The evolution of a magnetic field subject to Taylor’s constraint using a projection operator

Author： Livermore Philip W.   Ierley Glenn   Jackson Andrew  

Publisher： Oxford University Press

ISSN： 0956-540X

Source： Geophysical Journal International, Vol.187, Iss.2, 2011-11, pp. : 690-704

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Evolution of non-linear α 2 -dynamos and taylor's constraint

By Fearn D.R.   Rahman M.M.  

Geophysical and Astrophysical Fluid Dynamics, Vol. 98, Iss. 5, 2004-10 ,pp. : 385-406

Taylor & Francis Ltd

Access to resources Recommend Favorite

On the modified Taylor constraint

By  

Geophysical and Astrophysical Fluid Dynamics, Vol. 108, Iss. 6, 2014-11 ,pp. : 696-715

Taylor & Francis Ltd

Access to resources Recommend Favorite

Core surface magnetic field evolution 2000–2010

By Finlay C. C.   Jackson A.   Gillet N.   Olsen N.  

Geophysical Journal International, Vol. 189, Iss. 2, 2012-05 ,pp. : 761-781

Oxford University Press

Access to resources Recommend Favorite

Structure and evolution of the solar coronal magnetic field

By Aly J. J.  

Geophysical and Astrophysical Fluid Dynamics, Vol. 101, Iss. 3-4, 2007-06 ,pp. : 249-287

Taylor & Francis Ltd

Access to resources Recommend Favorite

Torque balance, Taylor's constraint and torsional oscillations in a numerical model of the geodynamo

By Dumberry M.   Bloxham J.  

Physics of the Earth and Planetary Interiors, Vol. 140, Iss. 1, 2003-11 ,pp. : 29-51

Elsevier

Access to resources Recommend Favorite