Suite à une grève chez bpost il est possible que les livraisons connaissent des délais de livraison plus longs de coutume. Besoin de quelque chose en urgence ? Passez plutôt dans un magasin Club à proximité.
- Retrait gratuit dans votre magasin Club
- 7.000.000 titres dans notre catalogue
- Payer en toute sécurité
- Toujours un magasin près de chez vous
Suite à une grève chez bpost il est possible que les livraisons connaissent des délais de livraison plus longs de coutume. Besoin de quelque chose en urgence ? Passez plutôt dans un magasin Club à proximité.
- Retrait gratuit dans votre magasin Club
- 7.000.0000 titres dans notre catalogue
- Payer en toute sécurité
- Toujours un magasin près de chez vous
Magnetic Coupling Between the Interior and Atmosphere of the Sun
421,95 €
+ 843 points
Description
Solar physics in India has a tradition that can be traced to the setting up of the Kodaikanal Observatory in 1899 when the Madras Observatory was relocated to a high altitude site with a view to initiate observations of the sun. This conference on Magnetic Coupling between the Interior and the Atmosphere of the Sun during 2-5 December 2008 was planned to coincide with centenary of the Evershed effect discovery at Kodaikanal in 1909. The aim of this meeting was to bring to a critical focus a comprehensive - derstanding of the important issues pertaining to solar magnetism with particular emphasis on the various MHD processes that operate in the solar atmosphere. The current status of magnetic eld measurements and their implications in the light of recenttheoriesandnumericalmodelingthataddressthe fundamentalscalesandp- cessesinthehighlymagnetizedturbulentplasmawerereviewedduringthismeeting. The meeting was timely for the following reasons: Space observations such as from SOHO and TRACE have provided a wealth of multiwavelength observations onprocessesoccurringinregionsofthe atmosphereextendingfromthe photosphere up to the outer corona. With the launch of Hinode and STEREO in 2006 and of SDO (Solar Dynamics Observatory) shortly, this conference provided a platform for in-depth discussions on new results from various space missions as well as a comparison with ground-based observing facilities such as the Swedish 1-m Solar Telescope. Using sophisticated image processing techniques, such telescopes r- tinelygenerateobservationswitharesolutionbetterthan0. 1arcsec, therebyyielding more informative diagnostics for instance of the microstructure of ux tubes.
Spécifications
Parties prenantes
- Editeur:
Contenu
- Nombre de pages :
- 538
- Langue:
- Anglais
- Collection :
Caractéristiques
- EAN:
- 9783642262746
- Date de parution :
- 04-05-12
- Format:
- Livre broché
- Format numérique:
- Trade paperback (VS)
- Dimensions :
- 152 mm x 229 mm
- Poids :
- 793 g
