| Issue |
|
EAS Publications Series
Volume 21,
2006
Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
|
|
Page(s)
|
|
221 - 240 |
| DOI |
|
10.1051/eas:2006115 |
| Published online |
|
07 June 2006 |
|
Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars
M. Rieutord and B. Dubrulle (eds)
EAS Publications Series, 21 (2006) 221-240DOI: 10.1051/eas:2006115
Observations of the solar surface dynamics
N. Meunier Laboratoire d'Astrophysique de l'Observatoire Midi-Pyrénées, 57 avenue d'Azereix, BP. 826, 65008 Tarbes Cedex, France
Abstract
The dynamics of solar and stellar surfaces is very important to understand the dynamics
of their interior as well as their activity cycles. This paper describes the
dynamics observed at the solar surface from small scales (granulation) to the largest
scales (differential rotation and meridional circulation).
© EAS, EDP Sciences 2006
The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link containsarticle metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means:
- if your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages,
- you can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library,
- you can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.