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Latitude Dependence of the Angular Dispersion of the Geomagnetic Field

1970/08/01 by Allan Cox · 3 citations
Biochemistry, Genetics and Molecular Biology · Earth and Planetary Sciences · Mathematics · #Geomagnetism and Paleomagnetism Studies #Geophysical and Geoelectrical Methods #Geophysics and Gravity Measurements #Earth's magnetic field #Latitude #Dipole #Geophysics #Geomagnetic pole #Ionospheric dynamo region #Magnetic dipole #Geomagnetic secular variation #Field (mathematics) #Dipole model of the Earth's magnetic field #Intensity (physics) #Geology #Physics #Geodesy #Secular variation #Ring current #Magnetic field #Optics #Interplanetary magnetic field #Solar wind #Geomagnetic storm #Mathematics

paper · doi:10.1111/j.1365-246x.1970.tb06069.x

openalex publication_date 1970/08/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/22

Abstract

Changes in the direction of the Earth's magnetic field at a given site are produced in part by wobble of the main geomagnetic dipole, in part by fluctuations in the intensity and direction of the non-dipole field, and in part by changes in the intensity of the main dipole field. These three processes combine to produce an angular variance that is strongly latitude dependent. A method is presented for isolating the contribution due to variation with latitude of the average intensity of the non-dipole field.

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