All-sky radiative transfer calculations for IASI and IASI-NG: The σ-IASI-as code
Author(s) -
Giuliano Liuzzi,
M. G. Blasi,
Guido Masiello,
Carmine Serio,
Sara Venafra
Publication year - 2017
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
SCImago Journal Rank - 0.177
H-Index - 75
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.4975506
Subject(s) - radiative transfer , sky , context (archaeology) , environmental science , atmospheric radiative transfer codes , remote sensing , meteorology , physics , geology , optics , paleontology
In the context of the development by EUMETSAT of a new generation of meteorological satellites, we have built the new σ-IASI-as (where "as" stands for "all sky") radiative transfer code. Unlike its predecessor σ-IASI, the code is able to calculate both clear and cloudy sky radiances, as well as their Jacobians with respect to any desired geophysical parameter. In addition, σ-IASI-as can perform calculations to simulate the extinction effect of the most common types of atmospheric aerosols and of clouds via ab-initio Mie calculations. We briefly describe the analytical scheme on which the model is based, and have a glance to its potentialities illustrating some sample calculations. Overall, the new model is a complete and fast radiative transfer tool for IASI, and already available for IASI-NG and MTG-IRS
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