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...
Uloženo v:
| Hlavní autor: | |
|---|---|
| Další autoři: | , , , , , |
| Médium: | Livre numérique |
| Jazyk: | Anglais |
| Vydáno: |
New York, NY :
Springer New York
2013.
Cham : Springer Nature |
| Edice: | ISSI Scientific Report Series
11 |
| On-line přístup: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Poznámka: |
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 |
| Shrnutí: | 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). |
|---|---|
| Popis jednotky: | Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| ISBN: | 9781461450641 |
| ISSN: | 2946-1286 |
| Přístup: | Accès en ligne pour les établissements français bénéficiaires des licences nationales Accès soumis à abonnement pour tout autre établissement Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. chttps://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 |

