共查询到20条相似文献,搜索用时 15 毫秒
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Marty B 《Science (New York, N.Y.)》2006,312(5774):706-707
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Crisp D 《Science (New York, N.Y.)》2001,291(5503):444-445
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Lorenz RD 《Science (New York, N.Y.)》2000,290(5491):467-468
When the Voyager 1 spacecraft returned images in 1980, the dense atmosphere of Saturn's moon Titan was assumed to be bland and featureless. As Lorenz discusses in his Perspective, recent ground-based spectroscopy, and images from the Hubble Space Telescope, are changing this perception. Observations such as the short-lived clouds in Titan's atmosphere reported by Griffith et al. suggest that although average precipitation is likely to be low, individual precipitation events may be heavy enough to cause deep valleys on Titan's surface. 相似文献
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Sykes MV 《Science (New York, N.Y.)》2008,319(5871):1765
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McKinnon WB 《Science (New York, N.Y.)》2012,336(6078):162-163
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Podolak M 《Science (New York, N.Y.)》2007,317(5843):1330-1331
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Asphaug E 《Science (New York, N.Y.)》2007,316(5827):993-994
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Banin A 《Science (New York, N.Y.)》2005,309(5736):888-890
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Coates AJ 《Science (New York, N.Y.)》2011,332(6034):1157-1158
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Tielens AG 《Science (New York, N.Y.)》2003,300(5616):68-71
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Holdsworth RE 《Science (New York, N.Y.)》2004,303(5655):181-182
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