Turbulence, Dynamos, Accretion Disks, Pulsars and Collective Plasma Processes : First Kodai-Trieste Workshop on Plasma Astrophysics Held at the Kodaikanal Observatory Kodaikanal, India, August 27 - September 7, 2007
It is well established and appreciated by now that more than 99% of the baryonic matter in the universe is in the plasma state. Most astrophysical systems could be approximated as conducting fluids in a gravitational field. It is the combined effect of these two that gives rise to the mind boggling...
Enregistré dans:
| Autres auteurs: | , , , , |
|---|---|
| Format: | Livre numérique |
| Langue: | Anglais |
| Publié: |
Dordrecht :
Springer Netherlands : Springer e-books
[20..].
Cham : Springer Nature |
| Collection: | Astrophysics and Space Science Proceedings
|
| Accès en ligne: | Accès sur la plateforme de l'éditeur Accès sur la plateforme Istex Accès Université d'Orléans Accès INSA CVL |
| Note: |
Archives Springer e-books (Licence nationale) Archives Springer e-books (Licence nationale) |
| Autres localisations: | Voir dans le Sudoc |
| Edition sous un autre format: | • Turbulence, dynamos, accretion disks, pulsars and collective plasma processes, First Kodai-Trieste Workshop on Plasma Astrophysics held at the Kodaikanal Observatory, Kodaikanal, India, August 27-September 7, 2007, edited by S. S. Hasan, R. T. Gangadhara, and V. Krishan, 2009, [Berlin], Springer, 1 vol. (XIII-342 p.), Astrophysics and space science proceedings, 978-1-402-08867-4 |