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Nakamura, Takasumi, Tajika, Eiichi (2003) Climate change of Mars-like planets due to obliquity variations: implications for Mars. Geophysical Research Letters, 30 (13) doi:10.1029/2002gl016725

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Reference TypeJournal (article/letter/editorial)
TitleClimate change of Mars-like planets due to obliquity variations: implications for Mars
JournalGeophysical Research Letters
AuthorsNakamura, TakasumiAuthor
Tajika, EiichiAuthor
Year2003 (July)Volume30
Issue13
PublisherAmerican Geophysical Union (AGU)
DOIdoi:10.1029/2002gl016725Search in ResearchGate
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Mindat Ref. ID806437Long-form Identifiermindat:1:5:806437:4
GUID0
Full ReferenceNakamura, Takasumi, Tajika, Eiichi (2003) Climate change of Mars-like planets due to obliquity variations: implications for Mars. Geophysical Research Letters, 30 (13) doi:10.1029/2002gl016725
Plain TextNakamura, Takasumi, Tajika, Eiichi (2003) Climate change of Mars-like planets due to obliquity variations: implications for Mars. Geophysical Research Letters, 30 (13) doi:10.1029/2002gl016725
In(2003, July) Geophysical Research Letters Vol. 30 (13) American Geophysical Union (AGU)

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Kurahashi-Nakamura, Takasumi, Tajika, Eiichi (2006) Atmospheric collapse and transport of carbon dioxide into the subsurface on early Mars. Geophysical Research Letters, 33 (18) doi:10.1029/2006gl027170
Nakamura, Takasumi, Tajika, Eiichi (2001) Stability and evolution of the climate system of Mars. Earth, Planets and Space, 53 (8) 851-859 doi:10.1186/bf03351682
Nakamura, Takasumi, Tajika, Eiichi (2002) Stability of the Martian climate system under the seasonal change condition of solar radiation. Journal of Geophysical Research: Planets, 107. 4 doi:10.1029/2001je001561
Spada, Giorgio, Alfonsi, Laura (1998) Obliquity variations due to climate friction on Mars: Darwin versus layered models. Journal of Geophysical Research: Planets, 103. 28599-28605 doi:10.1029/98je02495
Parry Rubincam, David (1999) Mars secular obliquity change due to water ice caps. Journal of Geophysical Research: Planets, 104. 30765-30771 doi:10.1029/1999je001045
Tajika, Eiichi, Sasaki, Sho (1996) Magma generation on Mars constrained from an40Ar degassing model. Journal of Geophysical Research: Planets, 101. 7543-7554 doi:10.1029/95je03863
Rubincam, David Parry (1992) Mars secular obliquity change due to the seasonal polar caps. Journal of Geophysical Research, 97. 2629 doi:10.1029/91je03119
Jenkins, Gregory S. (2001) High-obliquity simulations for the Archean Earth: Implications for climatic conditions on early Mars. Journal of Geophysical Research: Planets, 106. 32903-32913 doi:10.1029/2000je001427
Bills, Bruce G. (1999) Obliquity-oblateness feedback on Mars. Journal of Geophysical Research: Planets, 104. 30773-30797 doi:10.1029/1999je001057
Kreslavsky, M. A., Head, J. W. (2003) North-south topographic slope asymmetry on Mars: Evidence for insolation-related erosion at high obliquity. Geophysical Research Letters, 30 (15) doi:10.1029/2003gl017795
Golombek, M. P., Bridges, N. T. (2000) Erosion rates on Mars and implications for climate change: Constraints from the Pathfinder landing site. Journal of Geophysical Research: Planets, 105. 1841-1853 doi:10.1029/1999je001043
 
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