The sun and the heliopsphere [i.e. heliosphere] as an integrated system

This book, for the first time, ties together physical processes across the full scale of the heliosphere. It is about the natural connections that exist between the various parts of the system. Therefore, it is mainly cast in terms of those mechanisms and phenomena rather than individual missions in...

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מחברים אחרים: Poletto, Giannina (Éditeur intellectuel), Suess, Steven T. (Éditeur intellectuel)
פורמט: Livre numérique
שפה:Anglais
יצא לאור: Dordrecht ; Boston : Kluwer [2004].
סדרה:Astrophysics and space science library volume 317
גישה מקוונת:Accès sur la plateforme de l'éditeur
Accès sur la plateforme ISTEX
Accès Université d'Orléans
Accès INSA CVL
הערה: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Edition sous un autre format:• The sun and the heliopsphere [i.e. heliosphere] as an integrated system, edited by Giannina Poletto and Steven T. Suess, Dordrecht, Kluwer Academic, 2004, 1 vol. (XV-422 p.), Astrophysics and space science library, 1-4020-2830-X
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245 1 0 |a The sun and the heliopsphere [i.e. heliosphere] as an integrated system   |c edited by Giannina Poletto and Steven T. Suess. 
260 |a Dordrecht ;  |a Boston :  |b Kluwer,  |c [2004]. 
490 0 |a Astrophysics and space science library  |v volume 317 
500 |a Archives Springer e-books (Licence nationale) 
500 |a Archives Springer e-books (Licence nationale) 
504 |a Includes bibliographical references. 
505 0 |a From the contents: Preface -- 1. Hydrogen Walls: Mass Loss of Dwarf Stars and the Young Sun -- 2. The Heliospheric Interface: Models and Observations -- 3. Radiation from the Outer Heliosphere and Beyond -- 4. Ulysses at Solar Maximum -- 5. Propagation of Energetic Particles to High Latitudes -- 6. Solar Wind Properties from IPS Observations -- 7. The Dynamically Coupled Heliosphere -- 8. A Global Picture of CMEs in the Inner Heliosphere -- 9. MHD Turbulence in the Heliosphere: Evolution and Intermittency -- 10. Waves and Turbulence in the Solar Corona -- 11. The Influence of the Chromosphere -- Corona Coupling on Solar Wind and Heliospheric Parameters -- 12. Elemental Abundances in the Solar Corona -- 13. The Magnetic Field from the Solar Interior to the Heliosphere -- 14. Magnetic Reconnection 
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, for the first time, ties together physical processes across the full scale of the heliosphere. It is about the natural connections that exist between the various parts of the system. Therefore, it is mainly cast in terms of those mechanisms and phenomena rather than individual missions in space. However, to give credit, this has only been possible because of the existence of a fleet of deep space missions such as Ulysses, SOHO, and the Voyagers. It is only with them working in concert that a real understanding of the physics can be, and has been achieved. There are fourteen chapters in the book written by top scientists from around the world. The level of presentation is very high but the authors were given enough space to present understandable introductions, physical discussions, and extensive bibliographies. The audience for this book consists of graduate students and researchers in astronomy as well as specialists in solar physics and interplanetary plasma physics 
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700 1 |a Poletto, Giannina.  |4 edt 
700 1 |a Suess, Steven T.  |4 edt 
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