about
The abundances of constituents of Titan's atmosphere from the GCMS instrument on the Huygens probeChemical dynamics of triacetylene formation and implications to the synthesis of polyynes in Titan's atmosphere.The two-box model of climate: limitations and applications to planetary habitability and maximum entropy production studiesMethane storms on Saturn's moon Titan.Theoretical study of the C6H3 potential energy surface and rate constants and product branching ratios of the C2H(2Sigma+) + C4H2(1Sigma(g)+) and C4H(2Sigma+) + C2H2(1Sigma(g)+) reactions.Evolution of Titan and implications for its hydrocarbon cycle.The landscape of Titan as witness to its climate evolutionAre the basins of Titan's Hotei Regio and Tui Regio sites of former low latitude seas?Wind-driven surface waves on Titan
P2860
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P2860
description
1997 nî lūn-bûn
@nan
1997年の論文
@ja
1997年論文
@yue
1997年論文
@zh-hant
1997年論文
@zh-hk
1997年論文
@zh-mo
1997年論文
@zh-tw
1997年论文
@wuu
1997年论文
@zh
1997年论文
@zh-cn
name
Photochemically driven collapse of Titan's atmosphere.
@en
type
label
Photochemically driven collapse of Titan's atmosphere.
@en
prefLabel
Photochemically driven collapse of Titan's atmosphere.
@en
P1433
P1476
Photochemically driven collapse of Titan's atmosphere.
@en
P2093
P304
P356
10.1126/SCIENCE.275.5300.642
P407
P577
1997-01-01T00:00:00Z