1970
DOI: 10.1111/j.1365-246x.1970.tb06069.x
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Latitude Dependence of the Angular Dispersion of the Geomagnetic Field

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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Cited by 273 publications
(264 citation statements)
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“…Although I and k can be used to compare different segments of the KM-3 record, it is the angular dispersion of poles (33 that is used to compare individual SV records with global averages of field behavior. This was done following Cox [1970] assuming that the poles are Fisherian distributed.…”
Section: Discussionmentioning
confidence: 99%
“…Although I and k can be used to compare different segments of the KM-3 record, it is the angular dispersion of poles (33 that is used to compare individual SV records with global averages of field behavior. This was done following Cox [1970] assuming that the poles are Fisherian distributed.…”
Section: Discussionmentioning
confidence: 99%
“…The angular standard deviation of poles (ASD) has often been used to monitor paleosecular variation [Cox, 1970] …”
Section: Comparison With Earlier Studymentioning
confidence: 99%
“…Cox (1962) and CREER (1962) proposed the model C including the dipole wobble and nondipole fields on the basis of the present field. Cox (1970) provided the model D in which the latitude dependence of angular dispersions is induced by a wobble of geocentric dipole, sinusoidal oscillation of its intensity, and nondipole fields oriented randomly with variable intensities. MCELHINNY and MERRILL (1975) compiled the world-wide data and provided further discussion on the latitude dependence of angular dispersion during the past 5 Ma.…”
Section: Introductionmentioning
confidence: 99%