EFFECT OF NON-COHERENCY ON INTENSITY OF RESONANTLY SCATTERED SUNLIGHT IN A PLANETARY ATMOSPHERE

被引：14

作者：

WALLACE, L

机构：

来源：

关键词：

D O I：

10.1016/0032-0633(71)90044-4

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：377 / &

共 16 条

[1]

Chamberlain J.W., 1961, PHYSICS AURORA AIRGL, P704

CHAMBERLAIN, JW ;

SOBOUTI, Y .

[3] BEHAVIOR OF ABSORPTION LINES IN A HAZY PLANETARY ATMOSPHERE [J].

CHAMBERLAIN, JW .

[4] DIFFUSE REFLECTION BY AN INHOMOGENEOUS PLANETARY ATMOSPHERE [J].

CHAMBERLAIN, JW ;

MCELROY, MB .

[5]

CHANDRASEKHAR S, 1950, RAD TRANSFER, P393

DONAHUE, TM .

[7]

DONAHUE TM, 1959, ANN GEOPHYS, V15, P481

[8] The doppler effect in resonance lines [J].

Henyey, LG .

[9] IMPRISONMENT OF RESONANCE RADIATION IN GASES [J].

HOLSTEIN, T .

PHYSICAL REVIEW, 1947, 72 (12) :1212-1233

HUMMER, DG .