Technical Note: A new discrete ordinate first-order rotational  Raman scattering radiative transfer model – implementation and first results

Kylling, Arve; Mayer, Bernhard; Blumthaler, M.

doi:10.5194/acp-11-10471-2011

Cited by 3 publications

(5 citation statements)

References 46 publications

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“…-rotational Raman scattering explaining the filling-in of Fraunhofer lines in the solar spectrum (Kylling et al, 2011);…”

Section: Emde Et Almentioning

confidence: 99%

“…Moreover libRadtran now includes a solver to calculate rotational Raman scattering (Kylling et al, 2011), which improves the accuracy of trace gas retrievals. Further the Raman-scattering signal can be used to estimate cloud top pressure from satellite measurements and aerosol properties from surface and satellite observations.…”

Section: Emde Et Almentioning

confidence: 99%

“…For calculations with rotational Raman scattering, the C version has been generalized so that arbitrary source functions (not only a solar or thermal source function) can be handled (Kylling and Stamnes, 1992;Kylling et al, 2011). Rotational (inelastic) Raman scattering from other wavelengths into the wavelength, for which the RTE is solved, is included into the source term.…”

Section: Disortmentioning

confidence: 99%

“…This way, the size distribution may differ between the atmospheric layers. An example can be found in Kylling et al (2013). …”

Section: Multiple Atmospheric Constituentsmentioning

confidence: 99%

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The libRadtran software package for radiative transfer calculations (version 2.0.1)

Buras-Schnell²,

et al. 2016

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Abstract. libRadtran is a widely used software package for radiative transfer calculations. It allows one to compute (polarized) radiances, irradiance, and actinic fluxes in the solar and thermal spectral regions. libRadtran has been used for various applications, including remote sensing of clouds, aerosols and trace gases in the Earth's atmosphere, climate studies, e.g., for the calculation of radiative forcing due to different atmospheric components, for UV forecasting, the calculation of photolysis frequencies, and for remote sensing of other planets in our solar system. The package has been described in Mayer and Kylling (2005). Since then several new features have been included, for example polarization, Raman scattering, a new molecular gas absorption parameterization, and several new parameterizations of cloud and aerosol optical properties. Furthermore, a graphical user interface is now available, which greatly simplifies the usage of the model, especially for new users. This paper gives an overview of libRadtran version 2.0.1 with a focus on new features. Applications including these new features are provided as examples of use. A complete description of libRadtran and all its input options is given in the user manual included in the libRadtran software package, which is freely available at http://www.libradtran.org.

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“…-rotational Raman scattering explaining the filling-in of Fraunhofer lines in the solar spectrum (Kylling et al, 2011);…”

Section: Emde Et Almentioning

confidence: 99%

Section: Emde Et Almentioning

confidence: 99%

Section: Disortmentioning

confidence: 99%

“…This way, the size distribution may differ between the atmospheric layers. An example can be found in Kylling et al (2013). …”

Section: Multiple Atmospheric Constituentsmentioning

confidence: 99%

See 2 more Smart Citations

The libRadtran software package for radiative transfer calculations (version 2.0.1)

Buras-Schnell²,

et al. 2016

View full text Add to dashboard Cite

show abstract

“…-rotational Raman scattering explaining the filling-in of Fraunhofer lines in the solar spectrum (Kylling et al, 2011); -Estimation of background radiation affecting lidar measurements (e.g. Ehret et al, 2008); -Remote sensing of planetary atmospheres (e.g.…”

Section: Introductionmentioning

confidence: 99%

The libRadtran software package for radiative transfer calculations (Version 2.0)

Emde¹,

Buras-Schnell²,

Kylling³

et al. 2015

Preprint

Self Cite

View full text Add to dashboard Cite

Abstract. libRadtran is a widely used software package for radiative transfer calculations. It allows to compute (polarized) radiances, irradiances, and actinic fluxes in the solar and thermal spectral regions. libRadtran has been used for various applications, including remote sensing of clouds, aerosols and trace gases in the Earth's atmosphere, climate studies, e.g., for the calculation of radiative forcing due to different atmospheric components, for UV-forcasting, the calculation of photolysis frequencies, and for remote sensing of other planets in our solar system. The package has been described in Mayer and Kylling (2005).. Since then several new features have been included, for example polarization, Raman scattering, a new molecular gas absorption parameterization, and several new cloud and aerosol scattering parameterizations. Furthermore a graphical user interface is now available which greatly simplifies the usage of the model, especially for new users. This paper gives an overview of libRadtran version 2.0 with focus on new features. A complete description of libRadtran and all its input options is given in the user manual included in the libRadtran software package, which is freely available at http://www.libradtran.org.

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Polarized radiative transfer through terrestrial atmosphere accounting for rotational Raman scattering

Lelli

Розанов

Vountas

et al. 2017

Journal of Quantitative Spectroscopy and Radiative Transfer

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Technical Note: A new discrete ordinate first-order rotational Raman scattering radiative transfer model – implementation and first results

Cited by 3 publications

References 46 publications

The libRadtran software package for radiative transfer calculations (version 2.0.1)

The libRadtran software package for radiative transfer calculations (version 2.0.1)

The libRadtran software package for radiative transfer calculations (Version 2.0)

Polarized radiative transfer through terrestrial atmosphere accounting for rotational Raman scattering

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