Towards understanding the climate of Venus : applications of terrestrial models to our sister planet

ESA s Venus Express Mission has monitored Venus since April 2006, and scientists worldwide have used mathematical models to investigate its atmosphere and model its circulation. This book summarizes recent work to explore and understand the climate of the planet through a research program under the...

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Detaylı Bibliyografya
Yazar: Bengtsson, Lennart O., 1935-
Diğer Yazarlar: Bengtsson, Lennart (Yayın yönetmeni), Bonnet, Roger-Maurice, 1937-2026, astrophysicien (Yayın yönetmeni), Grinspoon, David (Yayın yönetmeni), Koumoutsaris, Symeon (Yayın yönetmeni), Lebonnois, Sebastien (Yayın yönetmeni), Titov, Dmitri (Yayın yönetmeni)
Materyal Türü: Livre numérique
Dil:Anglais
Baskı/Yayın Bilgisi: New York, NY : Springer New York 2013.
Cham : Springer Nature
Seri Bilgileri:ISSI Scientific Report Series 11
Online Erişim:Accès sur la plateforme de l'éditeur
Accès sur la plateforme Istex
Accès Université d'Orléans
Accès INSA CVL
Not: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Edition sous un autre format:• Towards Understanding the Climate of Venus, Texte imprimé, 9781461450658
• Towards Understanding the Climate of Venus, Texte imprimé, 9781489988102
• Towards understanding the climate of Venus, applications of terrestrial models to our sister planet, Lennart Bengtsson, Roger-Maurice Bonnet, David Grinspoon ... [et al.], editors, 2013, New York, Springer, 1 vol. (VIII-185 p.), ISSI scientific report, 978-1-4614-5063-4
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100 1 |a Bengtsson, Lennart O.,  |d 1935- 
245 1 0 |a Towards understanding the climate of Venus :  |b applications of terrestrial models to our sister planet   |c edited by Lennart Bengtsson, Roger-Maurice Bonnet, David Grinspoon, Symeon Koumoutsaris, Sebastien Lebonnois, Dmitri Titov. 
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505 0 |a History of Venus Observation -- The Surface and Atmosphere of Venus: Evolution and Present State -- Radiative Energy Balance in the Venus Atmosphere -- Atmospheric Circulation and Dynamics -- The Dynamics and Circulation of Venus Atmosphere -- Modeling Effects -- Models of Venus Atmosphere -- Comparing Earth and Venus -- Future Prospects. 
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520 |a ESA s Venus Express Mission has monitored Venus since April 2006, and scientists worldwide have used mathematical models to investigate its atmosphere and model its circulation. This book summarizes recent work to explore and understand the climate of the planet through a research program under the auspices of the International Space Science Institute (ISSI) in Bern, Switzerland. Some of the unique elements that are discussed are the anomalies with Venus surface temperature (the huge greenhouse effect causes the surface to rise to 460ů, without which would plummet as low as -40ů), its unusual lack of solar radiation (despite being closer to the Sun, Venus receives less solar radiation than Earth due to its dense cloud cover reflecting 76% back) and the juxtaposition of its atmosphere and planetary rotation (wind speeds can climb up to 200 m/s, much faster than Venus sidereal day of 243 Earth-days). 
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700 1 |a Koumoutsaris, Symeon.  |4 pbd 
700 1 |a Lebonnois, Sebastien.  |4 pbd 
700 1 |a Titov, Dmitri.  |4 pbd 
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