Measurements of winds on Mars with Hubble Space Telescope images in 2003 opposition

被引：6

作者：

Kaydash, V. G.

Kreslavsky, M. A.

Shkuratov, Yu. G.

Videen, G.

Bell, J. F., III

Wolff, M.

机构：

[1] Kharkov Natl Univ, Astron Inst, UA-61022 Kharkov, Ukraine

[2] Univ Oulu, Dept Phys, FIN-90014 Oulu, Finland

[3] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA

[4] Space Sci Inst, Boulder, CO 80303 USA

[5] Univ Amsterdam, Astron Inst Anton Pannekoek, NL-1098 SJ Amsterdam, Netherlands

[6] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

来源：

ICARUS | 2006年 / 185卷 / 01期

基金：

美国国家航空航天局;

关键词：

Mars; climate; atmospheres; dynamics; ultraviolet observations;

D O I：

10.1016/j.icarus.2006.07.017

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The winds of Mars at the water cloud level are measured by tracking cloud features in sequential high-resolution Hubble Space Telescope UV images for 5 days during the perihelion season in 2003. Global circulation model (GCM) predictions are in general agreement with the observations for the zonal wind component, but reveal significant differences for the meridional component. (c) 2006 Elsevier Inc. All rights reserved.

引用

页码：97 / 101

页数：5

共 7 条

[1]

BELL J, 2003, EOS T AGU FALL M S, V84

[2] Improved general circulation models of the Martian atmosphere from the surface to above 80 km [J].