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Regional And Mesoscale Meteorology Team Satellite Discussion
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1. Visible (Ch. 1; 0.65 um) 2. Short-wave infrared (Ch. 2; 3.9 um) 3. Water vapor (Ch. 3; 6.7 um) 4. Long-wave infrared (Ch. 4; 10.7 um) 5. Long-wave (split-window) infrared (Ch. 5; 12.0 um) 6. Reflectivity product 7. Long-wave difference product In order to determine cloud type over Montana and the Dakotas, we access GOES-10 satellite imagery and products on an individual basis, and then integrate this information to make a final determination. We begin with a frame-by-frame examination over Montana and the Dakotas: 1. Visible
2.
Short-wave
infrared
3.
Water
vapor
4.
Window
infrared
5.
Split-window
infrared
6.
Reflectivity
product
7.
Long-wave
difference product
Taken together, these seven images/products suggest that the clouds over Montana and the Dakotas are thin cirrus. The visible image indicates that the clouds are optically thin, and the water vapor image indicates that the clouds are at mid- to upper-levels. In addition, the black/dark grey color of the clouds in the long-wave difference product is a common feature of thin cirrus. Optically-thin cirrus can explain the appearance of the clouds in the window and split-window infrared channels as well as in the short-wave infrared channel. The near freezing temperature of the clouds in the window and split-window infrared channels can be attributed to transmission of surface radiation through the optically-thin clouds, making the clouds appear significantly warmer. The dark grey appearance of the clouds in the short-wave infrared channel is consistent with optically-thin cirrus, since optically-thick cirrus would appear black. Evidence that these clouds are indeed thin cirrus comes from METAR observations from Dickinson (KDIK) in west-central North Dakota: KDIK 222053Z 32009KT 20SM BKN250 28/03 SLP111 which indicate that, on the 22nd at 2053Z, broken clouds were observed at 25,000 feet (BKN250). A cloud
top pressure product based on GOES sounder observations from the University
of Wisconsin/CIMSS shows the clouds at or above 300 mb.
We welcome your comments and discussion at ramsdis@comet.ucar.edu
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| Information Contact: Lewis Grasso | |
| CIRA/RAMM WebMaster: Roger Phillips | |
| Author: Bard Zajac | |
| Last Updated: October 26, 1999 |