Morphology and dynamics of the upper cloud layer of Venus

被引:0
|
作者
W. J. Markiewicz
D. V. Titov
S. S. Limaye
H. U. Keller
N. Ignatiev
R. Jaumann
N. Thomas
H. Michalik
R. Moissl
P. Russo
机构
[1] Max-Planck-Institut für Sonnensystemforschung,
[2] Space Research Institute (IKI),undefined
[3] Space Science and Engineering Center,undefined
[4] University of Wisconsin,undefined
[5] Madison,undefined
[6] Wisconsin 53706,undefined
[7] USA ,undefined
[8] Institut für Planetenforschung,undefined
[9] DLR,undefined
[10] 12489 Berlin,undefined
[11] Germany ,undefined
[12] Physikalisches Institut,undefined
[13] IDA,undefined
[14] TU Braunschweig,undefined
[15] D-38106 Braunschweig,undefined
[16] Germany ,undefined
来源
Nature | 2007年 / 450卷
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摘要
ESA's Venus Express probe has been in orbit since April 2006. Eight research papers in this issue present new results from the mission, covering the atmosphere, polar features, interactions with the solar wind and the controversial matter of venusian lightning. Håkan Svedham et al. open the section with a review of the similarities and (mostly) differences between Venus and its 'twin', the Earth. Andrew Ingersoll considers the latest results, and also how the project teams plan to make the most of the probe's remaining six years of life.
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页码:633 / 636
页数:3
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