Eastern US winter storm

January 3rd, 2018 |

GOES-16

GOES-16 “Red” Visible (0.64 µm, left) and Near-Infrared “Snow/Ice” (1.61 µm, right) images, with plots of hourly surface reports [click to play MP4 animation]

The initial impacts of a large Eastern US winter storm were seen in a comparison of GOES-16 (GOES-East) “Red” Visible (0.64 µm) and Near-Infrared “Snow/Ice” (1.61 µm) images (above) on 03 January 2018 — areas of southeastern Georgia received freezing rain and/or 1-6 inches of snowfall. As clouds began to dissipate, the resulting snow cover appeared bright on the Visible images (since fresh snow is highly reflective at the 0.64 µm wavelength), and darker shades of gray on the Near-Infrared images (since snow and ice are strong absorbers of radiation at the 1.61 µm wavelength). Note the brief appearance of a cloud plume streaming southward from the Hatch Nuclear Power Plant.

Earlier that morning, the Florida Panhandle also received snowfall (text | map), but the lighter accumulations there were insufficient to exhibit a good satellite signature.

In a toggle between Suomi NPP VIIRS true-color and false-color Red-Green-Blue (RGB) images from RealEarth (below), the deeper snow cover in Georgia appears as darker shades of cyan.

Suomi NPP VIIRS true-color and false-color images [click to enlarge]

Suomi NPP VIIRS true-color and false-color images [click to enlarge]

===== 04 January Update =====

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]

A toggle between Suomi NPP VIIRS Day/Night Band (0.7 µm) and Infrared Window (11.45 µm) images at 0620 UTC (1:20 AM Eastern time) on 04 January (above; courtesy of William Straka, CIMSS) showed a nighttime view of the rapidly-intensifying storm when it had an estimated minimum central pressure of 972 hPa or 28.70″. Note the signature of snow cover — extending from southeastern Georgia across eastern portions of South Carolina and North Carolina — which is evident on the “visible image at night” Day/Night Band (made possible by ample illumination from the Moon, which was in the Waning Gibbous phase at 92% of Full). A full-resolution version of the Day/Night Band image is available here.

During the following daytime hours, 30-second interval Mesoscale Sector GOES-16 “Red” Visible (0.64 µm) images (below) showed the evolution of the low pressure center of circulation as it continued to rapidly intensify (surface analyses) off the US East Coast.

30-second GOES-16

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

GOES-16

GOES-16 “Red” Visible (0.64 µm) images, with hourly surface weather type plotted in yellow [click to play MP4 animation]

A larger-scale view (using 5-minute CONUS sector data) of GOES-16 “Red” Visible (0.64 µm) images with hourly plots of surface weather (above) depicted the widespread precipitation associated with the storm. Similarly, plots of hourly wind gusts (below) portrayed the large wind field of the system. Some of the highest snowfall/ice accumulations and peak wind gusts are listed here and here.

GOES-16

GOES-16 “Red” Visible (0.64 µm) images, with hourly surface wind gusts plotted in yellow [click to play MP4 animation]

In the wake of the departing storm, the tropospheric column over Florida and the southeastern US was dry enough (3.7 mm or 0.15″ at Tallahassee FL and 4.0 mm or 0.16 ” at Charleston SC) to allow the GOES-16 Lower-level (7.3 µm) Water Vapor imagery (below) to detect the thermal contrast of surface land/water boundaries — portions of the coastline and a few of the larger inland lakes were evident.

"GOES-16

(7.3 µm, left), Mid-level (6.9 µm, center) and Upper-level (6.2 µm, right) images [click to play animation]” class=”size-medium” /> GOES-16 Lower-level (7.3 µm, left), Mid-level (6.9 µm, center) and Upper-level (6.2 µm, right) images [click to play animation]

A full-resolution Suomi NPP VIIRS true-color RGB image at 1738 UTC (below) revealed interesting storm features such its very large cloud shield and convection near the circulation center, as well as the swath of snow cover across parts of Georgia, South Carolina and North Carolina.

Suomi NPP VIIRS true-color RGB image [click to enlarge]

Suomi NPP VIIRS true-color RGB image [click to enlarge]

A toggle between the corresponding Suomi NPP VIIRS Visible (0.64 µm) and Snow/Ice RGB images (below) helped to highlight locations which received a significant accrual of ice from freezing rain– these areas show up as a darker shade of red on the Snow/Ice RGB image (along the southeastern edge of the swath of snow cover, which is a lighter shade of red). Notable ice accumulations included 0.50″ at Brunswick and Folkston GA, 0.25″ at Georgetown and Myrtle Beach SC, and 0.25″ at Kure Beach NC.

Suomi NPP VIIRS Visible (0.64 µm) and Snow/Ice RGB images, with surface station identifiers plotted in white [click to enlarge]

Suomi NPP VIIRS Visible (0.64 µm) and Snow/Ice RGB images, with surface station identifiers plotted in white [click to enlarge]

Finally, a 30-meter resolution Landsat-8 false-color RGB image viewed using RealEarth (below) showed the snow-covered Charleston, South Carolina area — areas with less dense trees and vegetation showed a more pronounced snow cover signature (shades of cyan). The Charleston International Airport remained closed, due to snow and ice-covered runways.

Landsat-8 false-color RGB image [click to enlarge]

Landsat-8 false-color RGB image [click to enlarge]

Additional imagery of this explosive cyclogenesis event can be found at this blog post.

A prescribed burn in Montana, as viewed from GOES-15, GOES-16 and GOES-13

January 2nd, 2018 |

GOES-15 (left), GOES-16 (center) and GOES-13 (right) Shortwave Infrared (3.9 µm) images, with plots of hourly surface reports [click to play MP4 animation]

GOES-15 (left), GOES-16 (center) and GOES-13 (right) Shortwave Infrared (3.9 µm) images, with plots of hourly surface reports [click to play MP4 animation]

A prescribed burn the SureEnough fire — in central Montana was viewed by GOES-15 (GOES-West), GOES-16 (GOES-East) and GOES-13 Shortwave Infrared (3.9 µm) imagery on 02 January 2018. The images are shown in the native projection for each of the 3 satellites.

Due to the improved spatial resolution of the GOES-16 3.9 µm Shortwave Infrared band (2 km at satellite sub-point, vs 4 km for GOES-15 and GOES-13) and the more frequent image scans (routinely every 5 minutes over CONUS for GOES-16), an unambiguous thermal anomaly or fire “hot spot” was first evident on GOES-16 at 1707 UTC, just southeast of Lewistown (station identifier KLWT). The GOES-16 fire thermal signature was also hotter (black pixels) compared to either GOES-15 or GOES-13.

GOES-13 will cease transmission on 3 January 2018 [Update: 8 January]

January 2nd, 2018 |

GOES-13 Visible (0.63 µm) Image, 1745 UTC on 2 January 2018 (Click to enlarge)

The GOES-13 Satellite, operational as GOES-East from April 2010 through December 2017 (with a notable interruption) will be turned off sometime after 1500 UTC on Wednesday 3 January 2018. (Update: due to an impending East Coast winter storm, GOES-13 deactivation was postponed to 8 January)

The visible Full Disk image above, from 1745 UTC on 2 January 2018, is one of the last fully illuminated visible image the satellite will process.  (The first processed full disk visible image, from 22 June 2006, can be viewed here.)

On 28 December 2017, GOES-13 imagery included a view of the Moon, as shown here (and zoomed in here).  Future GOES-East imagery from GOES-16 will not include images of the Moon.  GOES-16 will scan the moon when it is near the horizon (and there are occasional GOES-16 mesoscale sectors placed over the Moon for calibration purposes).  However, GOES-16 imagery is remapped to Earth points before being broadcast to the public.  The Moon (happily) is not on the Earth and its points will not be remapped.

Thank you GOES-13 for your long years of service.  A full-resolution version of the image above is available here.

When Water Vapor Channels are Window Channels

January 2nd, 2018 |

GOES-16 Low-Level Water Vapor Imagery (7.3 µm), 1322 UTC on 2 January 2017 (Click to enlarge)

The very cold and dry airmass over the eastern half of the United States during early January 2018 is mostly devoid of water vapor, a gas that, when present, absorbs certain wavelengths of radiation that is emitted from the surface (or low clouds). That absorbed energy is then re-emitted from higher (colder) levels. Typically, surface features over the eastern United States are therefore not apparent. When water vapor amounts in the atmosphere are small, however, surface information can escape directly to space, much in the same way as occurs with (for example) the Clean Window channel (10.3 µm) on GOES-16 (water vapor does not absorb energy with a wavelength of 10.3 µm). The low-level water vapor (7.3 µm) image above, from near sunrise on 2 January 2018, shows many surface features over North and South Carolina, Kentucky, Tennessee and southern Illinois. The features are mostly lakes and rivers that are markedly warmer than adjacent land. (In fact, Kentucky Lake and Lake Barkely in southwest Kentucky are also visible in the 6.9 µm imagery!)

Weighting Functions from 1200 UTC on 2 January for Davenport IA (left), Lincoln IL (center) and Greensboro NC (right) for 6.2 µm (Green), 6.95 µm (blue) and 7.3 µm (magenta), that is, the upper-, mid- and lower-level water vapor channels, respectively, on ABI. Peak pressures for the individual weighting functions are noted, as are Total Precipitable Water values at the station (Click to enlarge)

GOES-16 Weighting Functions (Click here ) describe the location in the atmosphere from which the GOES-16 Channel is detecting energy.  The upper-level (6.2 µm) and mid-level (6.95 µm) weighting functions show information originating from above the surface.  Much surface information is available at Greensboro, with smaller proportional amounts at Davenport and Lincoln.

The “Cirrus” Channel on GOES-16’s ABI (Band 4, 1.38 µm) also occupies a spot in the electromagnetic spectrum where water vapor absorption is strong.  Thus, reflected solar radiation from the surface is rarely viewed at this wavelength.  The toggle below, between the ‘Veggie’ Channel (0.86 µm) and the Cirrus Channel (1.38 µm) shows that some surface features — for example, lakes in North Carolina — are present in the Cirrus Channel.

ABI Band 3 (0.86 µm) and ABI Band 4 (1.38 µm) (That is, Veggie and Cirrus channels) at 1502 UTC on 2 January 2018 (Click to enlarge)

Whenever the atmosphere is exceptionally dry, and skies are clear, check the water vapor channels on ABI to see if surface features can be viewed. A few examples of sensing surface features using water vapor imagery from the previous generation of GOES can be seen here.