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The outer core rotation about an inclined axis from geomagnetic secular variations (Mitteilungen des Zentralinstituts für Physik der Erde, Nr. 1832)
Author(s) -
GreinerMai H.
Publication year - 1990
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/asna.2113110519
Subject(s) - physics , earth's magnetic field , rotation (mathematics) , dynamo , geomagnetic pole , rotational symmetry , outer core , earth's rotation , dynamo theory , dipole , inner core , core (optical fiber) , secular variation , excitation , classical mechanics , geometry , magnetic field , geophysics , mechanics , optics , quantum mechanics , mathematics
Non‐axisymmetric motions of the outer core of the Earth are important for the dynamo problem and the excitation of the decade variations of the polar motion. The components of the vector of a rigid rotation of the outer core about an inclined axis were estimated by a first‐order approximation of the frozen‐ field theory of the geomagnetic secular variation from 1903.5 to 1975.5. The trends and quasi‐periodic constituents of these quantities were computed. It was shown that the position and time behaviour of the rotational pole of the outer core differ considerably from the well‐know co‐ordinates of the dipole axis. Some periods of the equatorial components of the rotational vector are comparable with those of the axial component previously derived for a pure axial rotation. Additionally, the time behaviour of the pole path shows events like the well‐known Markowitz wobble but naturally with other extent. These and other results suggested that the investigations are worth to be continued in future by some physical interpretations.