The morphology and brightness of the zodiacal light and gegenschein

被引:25
作者
James, JF
Mukai, T
Watanabe, T
Ishiguro, M
Nakamura, R
机构
[1] KOBE UNIV, INFORMAT PROC CTR, NADA KU, KOBE, HYOGO 657, JAPAN
[2] KOBE UNIV, DEPT EARTH & PLANETARY SCI, NADA KU, KOBE, HYOGO 657, JAPAN
关键词
interplanetary medium;
D O I
10.1093/mnras/288.4.1022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A cooled CCD camera with 385 x 576 pixel has been used, in conjunction with a 16-mm fish-eye lens, to construct an isophot map of the zodiacal light and the gegenschein. The axis of symmetry of the zodiacal light at westerly elongations has been measured out to epsilon(.) = 80 degrees and found to be significantly south of the ecliptic plane and the axis of the invariable plane. A considerable north-south asymmetry in the intensity distribution was also found. The position and excess brightness of the gegenschein have also been measured. Its longitude is at the antisolar point within the limit of measurement, its centroid is 2.degrees 5 +/- 0.degrees 5 south of the ecliptic and its excess brightness is 40 +/- 5 S-10 units.
引用
收藏
页码:1022 / +
相关论文
共 23 条
[1]  
Blackwell D.E., 1967, ADV ASTRON ASTROPHYS, V5, P1
[2]   OBSERVATIONS OF THE ZODIACAL LIGHT FROM A VERY HIGH ALTITUDE STATION .1. THE AVERAGE ZODIACAL LIGHT [J].
BLACKWELL, DE ;
INGHAM, MF .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1961, 122 (02) :113-&
[3]  
Cooper BL, 1996, ASTR SOC P, V104, P333
[4]  
Dermott S. F., 1996, AIP C P, V348, P25
[5]  
DIVARI NB, 1960, AJ, V3, P832
[6]  
DUMONT R, 1976, ASTRON ASTROPHYS, V51, P393
[7]  
HONG SS, 1991, ASTROPHYS SPACE SC L, V173, P147
[8]   PHOTOELECTRIC OBSERVATIONS OF PHOTOMETRIC AXIS OF ZODIACAL LIGHT [J].
HURUHATA, M .
PLANETARY AND SPACE SCIENCE, 1965, 13 (03) :237-&
[9]  
KINGSLAKE R, 1989, HIST PHOTOGRAPHIC LE
[10]  
LEINERT C, 1982, ASTRON ASTROPHYS, V110, P355