Satellite Views of Meteor Vapor Trail Over Russia

February 15th, 2013
FY-2D 0.73 µm Visible image

FY-2D 0.73 µm Visible image

A Meteor entered the Earth’s atmosphere over the Ural Mountains of western Russia today at approximately 0320 UTC (09:20 AM local time). The visible image from just after sunrise, above, from the Chinese FY-2D satellite shows an east-west plume, likely from the meteor, near Chelyabinsk. Meteosat-9 also captured the event (YouTube | EUMETSAT), as did Meteosat-10.

Multi-channel animation of FY-2D imagery (courtesy of Tim Schmit, NOAA/NESDIS ASPB)

Multi-channel animation of FY-2D imagery (courtesy of Tim Schmit, NOAA/NESDIS ASPB)

FY-2D has multiple channels. An animation of the visible (0.73 µm), near-infrared (3.8 µm), ‘water vapor’ (6.8 µm) and far-infrared (11.0 µm) is shown above. The signature of the meteor vapor trail is present in each of the channels. A before/after comparison  (03:00 and 03:30 UTC) of FY-2D 0.73 µm visible, 3.8 µm shortwave IR, 6.8 µm water vapor, and 10.8 µm IR window channel images is shown below.

Before/after comparison of FY-2D 0.73 µm visible, 3.8 µm shortwave IR, 6.8 µm water vapor, and 10.8 µm IR window channel images

Before/after comparison of FY-2D 0.73 µm visible, 3.8 µm shortwave IR, 6.8 µm water vapor, and 10.8 µm IR window channel images

An oblique view using 0.73 µm visible channel images from the Japanese MTSAT-2 satellite (below; click image to play animation) revealed that the stratospheric component of the meteor trail could be seen for as long as 9 hours with the aid of illumination from the sun.

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)

A comparison of MTSAT-2 3.75 µm shortwave IR, 10.8 µm longwave IR, and 0.73 µm visible channel images (below; click image to play animation) showed that the meteor plume exhibited a dark (warm) signature on the shortwave IR images, due to this channel’s sensitivity to reflected solar radiation — that signature was seen to disappear with the loss of daytime sunlight. Since the meteor trail was not a particularly dense cloud, it did not exhibit a good signature on the longwave IR images; however, there was some recognizable signal due to the fact that the mean meteor trail IR brightness temperature of around 242 K (-31º C) was significantly warmer than that of the background IR brightness temperature of space (165 K or -108º C).

MTSAT-2 3.75 µm shortwave IR, 10.8 µm longwave IR, and 0.73 µm visible channel images (click image to play animation)

MTSAT-2 3.75 µm shortwave IR, 10.8 µm longwave IR, and 0.73 µm visible channel images (click image to play animation)

Strong Tornado in southern Italy

November 28th, 2012
Meteosat-9 10.8 µm infrared channel images (click image to play animation)

Meteosat-9 10.8 µm infrared channel images (click image to play animation)

A rare November tornado moved through Taranto, (YouTube video, AccuWeather blog entry) in southern Italy, on Wednesday November 28th. A loop of 10.8 µm Meteosat-9 imagery (above) shows the development of an overshooting top in a thunderstorm that is moving over Taranto between 0900 and 0915 UTC (Note that the time indicated on the satellite image is the nominal time — the time that the satellite starts scanning. The actual scan time over southern Italy is approximately 10 minutes later than the nominal time). Such cloud-top features are frequently associated with severe weather. A faint suggestion of an enhanced-V/thermal couplet is apparent in the later imagery as the strong thunderstorm moves northward across the Salento peninsula and then into the Adriatic Sea. METOP-A infrared imagery (below) shows the thunderstorm complex about an hour before a tornadic storm moved inland from the Ionian Sea. The corresponding Meteosat-9 image is here. The higher spatial resolution of the polar orbiter METOP-A allows the discernment of much finer detail in the cloud-top features.

METOP-A 10.8 µm IR imagery

METOP-A 10.8 µm IR imagery

Meteosat-9 0.6 µm visible channel images (click image to play animation)

Meteosat-9 0.6 µm visible channel images (click image to play animation)

Visible imagery from Meteosat-9, above, also shows the development of the overshooting top associated with the tornadic cell. A higher-resolution visible imager from METOP-B, below, showed the line of thunderstorms in which the tornadic cell, indicated by the yellow arrow, was embedded.

METOP-B 0.63 µm Visible imagery

METOP-B 0.63 µm Visible imagery

The tornadic weather was associated with an exceptionally deep extratropical cyclone. On Monday, that system was over the northwestern Mediterranean (see below), with ample evidence of exceptionally cold upper-level air over the Bay of Biscay. This storm also had a history of producing supercellular thunderstorms, as evidenced by the storm development just south of France in the animation below.

Meteosat-9 Visible imagery (0.6 µm) (click image to play animation)

Meteosat-9 Visible imagery (0.6 µm) (click image to play animation)

A multi-day loop of the Meteosat-9 infrared window channel imagery is below. It shows the strong extratropical cyclone moving across southern Europe.

Meteosat-9 10.8 µm infrared channel images (click image to play animation)

Meteosat-9 10.8 µm infrared channel images (click image to play animation)

Total solar eclipse shadow crossing northeastern Australia and the South Pacific Ocean

November 13th, 2012
MTSAT-1R 0.7 µm visible channel images

MTSAT-1R 0.7 µm visible channel images

The shadow from a total solar eclipse could be seen moving east-southeastward across northeastern Australia and the adjacent waters of the South Pacific Ocean on Japanese MTSAT-1R 0.7 µm visible channel images (above).

The solar eclipse shadow was also evident on a visible image from the Korean COMS-1 satellite (below).

COMS-1 visible channel image

COMS-1 visible channel image

As the eclipse shadow continued to move eastward, it was seen on a US NOAA GOES-15 0.63 µm visible channel image (below).

GOES-15 0.63 µm visible channel image

GOES-15 0.63 µm visible channel image