SPHERICAL HARMONICS METHODS FOR POLARIZED-LIGHT COMPUTATIONS - NOTE ABOUT FORMATION OF LIGHT SCATTERED BY OPTICALLY THICK PLANETARY ATMOSPHERES

被引：3

作者：

DEUZE, JL ^{[1
]}

DEVAUX, C ^{[1
]}

HERMAN, M ^{[1
]}

机构：

[1] UNIV SCI & TECHN LILLE,CNRS,LAB OPTIQUE ATMOSPH,F-59650 VILLENEUVE,FRANCE

来源：

NOUVELLE REVUE D OPTIQUE | 1975年 / 6卷 / 02期

关键词：

D O I：

10.1088/0335-7368/6/2/304

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

引用

页码：103 / 111

页数：9

共 13 条

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[4] COMPARISON OF VARIOUS METHODS FOR SOLVING EQUATION OF TRANSFER OR RADIATION IN SCATTERING MEDIUM
DEVAUX, C
FOUQUART, Y
HERMAN, M
LENOBLE, J
[J]. JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 1973, 13 (12) : 1421 - 1431
[5] HANSEN JE, 1971, J ATMOS SCI, V28, P120, DOI 10.1175/1520-0469(1971)028<0120:MSOPLI>2.0.CO
[6] 2
[7] CLOUDS OF VENUS - EVIDENCE FOR THEIR NATURE
HANSEN, JE
ARKING, A
[J]. SCIENCE, 1971, 171 (3972) : 669 - &
[8] HERMAN M, 1965, CR HEBD ACAD SCI, V260, P468
[9] HERMAN M, 1968, J QUANT SPECTROSC RA, V28, P355
[10] Kourganoff V., 1952, BASIC METHODS TRANSF