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dc.contributor.authorReilly, TA
dc.contributor.authorRaja, PKS
dc.contributor.authorMussett, AE
dc.contributor.authorBrock, A
dc.date.accessioned2014-04-29T07:16:23Z
dc.date.available2014-04-29T07:16:23Z
dc.date.issued1976-06
dc.identifier.citationGeophysical Journal of the Royal Astronomical Society Volume 45, Issue 3, pages 483–494, June 1976en_US
dc.identifier.urihttp://onlinelibrary.wiley.com/doi/10.1111/j.1365-246X.1976.tb06906.x/abstract
dc.identifier.urihttp://hdl.handle.net/11295/66133
dc.description.abstractPalaeomagnetic results from 246 sites in the East African Cenozoic volcanics are reported. Palaeomagnetic pole positions are obtained for different age ranges as follows: 0–1.8 My, 104° E, 89° N, A95= 3° (54 sites); 1.8–7.0 My, 148° E, 87° N, A95= 2° (102 sites); around 12 My, 187° E, 87° N, A95= 6° (22 sites); around 17 My, 163° E, 85° N, A95= 2° (62 sites). Apart from the youngest these poles show a far-sided and right-handed tendency which is ascribed to a late Tertiary offset dipole field rather than to polar wander. For at least the past 7 My and possibly for the past 13 My, secular variation in East Africa has been large and in accord with model predictions for near equatorial sites. This contrasts with low secular variation observed in Iavas younger than 5 My from the Hawaiian Islands.en_US
dc.language.isoenen_US
dc.publisherUniversity of Nairobien_US
dc.titleThe Palaeomagnetism of Late Cenozoic Volcanic Rocks from Kenya and Tanzaniaen_US
dc.typeArticleen_US


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