Whole-disk observations of Jupiter, Saturn, and Mars in millimeter/submillimeter bands

被引:28
|
作者
Goldin, AB
Kowitt, MS
Cheng, ES
Cottingham, DA
Fixsen, DJ
Inman, CA
机构
[1] UNIV CHICAGO,ENRICO FERMI INST,CHICAGO,IL 60637
[2] NASA,GLOBAL SCI & TECHNOL INC,ASTRON & SOLAR PHYS LAB,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771
[3] NASA,HUGHES STX,ASTRON & SOLAR PHYS LAB,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771
[4] UNIV CALIF SANTA BARBARA,DEPT PHYS,SANTA BARBARA,CA 93106
来源
ASTROPHYSICAL JOURNAL | 1997年 / 488卷 / 02期
基金
美国国家航空航天局;
关键词
balloons; cosmic microwave background; infrared; solar system; planets and satellites; individual; (Jupiter; Mars; Saturn); radio continuum;
D O I
10.1086/310919
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New balloon-borne observations of whole-disk brightness ratios for Jupiter, Saturn, and Mars are reported in four millimeter/submillimeter bands of bandwidth Delta nu approximate to 1-2 cm(-1). Using the effective planetary radii of Hildebrand et al., we find that TMars/TJupiter = 1.158 +/- 0.015, 1.189 +/- 0.015, 1.470 +- 0.019, and 1.515 +/- 0.019 and T-Saturn/T-Jupiter = 0.833 +/- 0.012, 0.758 +/- 0.010, 0.818 +/- 0.012, and 0.840 +/- 0.012, at nu = 5.7, 9.5, 16.5, and 22.5 cm(-1), respectively. Using models for the brightness temperature of Mars, we also give the whole-disk brightness temperatures for Jupiter and Saturn for the four frequencies.
引用
收藏
页码:L161 / L164
页数:4
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