1985
DOI: 10.1038/316623a0
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Absolute motion and evolution of the Bouvet triple junction

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Cited by 12 publications
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“…In fact, the ridge axes can always evolve with azimuths consistent with the orthogonal spreading of rigid plates on a sphere. Thus the "instability" Apotria and Gray [1985] propose never exists, much less increases, for the RRR TJ geometry.…”
Section: Introductionmentioning
confidence: 87%
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“…In fact, the ridge axes can always evolve with azimuths consistent with the orthogonal spreading of rigid plates on a sphere. Thus the "instability" Apotria and Gray [1985] propose never exists, much less increases, for the RRR TJ geometry.…”
Section: Introductionmentioning
confidence: 87%
“…But first, we address a previous attempt at explaining the observation. Apotria and Gray [1985] proposed a solution based on the increasing "instability" of the RRR configuration with time as the location of the TJ migrates in a reference frame tied to the Euler poles of rotation of the plates. Using the Minster and Jordan [1978] plate motions, they calculated that for the Bouvet TJ a RRR TJ would migrate about 15 mm/yr to the northwest and a RFF TJ would migrate about 6 mm/yr to the southeast in the hotspot reference frame.…”
Section: Introductionmentioning
confidence: 99%