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Bouvet triple junction

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Journal Article
Published: 01 May 2025
Russ. Geol. Geophys. (2025) 66 (5): 551–569.
...A.A. Kirdyashkin; V.A. Simonov; A.V. Kotlyarov; A.V. Jakovlev Three midocean ridges meet in the Bouvet triple-junction region: Mid-Atlantic, Southwest Indian, and American–Antarctic. The triple-junction region is indicated by the Bouvet hotspot magmatism. Available laboratory modeling data...
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Journal Article
Published: 01 November 2017
Russ. Geol. Geophys. (2017) 58 (11): 1289–1304.
...N.A. Migdisova; A.V. Sobolev; N.M. Sushchevskaya; E.P. Dubinin; D.V. Kuz’min Abstract Tholeiitic melts from the Bouvet triple junction (BTJ) of rift zones in the South Atlantic are moderately enriched rocks with specific lithophile-element patterns. The high (Gd/Yb) n values (up to 2.5) in some...
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Journal Article
Journal: Geology
Published: 01 March 1998
Geology (1998) 26 (3): 267–270.
... for a transform fault. The junction is therefore neither ridge-fault-fault nor ridge-ridge-ridge. We speculate that growth of Spiess Ridge adjacent to the triple junction has caused this complexity and discuss more generally the origins of distributed deformation at oceanic triple junctions. Geological Society...
Journal Article
Published: 01 December 1997
Russ. Geol. Geophys. (1997) 38 (12): 1963–1970.
...V. A. Simonov; A. S. Lapukhov; A. A. Milosnov; S. V. Kovyazin; R. D. Mel’nikova Investigation of a collection of rocks with ore and hydrothermal minerals gathered during the 18th cruise of the research vessel Akademik Nikolai Strakhov (1994) at the Bouvet Triple Junction provided new data...
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Journal Article
Published: 01 February 1996
Russ. Geol. Geophys. (1996) 37 (2): 78–87.
... of the Bouvet Triple Junction. Three major types of melts are determined: dry melts characterized by minimum contents of H 2 O, K 2 O, and TiO 2 , (N-MORB type); enriched melts with minimum contents of H 2 O (E-MORB type); and enriched melts with maximum contents of CO 2 , K 2 O, and TiO 2 (OIB type...
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Journal Article
Published: 01 October 2023
Russ. Geol. Geophys. (2023) 64 (10): 1251–1261.
...A.A. Kirdyashkin; A.G. Kirdyashkin; V.A. Simonov; M.M. Buslov; A.V. Kotlyarov Abstract —In the Bouvet Island region (South Atlantic), a hotspot operates in the region of the triple junction of midocean ridges. On the basis of laboratory modeling data, the structure of the conduit...
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Bouvet triple-junction region (South Atlantic). 1 – transform faults; 2 – MOR axes; 3 – other faults; 4 – Spiess Ridge; 5 – zero magnetic anomaly zones; 6 – isochrons based on magnetic anomalies (Ma); 7 – isobaths in meters; 8 – dredging stations of the 18th sail of research vessel Akademik Nikolai Strakhov. MAR is the end of the Mid-Atlantic Ridge; AAR is the end of the American–Antarctic deformation zone; the Spiess Ridge is a volcanic uplift, the end of the Southwest Indian Ridge (SWIR). The tectonic scheme is based on modified data from [Pushcharovskii and Peive, 1996; Ligi et al., 1999; Simonov et al., 2000]. The combination of colored elevation and shaded relief image is based on [Ryan et al., 2009] at https://www.gmrt.org/. The inset shows the Antarctic region in a polar stereographic projection, with the South Pole as the central point.
Published: 01 May 2025
Fig. 1. Bouvet triple-junction region (South Atlantic). 1 – transform faults; 2 – MOR axes; 3 – other faults; 4 – Spiess Ridge; 5 – zero magnetic anomaly zones; 6 – isochrons based on magnetic anomalies (Ma); 7 – isobaths in meters; 8 – dredging stations of the 18th sail
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Ocean floor relief in the Bouvet triple-junction region with superposed model trajectories of the Bouvet and Shona hotspots, modified after [Hartnady and le Roex, 1985]. 1 – model tracks of the Bouvet and Shona hotspots [Hartnady and le Roex, 1985], indicated by the black circles dated with a periodicity of 10 Ma; 2 – 1-km isobaths; 3 – 4.5-km isobaths; 4 – Agulhas–Falkland fracture zone (AFFZ); 5 – uplifts and ridges of the South Atlantic; 6 – MAR and SWIR (AfAR) regions; 7 – Bouvet transform fault. The large black circles show the model positions of the Bouvet (B64 and B) and Shona (Sh64 and Sh) hotspots at 64 Ma and at present; the corresponding positions of the Spiess Ridge (Sp64 and Sp) are also marked. The inset indicates the model tracks of the Bouvet (B) and Shona (Sh) hotspots [Morgan, 1983], starting in the south of the South African Platform.
Published: 01 May 2025
Fig. 2. Ocean floor relief in the Bouvet triple-junction region with superposed model trajectories of the Bouvet and Shona hotspots, modified after [ Hartnady and le Roex, 1985 ]. 1 – model tracks of the Bouvet and Shona hotspots [ Hartnady and le Roex, 1985 ], indicated by the black circles
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Diagram showing the Bouvet Triple Junction region with the directions of large-scale cellular free-convective flows as well as the ascending and descending flows of convective rolls in the Bouvet region. 1 – transform faults; 2 – rift valleys of the MOR; 3 – Spiess Ridge; 4 – dredging stations of the 18th cruise of R/V Akademik Nikolai Strakhov; 5 – directions of large-scale asthenospheric flows; 6 – ascending flows of asthenospheric rolls; 7 – descending flows of asthenospheric rolls; A–A, B–B, and C–C are the section lines.
Published: 01 October 2023
Fig. 6. Diagram showing the Bouvet Triple Junction region with the directions of large-scale cellular free-convective flows as well as the ascending and descending flows of convective rolls in the Bouvet region. 1 – transform faults; 2 – rift valleys of the MOR; 3 – Spiess Ridge; 4
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Free-convective flows in the asthenosphere in the Bouvet Triple Junction region. а – Diagram showing the free-convective roll flow (A–A section (Fig. 6)); δ ≈5–8 km – thickness of the oceanic lithosphere; Ltr – distance between the transform faults; L1 ≈60 km – height of asthenospheric convective rolls at the bottom of the oceanic lithosphere; the direction of the roll flow is perpendicular to the direction of the large-scale flow; b – diagram showing the large-scale asthenospheric free-convective flow (B–B section); c – diagram showing the free-convective roll flow and the Bouvet plume interacting with it (С–С section).
Published: 01 October 2023
Fig. 7. Free-convective flows in the asthenosphere in the Bouvet Triple Junction region. а – Diagram showing the free-convective roll flow (A–A section ( Fig. 6 )); δ ≈5–8 km – thickness of the oceanic lithosphere; L tr – distance between the transform faults; L 1 ≈60 km – height
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Bathymetry map of the Bouvet triple junction area. Symbols indicate the location of stations dredged during cruise S18 of the R/V Akademik Strakhov and cruise G96 of the R/V Gelendzhik (G96) (Peyve et al., 1999).
Published: 01 November 2017
Fig. 1. Bathymetry map of the Bouvet triple junction area. Symbols indicate the location of stations dredged during cruise S18 of the R/V Akademik Strakhov and cruise G96 of the R/V Gelendzhik (G96) ( Peyve et al., 1999 ).
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Geochemical characteristics of tholeiites from the Bouvet triple junction area. a, Lithophile element patterns normalized to primitive mantle after Hoffmann (1988); b–g, correlations between the proportions of pyroxenitic component, XPx Mn, and trace incompatible element ratios of BTJ melts. The figure shows average values for each station.
Published: 01 November 2017
Fig. 7. Geochemical characteristics of tholeiites from the Bouvet triple junction area. a , Lithophile element patterns normalized to primitive mantle after Hoffmann ( 1988 ); b–g , correlations between the proportions of pyroxenitic component, X Px Mn, and trace incompatible element ratios
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Compositions of basalts from the vicinity of the Bouvet Triple Junction. 1 – submarine slopes of Bouvet (stations S18-19, 20); 2, 3 – SWIR rift zone (2 – S18-16; 3 – S18-31); 4 – Bouvet Fracture Zone (S18-10); 5–7 – MAR rift zone (5 – southern segment, S18-50, 6 – central segment, S18-53, 7 – northern segment, S18-62, 63); 8 – dredging stations at a distance from the MAR axis (S18-57, 66); 9 – Spiess Ridge (S18-46); 10 – fields: I – tholeiitic, II – subalkaline (II – hawaiites, II2 – mugearites, II3 – benmoreites) and III – alkaline series; 11 – field of hawaiites from the Hawaiian Islands, according to data [17].
Published: 01 February 1996
Fig. 2. Compositions of basalts from the vicinity of the Bouvet Triple Junction. 1 – submarine slopes of Bouvet (stations S18-19, 20); 2 , 3 – SWIR rift zone ( 2 – S18-16; 3 – S18-31); 4 – Bouvet Fracture Zone (S18-10); 5 – 7 – MAR rift zone ( 5 – southern segment, S18-50, 6
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Diagram TiO2–for basalts from the vicinity of the Bouvet Triple Junction. 1 – initial compositions of melt inclusions in olivines from the MAR basalts, 9° N; 2 – primary mantle melt, equilibrated with lherzolite-harzburgite restite; 3 – primary melt, equilibrated with lherzolites; 4–6 – fields; 4 – Spiess Ridge basalts [14], 5 – basalts of E-MORB type from fault zone 15°20′, 6 – melt inclusions in olivines from fracture zone 15°20′ basalts; 7 – trend of N-MORB basalts from fracture zone 15°20′. 1–3 – according to data [18]; 5–7 – according to data of Simonov and Kolobov. See Fig. 2 for other notations.
Published: 01 February 1996
Fig. 3. Diagram TiO 2 –for basalts from the vicinity of the Bouvet Triple Junction. 1 – initial compositions of melt inclusions in olivines from the MAR basalts, 9° N; 2 – primary mantle melt, equilibrated with lherzolite-harzburgite restite; 3 – primary melt, equilibrated with lherzolites
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Real data inversion for the southern segment of the MAR between 50°S and 70°S. a – P-wave anomaly distribution at depths of 100, 200, 300, and 400 km. b – P-wave velocity anomalies in a vertical section through the triple-junction region of the MOR and the Bouvet hotspot. The Bouvet triple-junction region, the tectonic sketch map of which is presented in Fig. 1, is shown by a dotted frame in Fig. 12a in the horizontal section at a depth of 100 km. The section line is shown in red in Fig. 12a. The black dots are earthquake epicenters; the star denotes the Bouvet Island location; B is the Bouvet transform fault; C is the Conrad transform fault; and SWIR is the end of the Southwest Indian Ridge. The axes of the main morphostructures of the Bouvet triple junction are shown as green lines.
Published: 01 May 2025
Fig. 12. Real data inversion for the southern segment of the MAR between 50°S and 70°S. a – P -wave anomaly distribution at depths of 100, 200, 300, and 400 km. b – P -wave velocity anomalies in a vertical section through the triple-junction region of the MOR and the Bouvet hotspot
Series: Geological Society, London, Special Publications
Published: 01 January 2003
DOI: 10.1144/GSL.SP.2003.219.01.16
EISBN: 9781862394674
... the South American-Antarctic Ridge, which connects the Bouvet triple junction to the South Sandwich subduction system. Four samples dredged from segment E2 have 4 He/ 3 He ratios of 85 000–90 200 (8.5–8.0 R/R A , where) R/R A is the 4 He/ 3 He ratio normalized to air) and three wax core samples...
Journal Article
Journal: Geology
Published: 01 May 2013
Geology (2013) 41 (5): 575–578.
... sulfide melt globules highly enriched in noble metals (Pt, Pd, Au; 120 ppm total platinum group elements [PGE]) within an unusual high-Mg andesitic glass (8.2 wt% MgO, 57.3 wt% SiO 2 ) dredged from the southern Mid-Atlantic Ridge, near the Bouvet triple junction. The composition of this glass indicates...
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Journal Article
Journal: Geology
Published: 01 March 2001
Geology (2001) 29 (3): 243–246.
...Vadim S. Kamenetsky; Roland Maas; Nadezhda M. Sushchevskaya; Marc D. Norman; Ian Cartwright; Alexander A. Peyve Abstract Dredged glass from the southern Mid-Atlantic Ridge near the Bouvet Triple Junction has unique major element, trace element, and isotopic composition, distinct from typical mid...
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Relationship between the ocean floor morphostructures with deep-seated geodynamic systems in the Bouvet triple-junction region. a – Diagram showing the relationship of the ocean floor morphostructures with the system of asthenospheric freeconvection flows in the Bouvet triple-junction region; b – diagram showing the asthenospheric free-convection roll flow and the Bouvet plume conduit in the section along line I–I. 1 – MOR; 2 – Spiess Ridge; 3 – transform faults; 4 – directions of free-convection cellular flows in the asthenosphere causing plate motion in the MOR zones; 5 – ascending free-convection roll flows at the top of the asthenosphere; 6 – descending roll flows, 7 – dredging stations. ll is the thickness of the oceanic lithosphere, and lr is the height of asthenospheric rolls.
Published: 01 May 2025
Fig. 10. Relationship between the ocean floor morphostructures with deep-seated geodynamic systems in the Bouvet triple-junction region. a – Diagram showing the relationship of the ocean floor morphostructures with the system of asthenospheric freeconvection flows in the Bouvet triple-junction
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Figure 4. Predicted and observed changes at the Rodriguez and Bouvet triple junctions in response to rate change at the SWIR. A: Location map. The Rodriguez triple junction is to the east where the SWIR meets the CIR and the SEIR. The Bouvet triple junction is to the west where the SWIR meets the SMAR and the SAAR. B: Triple junction velocity triangles predict spreading direction change at the CIR and SAAR, constant plate motion for the SMAR and SEIR assumed. The period A13–A8 is shown in red and A6–A5 in black. C and D: Evidence for plate motion change between A8 and A6 in satellite-derived gravity maps of CIR (C) and SAAR (D). CIR—Central Indian Ridge; SEIR—Southeast Indian Ridge; SWIR—Southwest Indian Ridge; SMAR—Southern Mid-Atlantic Ridge; SAAR—South American–Antarctic Ridge.
Published: 01 March 2008
Figure 4. Predicted and observed changes at the Rodriguez and Bouvet triple junctions in response to rate change at the SWIR. A: Location map. The Rodriguez triple junction is to the east where the SWIR meets the CIR and the SEIR. The Bouvet triple junction is to the west where the SWIR meets