Numerical Modelling of Convection and Dynamo Processes in Fully Convective Stars

Wolfgang Dobler ()
Additional contact information
Wolfgang Dobler: Kiepenheuer-Institut für Sonnenphysik

A chapter in High Performance Computing in Science and Engineering’ 04, 2005, pp 39-45 from Springer

Abstract: Abstract In the current project, we simulate thermal convection and generation of magnetic fields inside a fully convective star, like an M-dwarf or a T-tauri star. The numerical resolution required to reasonably well describe convection properties inside the star is 2563 to 5123.

Keywords: Magnetic Field; Differential Rotation; Meridional Circulation; Protoplanetary Disc; Stellar Surface (search for similar items in EconPapers)
Date: 2005
References: Add references at CitEc
Citations:

There are no downloads for this item, see the EconPapers FAQ for hints about obtaining it.

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:spr:sprchp:978-3-540-26589-4_5

Ordering information: This item can be ordered from
http://www.springer.com/9783540265894

DOI: 10.1007/3-540-26589-9_5

Access Statistics for this chapter

More chapters in Springer Books from Springer
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().