The merger of two giant anticyclones in the atmosphere of Jupiter

被引:48
作者
Sanchez-Lavega, A
Orton, GS
Morales, R
Lecacheux, J
Colas, F
Fisher, B
Fukumura-Sawada, P
Golisch, W
Griep, D
Kaminski, C
Baines, K
Rages, K
West, R
机构
[1] Univ Basque Country, ETS Ingenieros, Dept Fis Aplicada 1, Bilbao 48013, Spain
[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[3] Observ Paris, DESPA, F-92195 Meudon, France
[4] Inst Mecan Celeste, F-75014 Paris, France
[5] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[6] Space Phys Res Inst, Sunnyvale, CA 94087 USA
基金
美国国家航空航天局;
关键词
Jupiter; atmosphere; atmospheric dynamics;
D O I
10.1006/icar.2000.6548
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Two giant ovals in Jupiter's southern atmosphere, vortices of counterclockwise-rotating winds, merged in a 3-week period, starting in March 2000. One of the ovals called FA was more than 60 years old; the other called BE was the product of two 60-year-old ovals (BC and DE) that merged in 1998 (A, Sanchez-Lavega ef al. 1999, Icarus 142, 116-124). The merger took place when the ovals were southeast of the Great Red Spot and after the disappearance of a smaller clockwise-rotating oval midway between them. The interaction began when the high-altitude oval clouds showed counterclockwise rotation about each other, followed by coalescence and shrinking. The interaction in deeper clouds did not include mutual rotation, but there was evidence of complex cloud structure during the merger. (C) 2001 academic Press.
引用
收藏
页码:491 / 495
页数:5
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