Giant Planets of Our Solar System : Atmospheres, Composition, and Structure
This book reviews the current state of knowledge of the atmospheres of the giant gaseous planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are reviewed and their recently observed temperature, composition and cloud structures are contrasted and compared with simp...
Zapisane w:
| 1. autor: | |
|---|---|
| Format: | Livre numérique |
| Język: | Anglais |
| Wydane: |
Berlin, Heidelberg :
Springer Berlin Heidelberg
[20..].
Cham : Springer Nature |
| Wydanie: | Second Edition. |
| Seria: | Astronomy and Planetary Sciences
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| Dostęp online: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Komentarz: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Giant planets of our solar system, atmospheres, composition, and structure, Patrick G. J. Irwin, Second edition, Chichester, Springer, Praxis Publishing, 2009, 1 vol. (XXVII-403 p.), Springer-Praxis books in astronomy and planetary sciences, 978-3-540-85157-8 |
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| 082 | |a 520 | ||
| 082 | |a 500.5 | ||
| 100 | 1 | |a Irwin, Patrick G. J. | |
| 245 | 1 | 0 | |a Giant Planets of Our Solar System : |b Atmospheres, Composition, and Structure |c by Patrick G. J. Irwin. |
| 250 | |a Second Edition. | ||
| 260 | |a Berlin, Heidelberg : |b Springer Berlin Heidelberg. | ||
| 260 | |a Cham : |b Springer Nature, |c [20..]. | ||
| 490 | 0 | |a Astronomy and Planetary Sciences |x 2366-0090 | |
| 500 | |a Archives Springer e-books (Licence nationale) | ||
| 500 | |a Archives Springer e-books (Licence nationale) | ||
| 505 | 1 | |a Formation of the giant planets Evolution processes in outer planet atmospheres Vertical structure of temperature, composition, and clouds Dynamical processes Radiative transfer processes in outer planetary atmospheres Sources of remotely sensed data on the giant planets Future of giant planet observations | |
| 506 | |a Accès en ligne pour les établissements français bénéficiaires des licences nationales | ||
| 506 | |a Accès soumis à abonnement pour tout autre établissement | ||
| 506 | |a Conditions particulières de réutilisation pour les bénéficiaires des licences nationales. https://www.licencesnationales.fr/springer-nature-ebooks-contrat-licence-ln-2017 | ||
| 520 | |a This book reviews the current state of knowledge of the atmospheres of the giant gaseous planets: Jupiter, Saturn, Uranus, and Neptune. The current theories of their formation are reviewed and their recently observed temperature, composition and cloud structures are contrasted and compared with simple thermodynamic, radiative transfer and dynamical models. The instruments and techniques that have been used to remotely measure their atmospheric properties are also reviewed, and the likely development of outer planet observations over the next two decades is outlined. This second edition has been extensively updated following the Cassini mission results for Jupiter/Saturn and the newest ground-based measurements for Uranus/Neptune as well as on the latest development in the theories on planet formation | ||
| 776 | 0 | |0 132700794 |t Giant planets of our solar system |o atmospheres, composition, and structure |f Patrick G. J. Irwin |e Second edition |c Chichester |n Springer |n Praxis Publishing |d 2009 |p 1 vol. (XXVII-403 p.) |s Springer-Praxis books in astronomy and planetary sciences |z 978-3-540-85157-8 | |
| 856 | 4 | |q PDF |u https://doi.org/10.1007/978-3-540-85158-5 |z Accès sur la plateforme de l'éditeur | |
| 856 | 4 | |u https://revue-sommaire.istex.fr/ark:/67375/8Q1-73CR070W-Q |z Accès sur la plateforme Istex | |
| 856 | 4 | |5 452349901:747848297 |u https://ezproxy.univ-orleans.fr/login?url=https://dx.doi.org/10.1007/978-3-540-85158-5 |z Accès Université d'Orléans | |
| 856 | 4 | |5 180339901:750865814 |u https://ezproxy.insa-cvl.fr/login?qurl=https://dx.doi.org/10.1007/978-3-540-85158-5 |z Accès INSA CVL | |
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