An efficient method for computing the eigenfunctions of the dynamo equation

Schrinner, M.; Schmitt, D.; Jiang, J.; Hoyng, P.

doi:10.1051/0004-6361/200913702

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Journal Article

An efficient method for computing the eigenfunctions of the dynamo equation

MPS-Authors

/persons/resource/persons104194

Schrinner, M.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104193

Schmitt, D.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons103991

Jiang, J.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Schrinner, M., Schmitt, D., Jiang, J., & Hoyng, P. (2010). An efficient method for computing the eigenfunctions of the dynamo equation. Astronomy and Astrophysics, 519: A80. doi:10.1051/0004-6361/200913702.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-05B4-2

Abstract

There is no abstract available