Climate evolution of Venus

被引：30
|
作者：
Taylor, F. [1 ]
Grinspoon, D. [2 ]
机构：
[1] Univ Oxford, Dept Phys, Oxford OX1 3PU, England
[2] Denver Museum Nat & Sci, Denver, CO 80205 USA
来源：
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS | 2009年 / 114卷
关键词：
IMPACT CRATER DENSITIES; MIDDLE ATMOSPHERE; WATER-VAPOR; TERRESTRIAL PLANETS; RESURFACING HISTORY; GLOBAL DISTRIBUTION; PIONEER ORBITER; DEEP ATMOSPHERE; CARBON-MONOXIDE; CLOUD STRUCTURE;
D O I：
10.1029/2008JE003316
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
The processes in the atmosphere, interior, surface, and near-space environment that together maintain the climate on Venus are examined from the specific point of view of the advances that are possible with new data from Venus Express and improved evolutionary climate models. Particular difficulties, opportunities, and prospects for the next generation of missions to Venus are also discussed.
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页数：22
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