GOES-13 0.63 µm visible channel images

McIDAS images of 1-km resolution GOES-13 0.63 µm visible channel data (above) showed that there were a number of “hole punch clouds” and long “aircraft dissipation trails” (or “distrails”) drifting east-northeastward over eastern Georgia and the northern half of South Carolina on 17 February 2012. These features occur when aircraft ascend or descend through a cloud layer composed of supercooled water droplets — particles from the jet engine exhaust act as ice nuclei that initiate glaciation. The resulting relatively large ice crystals then begin to fall out of the supercooled water droplet cloud layer, causing the hole punch or aircraft dissipation trail to appear.

A closer view using a 250-meter resolution Terra MODIS true-color Red/Green/Blue (RGB) image from the SSEC MODIS Today site (below; viewed using Google Earth) shows more structural details of some of the hole punch and distrail features at 15:47 UTC (10:47 am local time). The aircraft likely penetrated the supercooled water droplet cloud over Georgia, after which the hole punch and distrail signatures grew as the cloud drifted east-northeastwrad over South Carolina.

MODIS true color Red/Green/Blue (RGB) image (viewed using Google Earth)

A comparison of 250-meter resolution Terra MODIS true-color and false-color Red/Green/Blue (RGB) images (below) helps to verify that the hole punch and distrail features were indeed composed of ice crystals (which appear as cyan on the false-color image, in contrast to the brighter white supercooled water droplet cloud features).

MODIS true-color and false-color Red/Green/Blue (RGB) images

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GOES-13 fog/stratus product (click image to play animation)

AWIPS images of the GOES-13 fog/stratus product (above; click image to play animation) did not do a particularly good job of depicting a well-defined signal of the fog/stratus that was in place across parts of the Ohio River Valley region on 17 February 2012. Note that a number of stations were reporting night-time fog and/or freezing fog in parts of far eastern Missouri, southern Illinois and Indiana, and western Kentucky.

4-km resolution GOES-13 and 1-km resolution MODIS fog/stratus product

Even with the improved 1-km resolution of the MODIS fog/stratus product, no good signal was displayed at 03:40 UTC  (above) or at 07:52 UTC (below) over the areas that were reporting fog/freezing fog.

4-km resolution GOES-13 and 1-km resolution MODIS fog/stratus product

As part of CIMSS participation in GOES-R Proving Ground activities, new satellite products are being developed and tested — and one such product is an Instrument Flight Rules (IFR) Probability product (below; click image to play animation). This IFR Probability product blends satellite data and model fields to display regions where the cloud ceiling is likely to be between 500 and 1000 feet. The IFR Probability product did a much better job at highlighting the relatively large area where IFR cloud ceiling conditions were present at a number of reporting stations (some of which were experiencing cloud ceilings of 100 to 200 feet, along with freezing fog limiting the visibility to 0.3 miles at times) — for example: Effingham IL (K1H2) / Mount Vernon IL (KMVN) / Harrisburg IL (KHSB) / Lawrenceville IL (KLWV) / Bloomington IN (KBMG) / Cape Girardeau MO (KGCI) / Pahducah KY (KPAH).

GOES-13 IFR Probability product (click image to play animation)

GOES-13 0.63 µm visible channel images (below; click image to play animation) showed the areas of fog/stratus burning off quickly after sunrise — and the fog/stratus appeared to be relatively shallow in nature. The fact that the fog/stratus did not appear to be very thick may have been a factor that limited detection by the traditional GOES-13 (10.7-3.9 µm) and MODIS (11-3.7 µm) fog/stratus products.

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

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GOES-15 6.5 µm water vapor channel images (click image to play animation)

GOES water vapor imagery tells you how moist or how dry the middle to upper troposphere is, right? Well, in general, yes — but it’s important to remember that the water vapor imagery actually displays the temperature of a layer of moisture that is emitting radiation. This layer of moisture emitting the radiation that is sensed by the water vapor detectors is usually located within the middle to upper troposphere, but if the atmosphere is quite dry (and/or quite cold), the water vapor channel can actually “see” further down through the troposphere and sense thermal radiation that is emitted from the surface.

On 14 February 2012, GOES-15 6.5 µm water vapor channel images (above; click image to play animation) centered on the Big Island of Hawaii showed how the two highest topographical features  (Mauna Kea and Mauna Loa) initially appeared cooler (darker blue color enhancement) than the rest of the island prior to sunrise, but then quickly warmed (exhibiting brighter yellow colors) during the morning hours as sunlight warmed the surface.

GOES-15 0.63 µm visible channel images (below; click image to play animation) showed that the peaks of Mauna Kea and Mauna Loa were cloud-free during this period.

GOES-15 0.63 µm visible channel images (click image to play animation)

While there was a band of higher moisture associated with the ITCZ well south of Hawaii, and another band of moisture along a cold frontal boundary well northwest of Hawaii, the atmosphere over Hawaii itself was fairly dry — MIMIC Total Precipitable Water values (below) generally in the 20-25 mm range over the islands (animation).

MIMIC Total Precipitable Water product + surface analysis

In this case, the middle to upper troposphere over the Hawaii region was quite dry, which had the effect of shifting the altitude of the water vapor channel weighting function (below) to an altitude low enough to enable some thermal radiation emitted from the higher terrain on Hawaii to “bleed up” through what little water vapor was present aloft and be detected on the GOES-15 water vapor channel imagery.

GOES-15 water vapor channel weighting function (using Hilo HI rawinsonde data)

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Meteosat-7 10.8 µm IR images

EUMETSAT Meteosat-7 10.8 µm IR images from the CIMSS Tropical Cyclones site (above) showed the formation of a well-defined eye as Tropical Cyclone Giovanna (12S) intensified from a Category 3 to a Category 4 storm over the Indian Ocean late in the day on 12 February 2012.

Tropical Cyclone Giovanna maintained a Category 4 intensity as it approached the island nation of Madagascar on 13 February, with the diameter of the eye contracting somewhat on IR imagery as Giovanna was undergoing an eyewall replacement cycle (below).

Meteosat-7 10.8 µm IR images

A few hours prior to landfall, a timely overpass of the EUMETSAT Metop-A satellite allowed a nice view of the surface wind structure using ASCAT scatterometer winds (below).

Meteosat-7 10.8 µm IR images + MetOp-A ASCAT scatterometer surface winds

As the tropical cyclone approached the eastern coast of Madagascar, the erosion of the eastern semicircle of the inner eyewall of Giovanna could be seen in the MIMIC-TC product (below).

MIMIC-TC microwave product

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