1997
DOI: 10.1029/97jb00624
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Structure and origin of the 85°E ridge

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Cited by 59 publications
(26 citation statements)
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“…The crustal model also suggests that the 85 • E Ridge and sedimentary load over the ridge are compensated by the regional flexure of the Moho boundary (figure 4). This observation is not in agreement with the earlier interpretations of the ridge structure (Liu et al 1982;Mukhopadhyay and Krishna 1991;Ramana et al 1997;Subrahmanyam et al 1999;Anand et al 2009), wherein they favoured the Airy model of isostatic compensation for the 85 • E Ridge. Subrahmanyam et al (1999) have considered underplated magmatic material within the deep crust beneath the ridge in order to explain the negative gravity field satisfactorily; this led to believe that the 85 • E Ridge was formed by a hotspot on young oceanic crust similar to the cases of emplacement of the Ninetyeast and Chagos-Laccadive ridges.…”
Section: Structure and Tectonics Of The 85 • E Ridgecontrasting
confidence: 76%
See 1 more Smart Citation
“…The crustal model also suggests that the 85 • E Ridge and sedimentary load over the ridge are compensated by the regional flexure of the Moho boundary (figure 4). This observation is not in agreement with the earlier interpretations of the ridge structure (Liu et al 1982;Mukhopadhyay and Krishna 1991;Ramana et al 1997;Subrahmanyam et al 1999;Anand et al 2009), wherein they favoured the Airy model of isostatic compensation for the 85 • E Ridge. Subrahmanyam et al (1999) have considered underplated magmatic material within the deep crust beneath the ridge in order to explain the negative gravity field satisfactorily; this led to believe that the 85 • E Ridge was formed by a hotspot on young oceanic crust similar to the cases of emplacement of the Ninetyeast and Chagos-Laccadive ridges.…”
Section: Structure and Tectonics Of The 85 • E Ridgecontrasting
confidence: 76%
“…Though many subsequent researchers favoured the hotspot activity for the emplacement of the ridge (Müller et al 1993;Gopala Rao et al 1997;Subrahmanyam et al 1999;Krishna 2003;Bastia et al 2010;Radhakrishna et al 2010;Michael and Krishna 2011), the source of the hotspot volcanism remains speculative. Alternatively, formation of the ridge due to shearing or sagging of crust by horizontal stretching/compressional forces has been proposed by others (Ramana et al 1997;Anand et al 2009). Following the analogy of the negative gravity signature of the Laxmi Ridge in the Arabian Sea and its continental sliver interpretation (Naini and Talwani 1983;Talwani and Reif 1998;Krishna et al 2006), one can also think in the direction of continental origin to the 85 • E Ridge.…”
Section: Introductionmentioning
confidence: 94%
“…Subrahmanyam et al (2001) modeled the strong gravity low associated with the submerged 85 • E Ridge and convincingly attributed it to a depression-like structure in the Moho, created by the volcanic load of the ridge which has as much density as that of the oceanic crust. The proposition of Subrahmanyam et al (2001) differed from the other interpretations which attributed the strong gravity low of the 85 • E Ridge to several anomaly sources, viz., thickening of the crust beneath the ridge on account of the isostatic compensation (Liu et al 1982;Gopala Rao et al 1997;Subrahmanyam et al 1999), an up-warped model of the ridge with a low-density crust and a shallow root (Ramana et al 1997) and combined sources of meta-sediments having high densities against the volcanic material, and flexure at Moho boundary due to volcanic load of the ridge (Krishna 2003). Subrahmanyam et al (2001) have also opined that each gravity low in the Bay of Bengal should be associated with a structural high like feature as in the case of 85 • E Ridge, and need to be explained by a corresponding flexure in the mantle.…”
Section: Introductionmentioning
confidence: 99%
“…• E Ridge running parallel to the Ninetyeast Ridge and almost buried under the sediments of Bengal fan, evolved due to the interaction of the Indian plate with the Crozet hotspot (Curray and Munashinghe, 1991;Ramana et al, 1997;Subrahmanyam et al, 1999). The extended chain of submarine volcanic islands, ChagosLacadive ridge system, in the western margin and stretching to the proximity of central Indian Ocean, define the track of the Reunion hotspot.…”
Section: Geology and Tectonicsmentioning
confidence: 99%