|
INTERPRETATION
August 20, 1999 |
|
|
||
Figure 5 |
Figure 6 |
Figure 7 |
| During the nighttime, however, the brightness temperature
gradient across the dryline reverses, as seen in Figure
5, the 0225 UTC 12.0 µm image of 21 May 1999. Here the
darker (warmer) signal is to the east of the dryline, and the cooler (lighter)
signal comes from west of the dryline. Again, examining typical nighttime
temperature and moisture profiles west and east of the dryline provides
the explanation.
Figure 6 shows a typical nighttime sounding from west of the dryline. The surface skin temperature drops rapidly and dominates the 12.0 µm brightness temperature, because there is still a lack of low level moisture. The result is a cool signal. East of the dryline (Figure 7), the surface skin temperature decreases more slowly, and is higher than that west of the dryline. In addition, the low level water vapor now lies in a surface inversion, that is, it is warmer than the surface skin temperature. The combination of the ground and the low level moisture is a 12.0 µm signal which is now warmer than the signal west of the dryline. |
The attached loop shows the movement of the dryline from 2145 UTC to 0515 UTC. Note that because the 12.0 µm brightness temperature west of the dryline drops from greater than, to less than that east of the dryline, there necessarily exists a period of time when the brightness temperature difference across the dryline vanishes, and the position of the dryline cannot be determined using the 12.0 µm channel alone.
The 10.7 µm channel may also be used for this purpose, but it has less moisture attenuation, so the contrast between dry and moist air masses will not be as great.
We welcome your comments and discussion at ramsdis@comet.ucar.edu
| Information Contact: Lewis Grasso | |
| CIRA/RAMM WebMaster: Roger Phillips | |
| Author: Jack Dostalek | |
| Last Updated: August 20, 1999 |