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Thunderstorms over Arizona: turbulence, hail, and damaging winds

AWIPS images of MODIS 0.64 µm visible channel and 6.7 µm water vapor channel images with an overlay of CRAS model 500 hPa geopotential height contours (above) showed an upper-level trough of low pressure that was moving inland across southern California and Arizona on Read More

MODIS 0.65 µm visible channel and 6.7 µm water vapor channel images (with CRAS model 500 hPa geopotential height contours)

MODIS 0.65 µm visible channel and 6.7 µm water vapor channel images (with CRAS model 500 hPa geopotential height contours)

AWIPS images of MODIS 0.64 µm visible channel and 6.7 µm water vapor channel images with an overlay of CRAS model 500 hPa geopotential height contours (above) showed an upper-level trough of low pressure that was moving inland across southern California and Arizona on 08 March 2013.

Suomi NPP VIIRS 0.64 µm visible channel and 11.45 µm IR channel images (with surface reports and surface fronts)

Suomi NPP VIIRS 0.64 µm visible channel and 11.45 µm IR channel images (with surface reports and surface fronts)

A comparison of Suomi NPP VIIRS 0.64 µm visible channel and 11.45 µm IR channel images (above) showed that widespread thunderstorms had developed on either side of a cold frontal boundary that was moving eastward across Arizona. The Blended Total Precipitable Water (TPW) product (below) indicated that TPW values were as high as 20 mm or 0.79 inch over much of Arizona, which was in excess of 200% or normal for this time of the year. With unseasonably high moisture in place, these thunderstorms produced a daily record rainfall  of 0.84 inch at Phoenix, with several locations in the Phoenix area receiving over 1 inch of precipitation (Public Information Statement). Hail up to 0.5 inch in diameter was reported — in some cases the hail accumulated to the point of totally covering the ground — and winds gusted to 45-55 mph at several locations.

Blended Total Precipitable Water and Percent of Normal Total Precipitable Water products

Blended Total Precipitable Water and Percent of Normal Total Precipitable Water products

In addition to heavy rainfall, hail, and damaging surface winds, there were several pilot reports of turbulence. Particularly noteworthy were a pilot report of Severe turbulence at an altitude of 28,000 feet, and a pilot report of Severe to Extreme turbulence at an altitude of 11,000 feet. Both of these turbulence reports appeared to be associated with convective cells that were growing rapidly, as seen with GOES-13 10.7 µm IR channel images (below; click image to play animation).

GOES 15/13 10.7 µm IR channel images with pilot reports of turbulence (click image to play animation)

GOES 15/13 10.7 µm IR channel images with pilot reports of turbulence (click image to play animation)

 

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Volcanic ash fall plume over the Kamchatka Peninsula

AWIPS images of Suomi NPP VIIRS 0.64 µm visible channel images (above) revealed some interesting curved ice floe gyres in the Bering Sea just off the eastern coast of the Russian Kamchatka Peninsula on 07 March 2013. Also evident near the center of the visible images was a long, narrow,... Read More

Suomi NPP VIIRS 0.64 µm visible channel images

Suomi NPP VIIRS 0.64 µm visible channel images

AWIPS images of Suomi NPP VIIRS 0.64 µm visible channel images (above) revealed some interesting curved ice floe gyres in the Bering Sea just off the eastern coast of the Russian Kamchatka Peninsula on 07 March 2013. Also evident near the center of the visible images was a long, narrow, and slightly darker feature that was oriented approximately west-to-east, and located to the northwest and north of the village of Ust’-Kamchatsk (station identifier 32408). This darker feature was a volcanic ash fall plume from the Sheveluch Volcano (located 31 miles or 50 km to the northwest), which had experienced eruptions producing volcanic ash (photos) on 02 March and 04 March — the darker color of the narrow strip of volcanic ash made it stand out against the adjacent snow-covered areas (annotated visible image).

A comparison of a Suomi NPP VIIRS 0.64 µm visible channel image with the corresponding false-color Red/Green/Blue (RGB) image (below) also showed the contrast between the narrow strip of ash-covered snow and the surrounding undisturbed snow cover (snow and ice appear as darker shades of red in the RGB image).

Suomi NPP VIIRS 0.64 µm visible channel image + False-color Red/Green/Blue (RGB) image

Suomi NPP VIIRS 0.64 µm visible channel image + False-color Red/Green/Blue (RGB) image

A comparison of Suomi NPP VIIRS 0.64 µm visible channel, 3.74 µm shortwave IR channel, and 11.45 µm IR channel images (below) showed that the strip of ash-covered snow appeared significantly warmer (darker) on the shortwave IR image, due to the fact that the volcanic ash particles were efficient reflectors of incoming solar radiation. The ash-covered snow even appeared slightly warmer (darker) on the 11.45 µm IR image, since the lower albedo of the ash-covered snow allowed it to absorb more incoming solar radiation.Also evident on the shortwave IR image was a distinct hot thermal anomaly (yellow to red color enhancement) associated with the active Kizimen volcano.

Suomi NPP VIIRS 0.64 µm visible channel, 3.74 µm shortwave IR channel. and 11.45 µm IR channel images

Suomi NPP VIIRS 0.64 µm visible channel, 3.74 µm shortwave IR channel. and 11.45 µm IR channel images

An animation of McIDAS images of MTSAT-2 0.73 µm visible channel data (below; click image to play animation) confirmed that the darker volcanic ash fall plume was a stationary feature, and not an airborne volcanic ash plume. The animation also showed the anticyclonic rotation of the gyres of ice floes just off the east coast of Kamchatka.

MTSAT-2 0.73 µm visible channel images (click image to play animation)

MTSAT-2 0.73 µm visible channel images (click image to play animation)

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Undular bore over Texas and the Gulf of Mexico

A comparison of AWIPS images of MODIS 11.0-3.7 µm IR brightness temperature difference “fog/stratus product”, 3.7 µm shortwave IR, 11.0 µm IR window, and 6.7 µm water vapor channel images (above) showed the night-time (08:04 UTC or 3:04 AM local time) development of parallel cloud bands associated with an undular... Read More

MODIS IR brightness temperature difference

MODIS IR brightness temperature difference “fog/stratus product”, 3.7 µm shortwave IR, 11.0 µm IR window, and 6.7 µm water vapor channel images

A comparison of AWIPS images of MODIS 11.0-3.7 µm IR brightness temperature difference “fog/stratus product”, 3.7 µm shortwave IR, 11.0 µm IR window, and 6.7 µm water vapor channel images (above) showed the night-time (08:04 UTC or 3:04 AM local time) development of parallel cloud bands associated with an undular bore that was forming in advance of a strong cold frontal boundary which was  moving southward across Texas on 05 March 2013. Note how the cloud band features showed up with better clarity in the 3.7 µm IR image compared to the 11.0 µm IR image, since the shortwave IR channel is more sensitive to warmer temperatures (the IR brightness temperatures of the cloud bands averaged about +5º C).

After sunrise, the undular bore cloud bands coud be seen moving southeastward off the coast of Texas and across the adjacent offshore waters of the Gulf of Mexico on McIDAS images of GOES-13 0.63 µm visible channel data (below; click image to play animation).

GOES-13 0.63 µm visible channel images (click image to play animation)

GOES-13 0.63 µm visible channel images (click image to play animation)

As the leading edge of the bore passed through Corpus Christi, Texas (CRP on the GOES-13 visible images), surface observations (below) indicated that winds gusted to 38 knots or 44 mph at 12:27 UTC.

Corpus Christi surface observations

Corpus Christi surface observations

The 12 UTC morning rawinsonde data from Corpus Christi (below) revealed a very strong and deep boundary layer temperature inversion (with a top around 962 hPa or 2460 feet), which was acting to duct the undular bore as it propagated southeastward.

Corpus Christi, Texas rawinsonde data

Corpus Christi, Texas rawinsonde data

MODIS 0.65 µm visible channel image and MODIS Sea Surface Temperature product

MODIS 0.65 µm visible channel image and MODIS Sea Surface Temperature product

It is interesting to note that in the wake of the undular bore passage, there appeared to be a signal of Gulf of Mexico water wave activity in both the MODIS Sea Surface Temperature product (above) and the Suomi NPP VIIRS 11.45 µm IR channel image (below). On each corresponding visible channel image, a subtle wave signature could also be seen, but these waves did not appear to be cloud features. Could the strong winds of the bore passage have created wave swells which then acted to mix the water surface enough to allow a small amount of cold water upwelling?

Suomi NPP VIIRS 0.64 µm visible channel and 11.45 µm IR channel images

Suomi NPP VIIRS 0.64 µm visible channel and 11.45 µm IR channel images

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Polar low over the western Bering Sea

AWIPS images of 1-km resolution Suomi NPP VIIRS 0.7 µm Day/Night Band data (above) showed the development of a small polar low in the far western Bering Sea during the 02 March – 03 March 2013 period. A string of breaking Kelvin-Helmholtz waves could be seen feeding into the circulation... Read More

Suomi NPP VIIRS 0.7 µm Day/Night Band images

Suomi NPP VIIRS 0.7 µm Day/Night Band images

AWIPS images of 1-km resolution Suomi NPP VIIRS 0.7 µm Day/Night Band data (above) showed the development of a small polar low in the far western Bering Sea during the 02 March – 03 March 2013 period. A string of breaking Kelvin-Helmholtz waves could be seen feeding into the circulation of the developing low. Station identifiers 25941, 25954, and 21956 denote the villages of Cemurnaut, Korf, and Apuka (respectively) located on the northern end of the Kamchatka Peninsula of Russia.

The corresponding Suomi NPP VIIRS 11.45 µm IR channel images (below) indicated that cloud top IR brightness temperatures were colder than -30º C (darker blue color enhancement) near the center of the polar low circulation.

Suomi NPP VIIRS 11.45 µm IR channel images

Suomi NPP VIIRS 11.45 µm IR channel images

Suomi NPP VIIRS false-color Red/Green/Blue (RGB) images (below) showed that the polar low was developing just south of the sea ice edge (snow and ice appear as darker shades of red). The appearance of red shading also indicated that the cloud tops along the string of Kelvin-Helmholtz waves were beginning to glaciate. Note from the distance scale plotted on the lower left that the diameter of the polar low circulation was less than 100 miles.

Suomi NPP VIIRS false-color Red/Green/Blue (RGB) images

Suomi NPP VIIRS false-color Red/Green/Blue (RGB) images

A larger-scale view using a Suomi NPP VIIRS 0.64 µm visible channel image (below) helped to emphasize the small size of the Bering Sea polar low, especially when compared to the much larger storm system that was located just south of the Aleutian Islands at that time. The tightly-packed isobars of another strong storm approaching from the North Pacific Ocean could also be seen.

Suomi NPP VIIRS 0.64 µm visible channel image + Surface reports and surface analysis

Suomi NPP VIIRS 0.64 µm visible channel image + Surface reports and surface analysis

McIDAS images of MTSAT-2 0.73 µm visible channel data (below; click image to play animation) indicated that the polar low was initially moving southeastward away from the Kamchatka Peninsula, but then began to reverse direction and move back northwestward due to strong southeasterly flow in advance of the large and intense storm over the North Pacific Ocean.

MTSAT-2 0.73 µm visible channel images (click image to play animation)

MTSAT-2 0.73 µm visible channel images (click image to play animation)

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