Simulation of Solar Magneto-Convection

Robert Cameron (), Alexander Vögler () and Manfred Schüssler ()
Additional contact information
Robert Cameron: Max-Planck-Institut für Sonnensystemforschung
Alexander Vögler: Max-Planck-Institut für Sonnensystemforschung
Manfred Schüssler: Max-Planck-Institut für Sonnensystemforschung

A chapter in High Performance Computing in Science and Engineering, Munich 2004, 2005, pp 431-441 from Springer

Abstract: Abstract We describe the methods for realistic three-dimensional, time-dependent simulations of the interaction between convective flows, magnetic field and radiation near the visible solar surface and show some results recent of our computations: 1) the formation of magnetic patterns and small-scale intense magnetic fields for different amount of magnetic flux in the computational domain and, 2) the structure and dynamics of a larger flux concentration, a so-called pore. Experiences with running our code on the Hitachi SR80000 of HLRB are briefly described.

Keywords: Convection Zone; Colour Version; Radiative Transfer Equation; Solar Photosphere; Convective Energy Transport (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:978-3-540-26657-0_41

Ordering information: This item can be ordered from
http://www.springer.com/9783540266570

DOI: 10.1007/3-540-26657-7_41

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 ().