JUPITER AND SATURN - NEAR-INFRARED SPECTRAL ALBEDOS

被引:24
作者
CLARK, RN [1 ]
MCCORD, TB [1 ]
机构
[1] UNIV HAWAII,INST ASTRON,HONOLULU,HI 96822
基金
美国国家航空航天局;
关键词
D O I
10.1016/0019-1035(79)90063-0
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The near-infrared (0.65-2.5μm) spectral albedo of Jupiter and Saturn with 1.5% spectral resolution is presented for the center of disk and for the limb. There is a distinct difference in the continuum slope between Jupiter and Saturn which may be attributed to a difference in the dust content or composition of the two atmospheres. There is an indication of limb brightening in the deepest CH4 bands on Saturn. No limb brightening is found for Jupiter. © 1979.
引用
收藏
页码:180 / 188
页数:9
相关论文
共 38 条
[1]   INHOMOGENEOUS MODELS OF ATMOSPHERE OF JUPITER [J].
AXEL, L .
ASTROPHYSICAL JOURNAL, 1972, 173 (02) :451-&
[2]   IR SPECTROPHOTOMETRY OF JUPITER AND SATURN [J].
BINDER, AB ;
MCCARTHY, DW .
ASTRONOMICAL JOURNAL, 1973, 78 (09) :939-950
[3]  
BUGAENKO LA, 1972, ASTRON VESTN, V6, P19
[4]  
CLARK RN, UNPUBLISHED
[5]  
CLARK RN, ICARUS
[6]   MINOR CONSTITUENTS IN ATMOSPHERE OF JUPITER [J].
CRUIKSHA.DP ;
BINDER, AB .
ASTROPHYSICS AND SPACE SCIENCE, 1969, 3 (03) :347-&
[7]  
CRUIKSHANK DP, 1968, 103 U AR LUN PLAN LA, P275
[8]   INFRARED SPECTRUM OF JUPITER [J].
DANIELSON, RE .
ASTROPHYSICAL JOURNAL, 1966, 143 (03) :949-+
[9]  
DELBOUILLE L, 1964, MEM SOC ROY SCI LIEG, V9, P125
[10]  
FRANZ OG, 1977, ASTROPHYS J LETT, V214, P145