOAA-20 and Suomi NPP  as visualized using RealEarth (below) provided a detailed view of these vortices.

VIIRS True Color RGB images from NOAA-20 and Suomi NPP [click to enlarge]

VIIRS True Color RGB images from NOAA-20 and Suomi NPP [click to enlarge]

In spite of the lower spatial resolution and large satellite viewing angle, the von Karman vortices could also be seen in GOES-16 “Red” Visible (0.64 µm) images (below).

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

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

 

View only this post Read Less

Wildfire in the Oklahoma Panhandle

1-minute Mesoscale Domain Sector GOES-16 (GOES-East) “Red” Visible (0.64 µm) and Shortwave Infrared (3.9 µm) images along with 5-minute Fire Power and Fire Temperature products (which are components of the GOES Fire Detection and Characterization Algorithm (SHyMet | ATBD) showed the rapid northeastward run (as fast as 103 feet per minute) of the 13,000 acre “Beaver Fire” (also known as the... Read More

GOES-16

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

1-minute Mesoscale Domain Sector GOES-16 (GOES-East) “Red” Visible (0.64 µm) and Shortwave Infrared (3.9 µm) images along with 5-minute Fire Power and Fire Temperature products (which are components of the GOES Fire Detection and Characterization Algorithm (SHyMet | ATBD) showed the rapid northeastward run (as fast as 103 feet per minute) of the 13,000 acre “Beaver Fire” (also known as the “412 Fire”) in the Oklahoma Panhandle on 07 March 2020. An elevated thermal signature on Shortwave Infrared imagery first began to appear southwest of Beaver, OK around 1546 UTC  — and 3.9 µm infrared brightness temperatures eventually peaked around 139ºC. Maximum Fire Power and Fire Temperature values exceeded 3100 MW and 2900 K, respectively. Fire Warnings were issued, with residents of Beaver and Forgan being advised to evacuate as the fire rapidly approached. In Visible imagery, the dark signature of a long, narrow vegetation burn scar was evident — and pyrocumulus clouds were seen developing over the fire.


Extreme fire behavior was aided by anomalously-strong winds across the southern Plains. The peak wind gust at Beaver, Oklahoma was 46 mph; south of the fire, surface winds were gusting to 43 mph at Perryton (in far the northern Texas Panhandle), and west of the fire winds gusted to 42 mph at Guymon (in the Oklahoma Panhandle). A large-scale animation of 1-minute GOES-16 Visible images from the AOS site (below) indicated that the smoke plume was transported northeastward across Kansas and eventually moved over south-central Nebraska. Smoke reduced the surface visibility to 6 miles at Dodge City as it moved across southwestern Kansas.

GOES-16

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

Shortwave Infrared images from MODIS (3.7 µm) and VIIRS (3.74 µm) (below) displayed three snapshots of the 10-15 mile long thermal anomaly (elongated cluster of black pixels) associated with the wildfire.

Shortwave Infrared images from MODIS (3.7 µm) and VIIRS (3.74 µm) [click to enlarge]

Shortwave Infrared images from MODIS (3.7 µm) and VIIRS (3.74 µm) [click to enlarge]

===== 08 March Update =====

NOAA-20 VIIRS Day/Night Band (0.7 µm) and Shortwave Infrared (3.74 µm) images at 0857 UTC [click to enlarge]

NOAA-20 VIIRS Day/Night Band (0.7 µm) and Shortwave Infrared (3.74 µm) images at 0857 UTC [click to enlarge]

During the subsequent overnight hours, a comparison of NOAA-20 VIIRS Day/Night Band (0.7 µm) and Shortwave Infrared (3.74 µm) images at 0857 UTC or 3:57 am local time (above) revealed the dark southwest-to-northeast oriented burn scar, with isolated small fires still burning along the northwestern periphery of the burn scar. Note: the NOAA-20 images are incorrectly labelled as Suomi NPP.

===== 09 March Update =====

GOES-16 Land Surface Temperature product and

GOES-16 Land Surface Temperature product and “Red” Visible (0.64 µm) image [click to enlarge]

A toggle between a GOES-16 Land Surface Temperature product and the corresponding Visible image (above) showed the fire burn scar at 2101 UTC on 09 March. Land Surface Temperature values were 10ºF warmer within the burn scar (middle 80s F, shades of yellow to orange) compared to areas immediately adjacent to the burn feature.

View only this post Read Less

Rapidly intensifying storm in the North Pacific Ocean

GOES-17 (GOES-West) Mid-level Water Vapor (6.9 µm) and Air Mass RGB images (above) depicted a rapidly intensifying Storm Force low (surface analyses) moving from the North Pacific Ocean toward the Alaska Panhandle on 04 March 2020. A comparison of GOES-17 Mid-level Water Vapor and Air Mass RGB images with NAM40 PV1.5 pressure (below) showed... Read More

GOES-17 Mid-level (6.9 µm) and Air Mass RGB images [click to play animation | MP4]

GOES-17 Mid-level Water Vapor (6.9 µm) and Air Mass RGB images [click to play animation | MP4]

GOES-17 (GOES-West) Mid-level Water Vapor (6.9 µm) and Air Mass RGB images (above) depicted a rapidly intensifying Storm Force low (surface analyses) moving from the North Pacific Ocean toward the Alaska Panhandle on 04 March 2020. A comparison of GOES-17 Mid-level Water Vapor and Air Mass RGB images with NAM40 PV1.5 pressure (below) showed that the Dynamic Tropopause — taken to be the pressure of the Potential Vorticity 1.5 surface — had descended to the 650 hPa pressure level in the vicinity of the low at 1200 UTC. The deeper red hues on Air Mass RGB imagery also indicated the presence of ozone-rich stratospheric air within the atmospheric column as the tropopause lowered in the vicinity of the rapidly-deepening low pressure.

GOES-17 Mid-level (6.9 µm) and Air Mass RGB images, with NAM40 PV1.5 pressure [click to enlarge]

GOES-17 Mid-level Water Vapor (6.9 µm) and Air Mass RGB images, with NAM40 PV1.5 pressure [click to enlarge]

1-minute Mesoscale Domain Sector GOES-17 “Red” Visible (0.64 µm) images (below) revealed mesovortices within the core of the large low pressure system.

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

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

===== 05 March Update =====

GOES-17

GOES-17 “Clean” Infrared Window (10.35 µm) mages [click to play animation | MP4]

On the following day, GOES-17 “Clean” Infrared Window (10.35 µm) mages (above) showed clouds associated with the Storm Force low as it moved slowly northward near the coast of the Alaska Panhandle (surface analyses). The storm prompted a wide variety of advisories, including a High Wind Warning for the Juneau area and a Blizzard Warning for the Skagway area.


GOES-17 True Color Red-Green-Blue (RGB) images created using Geo2Grid (below) revealed several plumes of airborne glacial silt drifting over the Gulf of Alaska, lofted by a strong offshore gap winds. A ship near Prince William Sound reported blowing dust at 18 UTC. Also seen in the images was the northwestward drift of ice into Cook Inlet and Turnagain Arm as high tide approached.

GOES-17 True Color RGB images [click to play animation | MP4]

GOES-17 True Color RGB images [click to play animation | MP4]

View only this post Read Less

GOES-17 IFR Probability Fields are now available via LDM Feed

When GOES-15 stopped sending data, IFR Probability fields based on GOES-15 ceased being sent over LDM to users. CIMSS is now sending GOES-17 IFR Probability fields (shown in a toggle above with the Night Fog Brightness Temperature Difference field) via the EXP LDM feed from CIMSS.  Particular strengths of IFR Probability fields include giving a useful low cloud signal below... Read More

GOES-17 IFR Probability Fields and Night Fog Brightness Temperature Difference (10.3 µm – 3.9 µm) fields, 1311 UTC on 3 March 2020 (Click to enlarge)

When GOES-15 stopped sending data, IFR Probability fields based on GOES-15 ceased being sent over LDM to users. CIMSS is now sending GOES-17 IFR Probability fields (shown in a toggle above with the Night Fog Brightness Temperature Difference field) via the EXP LDM feed from CIMSS.  Particular strengths of IFR Probability fields include giving a useful low cloud signal below high clouds (as over the western Olympic Peninsula in Washington) and differentiating between elevated stratus and fog, as in the northern Willamette Valley in Oregon.

Note that the Brightness Temperature Difference field shows artifacts related to GOES-17’s poorly-functioning Loop Heat Pipe.  Those artifacts are rapidly diminish day-to-day in early March as GOES-17 enters eclipse season.  Blog posts that discuss GOES-17 IFR Probability are available <a href=”https://fusedfog.ssec.wisc.edu/?cat=36″>here</a>.

View only this post Read Less