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Results are shown for MODIS band 27 (water vapor absorption band) and band 31 (window band).
Fig. 3 The Ash RGB (upper row), band #13 image (middle row) and split window (band #13–#15) image (bottom row).
Figure 1 shows the BT and BT differences (BTDs) at the split window band, calculated for liquid and ice clouds with a CTT of 247 K in a tropical atmosphere with a sea surface temperature of 300 K.
These bands enable us to detect "SO2 rich" plumes which are overlooked by using conventional images such as IR (band #13) and a split window (band #13–#15) for Himawari-8.
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The typical Wright-designed residence from this period displayed a wide, low roof over continuous window bands that turned corners, defying the conventional boxlike structure of most houses, and the house's main rooms flowed together in an uninterrupted space.
Cloud emissivities in the split window bands can be obtained by using this cloud temperature estimate.
As shown in Fig. 1, the split window bands are sensitive to the cloud phase.
Fig. 1 Sensitivities of the split window bands to COT, effective particle radius, and cloud thermodynamic phase.
The maximum noise is 0.4 K at MODIS band 27, and the noise is less than 0.25 K in the window bands.
Baum et al. (2012) showed that in their algorithm refinement for MODIS C6, using cloud emissivity ratios between the split window bands substantially improves the inference of the ice cloud phase, especially for optically thin ice clouds.
Iwabuchi et al. (2014) also used the CTT obtained from the CO2 slicing technique to help estimate the optical and microphysical properties from the split window bands of MODIS.
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