Dynamics of polar reversals in spherical dynamos

Pascal Chossat, Hans Armbruster

Research output: Contribution to journalArticle

7 Citations (Scopus)

Abstract

Structurally stable heteroclinic cycles (SSHCs) are proposed as the mathematical structures that are responsible for the reversals of dipolar magnetic fields in spherical dynamos. The existence of SSHCs involving dipolar magnetic fields generated by convection in a spherical shell for a non-rotating sphere is rigorously proven. The possibility of SSHCs in a rotating shell is proposed, and their existence in a low-dimensional model of the magnetohydrodynamic equations is numerically confirmed. The resulting magnetic time-series shows a dipolar magnetic field, aligned with the rotation axis that intermittently becomes unstable, changes the polar axis, starts rotating, disappears completely and eventually re-establishes itself in its original or opposite direction, chosen randomly.

Original languageEnglish (US)
Pages (from-to)577-596
Number of pages20
JournalProceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences
Volume459
Issue number2031
DOIs
StatePublished - Mar 8 2003

Fingerprint

DC generators
Heteroclinic Cycle
rotating generators
Reversal
Magnetic Field
Magnetic fields
cycles
Rotating
magnetic fields
Magnetohydrodynamic Equations
Spherical Shell
spherical shells
Magnetohydrodynamics
magnetohydrodynamics
Convection
Time series
Shell
convection
Unstable
Model

Keywords

  • Heteroclinic cycles
  • Reversals
  • Spherical dynamos

ASJC Scopus subject areas

  • General

Cite this

Dynamics of polar reversals in spherical dynamos. / Chossat, Pascal; Armbruster, Hans.

In: Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 459, No. 2031, 08.03.2003, p. 577-596.

Research output: Contribution to journalArticle

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