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Автор Paul Lorrain
Дата выпуска 1993-03-01
dc.description The rotation of the conducting core of the earth in its own magnetic field generates both a v × B field and a competing electrostatic field - ∇V. These two fields together excite toroidal currents, and therefore azimuthal magnetic fields, on the condition that v and B satisfy a certain general condition within the core. Ferraro's law of isorotation is valid, but it concerns a special case. We calculate these azimuthal magnetic fields, first with the core rotating as a solid, and then differentially, with the angular velocity a function of the axial coordinate and a function of the radial coordinate. Our straightforward calculation shows that these azimuthal fields are much weaker than is usually believed. The computer codes are available from the author.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Azimuthal magnetic fields in the Earth's core
Тип paper
DOI 10.1088/0031-8949/47/3/016
Electronic ISSN 1402-4896
Print ISSN 0031-8949
Журнал Physica Scripta
Том 47
Первая страница 461
Последняя страница 468
Аффилиация Paul Lorrain; Institut de Physique du Globe de Paris, Tour 24-25, Place Jussieu, 75252 Paris Cedex 05, France
Выпуск 3

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