2014
DOI: 10.1016/j.jqsrt.2014.02.030
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Analysis of cirrus cloud spectral signatures in the far infrared

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Cited by 25 publications
(32 citation statements)
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“…Radiative transfer computation are performed with the RTX code (Rizzi et al, ) that is an extension of the RT3 doubling and adding code introduced by Evans and Stephens (). RTX is a plane parallel, line‐by‐line multiple scattering radiative transfer algorithm used as a reference tool for faster radiative codes (Bozzo et al, ), for validation/calibration experiments (Maestri et al, ), for theoretical studies (Harries et al, ), for cloud properties studies (Bozzo et al, ), and in support of cloud properties retrievals (i.e., in Maestri et al, ).…”
Section: Microphysical Assumptions and Radiative Computations Setupmentioning
confidence: 99%
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“…Radiative transfer computation are performed with the RTX code (Rizzi et al, ) that is an extension of the RT3 doubling and adding code introduced by Evans and Stephens (). RTX is a plane parallel, line‐by‐line multiple scattering radiative transfer algorithm used as a reference tool for faster radiative codes (Bozzo et al, ), for validation/calibration experiments (Maestri et al, ), for theoretical studies (Harries et al, ), for cloud properties studies (Bozzo et al, ), and in support of cloud properties retrievals (i.e., in Maestri et al, ).…”
Section: Microphysical Assumptions and Radiative Computations Setupmentioning
confidence: 99%
“…An a priori analysis concerning the expansion of particles phase function in terms of Legendre polynomials is required as a compromise between model accuracy and computing time. Maestri et al () show that using nz = 16 zenith angles for each hemisphere is insufficient to obtain an accurate computation of the radiance spectral field, especially in presence of ice particle with large dimensions. The number of zenith angles used in the radiance field computations affect the representation accuracy of the phase function that is expanded in terms of Legendre coefficients ( nc ).…”
Section: Microphysical Assumptions and Radiative Computations Setupmentioning
confidence: 99%
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“…The contribution of the far infrared region (FIR) below 667 cm −1 (wavelength > 15 µm) is also very important (Maestri et al, 2014) because in this region the emitted spectrum is extremely sensitive to the cloud particle effective diameter, in particular for small particle sizes ( 20-30 µm). The sensitivity to the effective diameter is enhanced in the FIR because of the strong modulation of the imaginary part of the refractive index of ice (Lynch et al, 2002;Baran, 2007), which has a peak at 800 cm −1 and a minimum at 400 cm −1 .…”
Section: Introductionmentioning
confidence: 99%
“…The FIRR was developed as a technology demonstrator for the Thin Ice Clouds in Far-InfraRed Experiment (TICFIRE; Blanchet et al, 2011) satellite mission, the primary focus of which is on the water cycle in the Arctic, and ice clouds in particular. Like cirrus at midlatitudes (Cox et al, 2010;Maestri et al, 2014), ice clouds encountered in the Arctic significantly affect the atmosphere radiative budget in the FIR, especially because they can fill the whole troposphere (Grenier et al, 2009). In very dry conditions, they act as particularly efficient emitters that radiatively cool the atmosphere (Blanchet et al, 2011).…”
Section: Introductionmentioning
confidence: 99%