Differences

This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
Last revision Both sides next revision
documentation [2016/05/06 12:47]
claudia
documentation [2019/12/23 23:17]
admin
Line 1: Line 1:
 +=== Main documentation of libRadtran ===
  
-Get the main documentation of libRadtran:+    * Documentation for [[http://​www.libradtran.org/​doc/​libradtran.pdf|version 2.0.3 in pdf]] format, also included in the package (libRadtran/​doc/​libRadtran.pdf). 
 +    * A few words on the basic usage of the package can be found [[:basic usage|here]].
  
 +
 +    ​
 +=== libRadtran publications ===
 +
 +The two reference publications provide an **overview of libRadtran and examples of use**:
 +
 +  * C. Emde, R. Buras-Schnell,​ A. Kylling, B. Mayer, J. Gasteiger, U. Hamann, J. Kylling, B. Richter, C. Pause, T. Dowling, and L. Bugliaro. **The libradtran software package for radiative transfer calculations (version 2.0.1).** //​Geoscientific Model Development//,​ 9(5):​1647-1672,​ 2016, [[http://​www.geosci-model-dev.net/​9/​1647/​2016/​|link]]
 +
 +  * B. Mayer and A. Kylling. **Technical note: The libRadtran software package for radiative transfer calculations - description and examples of use**. //Atmos. Chem. Phys.//, 5: 1855-1877, 2005, [[http://​www.atmos-chem-phys.net/​5/​1855/​2005/​acp-5-1855-2005.html|link]]  ​
 +
 +
 +The **absorption parameterization REPTRAN** (default in libRadtran) is described in: 
 + 
 +  *  J. Gasteiger, C. Emde, B. Mayer, R. Buras, S.A. Buehler, and O. Lemke. **Representative wavelengths absorption parameterization applied to satellite channels and spectral bands.** //J. Quant. Spectrosc. Radiat. Transfer//, 148(0):​99-115,​ 2014, [[http://​www.sciencedirect.com/​science/​article/​pii/​S0022407314002842|link]],​{{::​reptran_paper_preprint.pdf|preprint}}
 +
 +Updates included into the **default radiative transfer solver DISORT** (C-Version of DISORT with improved intensity correction method) are described in:
 +
 +  * R. Buras, T. Dowling, and C. Emde. **New secondary-scattering correction in DISORT with increased efficiency for forward scattering.** //J. Quant. Spectrosc. Radiat. Transfer//, 112(12):​2028-2034,​ 2011. [[https://​doi.org/​10.1016/​j.jqsrt.2011.03.019|link]].
 +
 +The tool to calculate line-by-line absorption coefficients **py4CAtS** (PYthon for Computational ATmospheric Spectroscopy) is described in: 
 +
 +  * F. Schreier, S. Gimeno García, P. Hochstaffl, and S. Städt. **Py4CAtS—PYthon for Computational ATmospheric Spectroscopy**. Atmosphere 2019, 10, 262. [[https://​www.mdpi.com/​2073-4433/​10/​5/​262/​htm|link]]
 +
 +There are various publications related to the **Monte Carlo solver MYSTIC** (1D version available in the public version of libRadtran):​
 +
 +  * //General overview:// B. Mayer. **Radiative transfer in the cloudy atmosphere.** //European Physical Journal Conferences//,​ 1:75-99, 2009. [[http://​www.epj-conferences.org/​articles/​epjconf/​abs/​2009/​01/​epjconf1008/​epjconf1008.html|link]]
 +    ​
 +  * //Spherical geometry:// C. Emde and B. Mayer. **Simulation of solar radiation during a total eclipse: a challenge for radiative transfer.** //Atmos. Chem. Phys.//, 7:​2259-2270,​ May 2007. [[http://​www.atmos-chem-phys.net/​7/​2259/​2007/​|link]]
 +
 +  * //​Polarization://​ C. Emde, R. Buras, B. Mayer, and M. Blumthaler. **The impact of aerosols on polarized sky radiance: model development,​ validation, and applications.** //Atmos. Chem. Phys.//, 10, 383-396, 2010. [[http://​www.atmos-chem-phys.net/​10/​383/​2010/​acp-10-383-2010.html|link]]
 +
 +  * //​Topography://​ B. Mayer, S.W. Hoch, and C.D. Whiteman. **Validating the MYSTIC three-dimensional radiative transfer model with observations from the complex topography of Arizona'​s Meteor Crater.** //Atmos. Chem. Phys.//, 10, 8685-8696, 2010. [[https://​www.atmos-chem-phys.net/​10/​8685/​2010/​|link]]
 +
 +  * //Variance reduction methods:// R. Buras and B. Mayer. **Efficient unbiased variance reduction techniques for Monte Carlo simulations of radiative transfer in cloudy atmospheres:​ the solution.** //J. Quant. Spectrosc. Radiat. Transfer//, 112, 434-447, 2011. [[http://​www.sciencedirect.com/​science/​article/​pii/​S0022407311001373|link]]
 +
 +  * //Efficient spectral calculations://​ C. Emde, R. Buras, R., and B. Mayer. **ALIS: An efficient method to compute high spectral resolution polarized solar radiances using the Monte Carlo approach.** //J. Quant. Spectrosc. Radiat. Transfer//, 112, 1622-1631, 2011. [[http://​www.sciencedirect.com/​science/​article/​pii/​S0022407311001373|link]]
 +  ​
 +  * //Thermal heating and cooling rates:// C. Klinger and B. Mayer. **Three-dimensional Monte Carlo calculation of atmospheric thermal heating rates.** , //J. Quant. Spectrosc. Radiat. Transfer//, 144:​123--136,​ 2014. [[https://​www.sciencedirect.com/​science/​article/​pii/​S0022407314001642|link]]
 +
 +=== libRadtran development ===
 +
 +If you want to contribute to further development of libRadtran please contact the libRadtran developers.
  
  
-    * Documentation for [[http://​www.libradtran.org/​doc/​libradtran.pdf|version 2.0 in pdf]] format. 
-    * A few words on the basic usage of the package can be found [[:basic usage|here]]. 
-    * The [[http://​www.geosci-model-dev.net/​9/​1647/​2016/​|reference publication]] provides an overview of libRadtran and examples of use. 
  
-If you want to contribute to further development of libRadtran some ideas are provided in the [[:​documentation:​todo|TODO]] file. 
  
-More information is provided by several [[Publications]]. ​+ 
 
 
documentation.txt · Last modified: 2020/12/23 23:18 by admin
Recent changes RSS feed Creative Commons License Valid XHTML 1.0 Valid CSS Driven by DokuWiki
Drupal Garland Theme for Dokuwiki