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Microwave polarized signatures generated within cloud systems
The ATM code includes a series of routines to calculate the polarized radiative transfer
through layers of hydrometeors. These routines have been used to study polarized signatures
observed by the SSM/I instrument over some types of cloud systems. A certain degree of
asphericity and horizontal orientation of the particles is necessary to explain the observations.
You can get more information about this work by downloading paper 22
from my publications list.
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