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Planetary Magnetic Fields and Climate Evolution
DOI: 10.2458/azu_uapress_9780816530595-ch020 Bibcode: 2013cctp.book..487B

Luhmann, J. G.; Leblanc, F.; Brain, D. A. +2 more

2013 Comparative Climatology of Terrestrial Planets
VenusExpress 13
Atmospheric Escape and Climate Evolution of Terrestrial Planets
DOI: 10.2458/azu_uapress_9780816530595-ch023 Bibcode: 2013cctp.book..567T

Leblanc, F.; Brain, D.; Chassefière, E. +1 more

2013 Comparative Climatology of Terrestrial Planets
VenusExpress 11
Chemistry of the Atmospheres of Mars, Venus, and Titan
DOI: 10.2458/azu_uapress_9780816530595-ch011 Bibcode: 2013cctp.book..231K

Lefèvre, F.; Krasnopolsky, V. A.

2013 Comparative Climatology of Terrestrial Planets
VenusExpress 10
Global Climate Models of the Terrestrial Planets
DOI: 10.2458/azu_uapress_9780816530595-ch010 Bibcode: 2013cctp.book..213F

Forget, F.; Lebonnois, S.

2013 Comparative Climatology of Terrestrial Planets
VenusExpress 8
The Atmosphere and Climate of Venus
DOI: 10.2458/azu_uapress_9780816530595-ch002 Bibcode: 2013cctp.book...19B

Bullock, Mark A.; Grinspoon, David H.

Venus lies just sunward of the inner edge of the Sun's habitable zone. Liquid water is not stable. Like Earth and Mars, Venus probably accreted at least an ocean's worth of water, although there are alternative scenarios. The loss of this water led to the massive, dry CO2 atmosphere, extensive H2SO4 clouds (at least some of the time), and an inten…

2013 Comparative Climatology of Terrestrial Planets
VenusExpress 7
Clouds and Aerosols on the Terrestrial Planets
DOI: 10.2458/azu_uapress_9780816530595-ch013 Bibcode: 2013cctp.book..329E

Kahre, M. A.; Esposito, L. W.; Colaprete, A. +2 more

2013 Comparative Climatology of Terrestrial Planets
VenusExpress 0