Supermoon VIIRS Day/Night Band imagery

December 3rd, 2017 |

Composite of Suomi NPP VIIRS Day/Night Band swaths [click to enlarge]

Composite of Suomi NPP VIIRS Day/Night Band swaths [click to enlarge]

The only Supermoon of 2017 occurred on 03 December — and a composite of Suomi NPP VIIRS Day/Night Band (0.7 µm) swaths viewed using RealEarth (above) demonstrated the “visible image at night” capability of that spectral band. A VIIRS instrument is also part of the payload on recently-launched JPSS-1/NOAA-20.

A few examples providing closer looks using VIIRS Day/Night Band (DNB) imagery are shown below, beginning with the western portion of an Atlantic storm that had been producing Gale Force winds during the previous 6-12 hours.

Suomi NPP VIIRS Day/Night Band (0.7 µm) image centered over the western Atlantic [click to enlarge]

Suomi NPP VIIRS Day/Night Band (0.7 µm) image centered over the western Atlantic [click to enlarge]

A toggle between Day/Night Band (0.7 µm) and Fog/stratus Infrared Brightness Temperature Difference (11.45 µm – 3.74 µm) images, centered over the Southeast US (below) showed widespread areas of fog and/or stratus The brighter fog/stratus features were generally brighter on the DNB image..

Suomi NPP VIIRS Day/Night Band (0.7 µm) and Fog/stratus Infrared Brightness Temperature Difference (11.45 µm - 3.74 µm) images, centered over the Southeast US [click to enlarge]

Suomi NPP VIIRS Day/Night Band (0.7 µm) and Fog/stratus Infrared Brightness Temperature Difference (11.45 µm – 3.74 µm) images, centered over the Southeast US [click to enlarge]

Another toggle between DNB and Fog/stratus Infrared Brightness Temperature Difference images, this time centered over Minnesota, Wisconsin and the UP of Michigan (below) revealed snow cover that was much below average for the date — especially across the UP of Michigan.

Suomi NPP VIIRS Day/Night Band (0.7 µm) and Fog/stratus Infrared Brightness Temperature Difference (11.45 µm - 3.74 µm) images, centered over Minnesota and the UP of Michigan [click to enlarge]

Suomi NPP VIIRS Day/Night Band (0.7 µm) and Fog/stratus Infrared Brightness Temperature Difference (11.45 µm – 3.74 µm) images, centered over Minnesota, Wisconsin and the UP of Michigan [click to enlarge]

Finally, a toggle between DNB images from consecutive overpass times (0935 and 1116 UTC), showing small clusters of rain showers moving inland along the coast of Oregon and far northern California (below). Because of the wide scan swath of the VIIRS instrument (2330 km), there are times when the same area will be imaged during 2 consecutive overpasses.

Suomi NPP VIIRS Day/Night Band images, centered off the coast of Oregon [click to enlarge]

Suomi NPP VIIRS Day/Night Band images, centered off the coast of Oregon [click to enlarge]

Dissipation of nocturnal valley fog across New England

October 28th, 2017 |

GOES-16 Visible (0.64 µm) images, with hourly surface reports of fog plotted in yellow [click to play animation]

GOES-16 Visible (0.64 µm) images, with hourly surface reports of fog plotted in yellow [click to play animation]

* GOES-16 data posted on this page are preliminary, non-operational and are undergoing testing *

With high pressure dominating across the region during the pre-dawn nighttime hours (surface analyses), strong radiational cooling (minimum temperatures) aided in the formation of widespread valley fog across New England on 28 October 2017.  Post-sunrise GOES-16 “Red” Visible (0.64 µm) images revealed the areal extent of the valley fog; however, fog dissipation was fairly rapid during the morning hours as surface heating from abundant sunlight promoted sufficient boundary layer mixing.

During the preceding nighttime hours, development of widespread valley fog could be seen on Suomi NPP VIIRS Infrared Brightness Temperature Difference (11.45 µm – 3.74 µm) images (below) — although surface fog features were obscured at times by patchy cirrus clouds aloft (black enhancement). This example demonstrates that because of the wide (3000 km) scan swath of the VIIRS instrument, in many cases the same region might be sampled by 2 consecutive overpasses. VIIRS will also be part of the instrument payload on the upcoming JPSS series of polar-orbiting satellites.

Suomi NPP VIIRS Infrared Brightness Temperature Difference (11.45 µm - 3.74 µm) images [click to enlarge]

Suomi NPP VIIRS Infrared Brightness Temperature Difference (11.45 µm – 3.74 µm) images [click to enlarge]

GOES-16 and Fog Detection

October 18th, 2017 |

GOES-16 Brightness Temperature Difference (10.3 µm – 3.9 µm) “Fog Product” from 0202 – 0357 UTC on 18 October 2017 (Click to animate)

GOES-16 data posted on this page are preliminary, non-operational and are undergoing testing.

Stratus and Fog formed over the valleys of Kentucky (and in surrounding states) early on 18 October 2017 (It was there on 17 October as well). When was the fog first obvious from Satellite imagery? It very much depends on the spatial resolution of the Satellite viewing the scene. The Brightness Temperature Difference field (10.3 µm – 3.9 µm) from GOES-16, shown above, can be used to identify regions of stratus clouds that are made up of water droplets. Carefully examine the animation; the time when fog is definitively present over valleys of eastern Kentucky (around 84º W Longitude) is around 0327 UTC.

GOES-16 has 2-km resolution (at the sub-satellite point — 89.5º W Longitude during GOES-16 Check-out); this is superior to GOES-13’s nominal 4-km resolution at the subpoint (75º West Longitude). The GOES-13 Brightness Temperature Difference Field (10.7 µm – 3.9 µm) at 0330 UTC shows no distinct indication of Fog/Stratus over eastern Kentucky. A series of animations of the GOES-13 Brightness Temperature Difference field, from 0215-0345 UTC, from 0415-0500, from 0545-0700 and from 0700-0815 suggest GOES-13 identified the region of fog about 4 hours after GOES-16, at 0730 UTC.

The GOES-13 vs. GOES-16 toggle below, from 0700 UTC on 18 October 2017, shows how the resolution improvement with GOES-16 facilitates earlier detection of fog and stratus as it develops overnight.

Toggle between 0700 UTC 18 October 2017 Brightness Temperature Differences from GOES-13 (10.7 µm – 3.9 µm) and GOES-16 (10.3 µm – 3.9 µm) (Click to enlarge)

Fog/stratus in the Strait of Juan de Fuca

May 20th, 2017 |

** The GOES-16 data posted on this page are preliminary, non-operational data and are undergoing testing. **

As seen in a Tweet from NWS Seattle/Tacoma (above), a plume of fog/stratus moved rapidly eastward through the Strait of Juan de Fuca on 20 May 2017. A closer view of GOES-16 Visible (0.64 µm) images (below; also available as an MP4 animation) shows the formation of “bow shock waves” as the leading edge of the low-level fog/stratus plume encountered the sharply-angled land surface of Whidbey Island at the far eastern end of the Strait near sunset — surface observations indicated that the visibility at Naval Air Station Whidbey Island was reduced to 0.5 mile just after the time of the final 0327 UTC image in the animation.

GOES-16 Visible (0.64 µm) images, with hourly plots of surface reports [click to play animation]

GOES-16 Visible (0.64 µm) images, with hourly plots of surface reports [click to play animation]

A Suomi NPP VIIRS Visible (0.64 µm) image with RTMA surface winds (below) indicated that westerly/northwesterly wind speeds were generally around 15 knots at 21 UTC (just after the primary fog/stratus plume began to move into the western end of the Strait). Four hours later, there was a northwesterly wind gust of 27 knots at Sheringham, British Columbia (CWSP).

Suomi NPP VIIRS Visible (0.64 µm) images, with RTMA surface winds plotted in cyan [click to enlarge]

Suomi NPP VIIRS Visible (0.64 µm) images, with RTMA surface winds plotted in cyan [click to enlarge]

During the following nighttime hours, a Suomi NPP VIIRS infrared Brightness Temperature Difference (11.45 – 3.74 µm) “Fog/Stratus Product” image at 0910 UTC (below) revealed that the fog/stratus plume covered much of the Strait (especially along the Washington coast), and that the leading edge had begun to spread both northward and southward from Whidbey Island. In addition, note the presence of a linear ship track (darker red enhancement) extending southwestward from Cape Flattery.

Suomi NPP VIIRS Infrared brightness temperature difference (11.45 - 3.74 µm)

Suomi NPP VIIRS infrared Brightness Temperature Difference (11.45 – 3.74 µm) “Fog/Stratus Product” image, with RTMA surface winds plotted in cyan [click to enlarge]

Bill Line (NWS Pueblo) showed the nighttime fog/stratus monitoring capability of a GOES-16 infrared Brightness Temperature Difference product:


On a side note, in the upper right portion of the GOES-16 (as well as the VIIRS) visible images one can also see the hazy signature of glacial sediment  flowing from the Fraser River westward into the Strait of Georgia. Longer-term changes in the pattern of this glacial sediment are also apparent in a comparison of Terra MODIS true-color Red/Green/Blue (RGB) images (source) from 20 April, 07 May and 20 May 2017 (below).

 

Terra MODIS true-color RGB images [click to enlarge]

Terra MODIS true-color RGB images [click to enlarge]