| contributor author | Dave, J. V. | |
| date accessioned | 2017-06-09T14:18:21Z | |
| date available | 2017-06-09T14:18:21Z | |
| date copyright | 1975/07/01 | |
| date issued | 1975 | |
| identifier issn | 0022-4928 | |
| identifier other | ams-16877.pdf | |
| identifier uri | http://onlinelibrary.yabesh.ir/handle/yetl/4152708 | |
| description abstract | It is shown that the method based on a direct numerical solution of the spherical harmonics approximation to the radiative transfer equation can be used for obtaining smooth scattered-intensity vs angle-of-observation curves for any arbitrary position of the sun. Results presented for models of moderate (?10) optical thickness and with Rayleigh, haze, as well as non-precipitating cloud phase functions show that intensity values of a given accuracy can be obtained with moderate computing resources. | |
| publisher | American Meteorological Society | |
| title | A Direct Solution of the Spherical Harmonies Approximation to the Radiative Transfer Equation for an Arbitrary Solar Elevation. Part II: Results | |
| type | Journal Paper | |
| journal volume | 32 | |
| journal issue | 7 | |
| journal title | Journal of the Atmospheric Sciences | |
| identifier doi | 10.1175/1520-0469(1975)032<1463:ADSOTS>2.0.CO;2 | |
| journal fristpage | 1463 | |
| journal lastpage | 1474 | |
| tree | Journal of the Atmospheric Sciences:;1975:;Volume( 032 ):;issue: 007 | |
| contenttype | Fulltext | |
