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A measurement of the albedo of thick cirrus clouds at 3.9 μm
Author(s) -
Kidder Stanley Q.
Publication year - 2002
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2001gl014041
Subject(s) - cirrus , albedo (alchemy) , zenith , radiance , transmittance , cloud albedo , solar zenith angle , remote sensing , environmental science , atmospheric sciences , physics , optics , cloud computing , geology , cloud cover , computer science , art , performance art , art history , operating system
Cirrus (ice) clouds are often semitransparent (transmittance greater than zero, but less than one), which makes it difficult to measure fundamental cloud properties, such as albedo. This paper explores a way to measure the albedo of thick cirrus clouds (zero transmittance) at 3.9 μm using GOES Imager data. In brief, the 10.7 μm GOES data are used to separate the cirrus clouds into temperature classes. Then the measured 3.9 μm radiance is plotted against the cosine of the solar zenith angle. A theoretical relationship between radiance and solar zenith angle is used to extract the albedo. The result is that thick cirrus clouds have an albedo of 1.08% ± 0.05% at 3.9 μm. The albedo of thick cirrus is a step toward the measurement of the transmittance of thin cirrus.

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