Movie 1. Animated imagery (visible, 3.9
micron, and 10.7-13.3 micron) from GOES-12.
Movie
2. Animated imagery (visible, 3.9
micron, and 10.7-12 micron) from GOES-11.
Fig. 1 Comparison between KTLX reflectivity at
2117 UTC and GOES-12 visible and 3.9 micron radiance
Fig. 2. Movie of radar reflectivity (KTLX 0.5 deg scans) superimposed
on GOES 3.9 micron radiance.
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Fig. 3. Movie of radar reflectivity (KTLX 0.5 deg scans)
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Fig. 4. Movie of radar reflectivity (KTLX RHI scan: 160 deg radial)
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Fig. 5. Movie of GOES 3.9 micron radiance
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Fig. 6. Movie of GOES visible and 3.9 micron radiance (hot spots in red)
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The fire locations can be seen as very
dark spots (high brightness temperature) in the 3.9 micron band. These
locations are obsured by clouds at some of the later times. Smoke
plumes are evident in the visible imagery when not obsured by clouds.
The 10.7-13.3 micron brightness temperature difference from GOES-12 is
greater than zero (blue) for clear sky and thin clouds. It approaches
zero for thick clouds and smoke. The 10.7-12 micron brightness
temperature difference from GOES-11 is also greater than zero (blue)
for clear sky and thin clouds, however smoke or dust can sometime be
indicated by a negative difference (green).