Spatial-Scale Characteristics of a Three-Dimensional Cloud-Resolving Solar Radiation Budget Based on Monte Carlo Radiative Transfer Simulations-Reference-Cited by-同舟云学术

Spatial-Scale Characteristics of a Three-Dimensional Cloud-Resolving Solar Radiation Budget Based on Monte Carlo Radiative Transfer Simulations

Published:2021 Issue:0 Volume:17 Page:228-233
ISSN:1349-6476
Container-title:SOLA
language:en
Short-container-title:SOLA

Author:

Ota Yoshifumi¹,Sekiguchi Miho²,Sato Yousuke³

Affiliation:

1. Meteorological Research Institute, Japan Meteorological Agency

2. Tokyo University of Marine Science and Technology

3. Faculty of Science, Hokkaido University

Publisher

Meteorological Society of Japan

Subject

Atmospheric Science

Link

https://www.jstage.jst.go.jp/article/sola/17/0/17_2021-040/_pdf

Reference19 articles.

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2. Bodhaine, B. A., N. B. Wood, E. G. Dutton, and J. R. Slusser, 1999: On Rayleigh optical depth calculation. J. Atmos. Oceanic Tech., 16, 1854-1861, doi:10.1175/1520-0426(1999)016<1854:ORODC>2.0.CO;2.

3. Brunner, T. A., T. J. Urbatsch, T. M. Evans, and N. A. Gentile, 2006: Comparison of four parallel algorithms for domain decomposed implicit Monte Carlo. J. Comput. Phys., 212, 527-539, doi:10.1016/j.jcp.2005.07.009.

4. Cahalan, R. F., L. Oreopoulos, A. Marshak, K. F. Evans, A. B. Davis, R. Pincus, K. H. Yetzer, B. Mayer, R. Davies, T. P. Ackerman, H. W. Barker, E. E. Clothiaux, R. G. Ellingson, M. J. Garay, E. Kassianov, S. Kinne, A. Macke, W. O'Hirok, P. T. Partain, S. M. Prigarin, A. N. Rublev, G. L. Stephens, F. Szczap, E. E. Takara, T. Várnai, G. Wen, and T. B. Zhuravleva, 2005: THE I3RC: Bringing together the most advanced radiative transfer tools for cloudy atmospheres. Bull. Amer. Meteor. Soc., 86, 1275-1293, doi:10.1175/BAMS-86-9-1275.

5. Emde, C., R. Buras, and B. Mayer, 2011: 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, doi:10.1016/j.jqsrt.2011.03.018.

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