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Retrieving cloud top structure from infrared satellite data

A new retrieval method to detect steep temperature gradients between the convective overshoots of cumulonimbus clouds and the surrounding cirrus has been applied to determine gradients and their orientation in the image plane of infrared data of the AVHRR. These orientations are used to derive cloud...

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Bibliographic Details
Published in:Journal of Geophysical Research 2000-06, Vol.105 (D12), p.15
Main Authors: van Hees, Richard M, Lelieveld, Jos
Format: Article
Language:English
Online Access:Get full text
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Summary:A new retrieval method to detect steep temperature gradients between the convective overshoots of cumulonimbus clouds and the surrounding cirrus has been applied to determine gradients and their orientation in the image plane of infrared data of the AVHRR. These orientations are used to derive cloud elevations which are brightened by the sun or are in shadow, which strongly affects the visible signal. The impact of temperature gradients on the visible radiances is illustrated by two examples that indicate deep convective overshoots. Both examples show that the illuminated side of the overshoots can exceed the cloud top reflectivity by 50 percent, while the shadows account for less than 50 percent of the cloud top reflectance. The shadows usually extend several pixels beyond the base of the overshoots. Here we show that statistical analyses of cloud optical depth are affected by the cloud top structure, based on one month of high-resolution AVHRR satellite data. The contribution of shadow side pixels with steep temperature gradients can exceed 30 percent for small optical depths. The contribution of illuminated sides of cloud top structures and cloud sides with steep temperature gradients can exceed 70 percent for large optical depths. (Author)
ISSN:0148-0227