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    The Role of Upper Mantle Heterogeneity and Plume-Ridge Interaction Along the Central Indian Ridge from 7°S and 18°S : a multidisciplinary investigation based on MORB geochemistry, bathymetry, and gravity analysis = 7°S -18°S 사이 인도양 중앙 해령 지역에서의 상부 맨틀 이질성과 플룸-해령 상호작용의 역할 : 중앙해령 지구화학, 측심 및 중력 분석에 기초한 학제간 연구

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    https://www.riss.kr/link?id=T17110050

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    다국어 초록 (Multilingual Abstract) kakao i 다국어 번역

    The mid-ocean ridges (MOR) are the largest volcanic system on Earth, generating the oceanic lithosphere that covers 65% of the Earth’s surface through seafloor spreading. This phenomenon is due to the tectonic plates moving away from each other, which induces the underlying mantle to rise and melt. The resultant buoyant melt erupts along the ridge axis in the form of mid-oceanic ridge basalts (MORB), and the geochemistry signature of these lavas are an important source of information on the melting conditions and the geochemical characteristics of the less accessible upper mantle. A multitude of parameters such as the spreading rate, the influence of mantle plume on the ridge or even the presence of heterogeneity embedded in the upper mantle may have an impact on morphology and/or geochemistry variations along portions of mid-ocean ridge. Variations of the spreading style, ridge morphology, and MORB geochemical signature will then reflect the nature of the mantle and the upwelling dynamics beneath the ridge. In this dissertation, the geochemical and isotopic signature of MORB sampled along the Central Indian Ridge axis between 8°and 17°S were investigated to better understand the different mantle source melting. The new trace element and isotopic analysis show that the MORB geochemical signature differs between segments along the studied portion of the ridge. The CIR portion between 12°and 17°S, especially the segment between 14°and 16°S show enriched MORB that can be explained by the presence of three mantle end-members: the depleted Indian-type MORB mantle, Réunion Plume, and Seychelles/Madagascar-like continental crust components. Moreover, the geophysical analysis of the enriched segment between 14°and 16°S reveals a correlation between its structural characteristics, gravity anomalies, and MORB enrichment variations. This correlation is best explained by the presence of a fertile heterogeneity in the melting regime which influences the melt production along a portion of this segment delimited by ridge discontinuities. Furthermore, this multidisciplinary analysis suggests that the magmatic accretion occurring along this segment is most certainly following the model of buoyancy-driven focused mantle upwelling. Another portion of the CIR formed by two segments between 8°and 12°S was investigated and their MORB geochemistry highlights the presence of a different enriched mantle component beneath this ridge area. This enriched source has a FOZO-like signature and its presence can be explained by the influence of an asthenospheric anomaly: the Mascarene Basin Asthenosphere Reservoir. Furthermore, it is proposed in this study that this plume-like anomaly is an aborted plume originally linked to a broad upwelling structure rooted in the lower mantle, in the African LLSVP. Thus, this study offers valuable insights into the geodynamics of the Indian Ocean mantle and its impact on MORB geochemistry and spreading processes along the CIR but also about processes affecting MOR in general. Keyword : Central Indian Ridge, Mantle upwelling, Seafloor spreading, Mantle heterogeneity, Mid-ocean ridge basalt, Isotope geochemistry, Ocean floor, Ridge segmentation Student Number : 2017-31049
    번역하기

    The mid-ocean ridges (MOR) are the largest volcanic system on Earth, generating the oceanic lithosphere that covers 65% of the Earth’s surface through seafloor spreading. This phenomenon is due to the tectonic plates moving away from each other, whi...

    The mid-ocean ridges (MOR) are the largest volcanic system on Earth, generating the oceanic lithosphere that covers 65% of the Earth’s surface through seafloor spreading. This phenomenon is due to the tectonic plates moving away from each other, which induces the underlying mantle to rise and melt. The resultant buoyant melt erupts along the ridge axis in the form of mid-oceanic ridge basalts (MORB), and the geochemistry signature of these lavas are an important source of information on the melting conditions and the geochemical characteristics of the less accessible upper mantle. A multitude of parameters such as the spreading rate, the influence of mantle plume on the ridge or even the presence of heterogeneity embedded in the upper mantle may have an impact on morphology and/or geochemistry variations along portions of mid-ocean ridge. Variations of the spreading style, ridge morphology, and MORB geochemical signature will then reflect the nature of the mantle and the upwelling dynamics beneath the ridge. In this dissertation, the geochemical and isotopic signature of MORB sampled along the Central Indian Ridge axis between 8°and 17°S were investigated to better understand the different mantle source melting. The new trace element and isotopic analysis show that the MORB geochemical signature differs between segments along the studied portion of the ridge. The CIR portion between 12°and 17°S, especially the segment between 14°and 16°S show enriched MORB that can be explained by the presence of three mantle end-members: the depleted Indian-type MORB mantle, Réunion Plume, and Seychelles/Madagascar-like continental crust components. Moreover, the geophysical analysis of the enriched segment between 14°and 16°S reveals a correlation between its structural characteristics, gravity anomalies, and MORB enrichment variations. This correlation is best explained by the presence of a fertile heterogeneity in the melting regime which influences the melt production along a portion of this segment delimited by ridge discontinuities. Furthermore, this multidisciplinary analysis suggests that the magmatic accretion occurring along this segment is most certainly following the model of buoyancy-driven focused mantle upwelling. Another portion of the CIR formed by two segments between 8°and 12°S was investigated and their MORB geochemistry highlights the presence of a different enriched mantle component beneath this ridge area. This enriched source has a FOZO-like signature and its presence can be explained by the influence of an asthenospheric anomaly: the Mascarene Basin Asthenosphere Reservoir. Furthermore, it is proposed in this study that this plume-like anomaly is an aborted plume originally linked to a broad upwelling structure rooted in the lower mantle, in the African LLSVP. Thus, this study offers valuable insights into the geodynamics of the Indian Ocean mantle and its impact on MORB geochemistry and spreading processes along the CIR but also about processes affecting MOR in general. Keyword : Central Indian Ridge, Mantle upwelling, Seafloor spreading, Mantle heterogeneity, Mid-ocean ridge basalt, Isotope geochemistry, Ocean floor, Ridge segmentation Student Number : 2017-31049

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    국문 초록 (Abstract) kakao i 다국어 번역

    중앙해령(Mid-Ocean Ridges, MOR)은 지구 표면의 65%를 구성하는 해양 지각을 해저면 확장을 통해 형성하는 지구에서 가장 큰 규모의 화산 활동이다. 이 현상은 지각판들이 서로 멀어지면서 그 아래에 존재하는 맨틀이 상승하여 용융한 결과물이며, 용융된 맨틀 물질은 해령의 축을 따라 중앙해령 현무암(Mid-Ocean Ridge Basalts, MORB)의 형태로 분출된다. 분출된 용암의 지구화학적 특성을 이해하는 것은 다른 방법으로는 접근하기 어려운 상부 맨틀에서의 용융 조건과 지구화학적 특성에 대한 중요한 정보를 제공한다. 판의 확장 속도, 해령에 대한 맨틀 플룸의 영향, 또는 상부 맨틀에 내재된 구성적 이질성과 같은 다양한 요소들이 해령의 일부분에서 그 형태학적 특성 및 지구화학적 변화를 초래할 수 있다. 그러므로 해저 확장의 방식, 해령의 형태학, MORB의 지구화학적 특성은 맨틀과 그 상승 과정의 동역학에 대한 정보를 제공한다.

    이 연구에서는 남위 8°에서 17° 사이의 인도양 중앙해령(Central Indian Ridge, CIR) 을 따라 획득한 MORB의 지구화학적 특성과 및 동위원소 구성을 조사하여 서로 다른 맨틀 근원의 용융을 연구하였다. 새로운 미량 원소와 동위원소 분석 결과는 연구 지역의 해령의 각 구간에서 MORB의 지구화학적 특성이 서로 다르다는 것을 지시한다. 남위 12°에서 17° 사이, 특히 남위 14°에서 16° 사이에 위치한 구역에서는 세 가지 근원맨틀 성분들(결핍된 인도양 MORB 맨틀, 레위니옹 플룸, 세이셸/마다가스카르 대륙 지각)로 설명될 수 있는 부화된 MORB를 확인하였다. 또한, 동 구역에 대한 지구물리학적 연구를 통해 구역의 지구조적 특성, 중력 이상, 그리고 MORB 부화 정도가 가지는 상관 관계를 규명하였다. 이 상관 관계는 해령의 불연속적 단절에 의해 구분되는 구역의 한 구간에서 맨틀 부화도의 이질성이 용융에 미치는 영향에 의해 잘 설명될 수 있다. 더 나아가, 이러한 지구화학 및 지구물리학을 통한 다학제적 분석 결과는 이 구역에서 발생하는 마그마 축적이 주로 부력에 의해 집중된 맨틀 용승 모델을 따르고 있음을 시사한다. 남위 8°에서 12° 사이에서 두 구역으로 나뉘어진 인도양 중앙해령의 또 다른 구간에서의 MORB의 지구화학적 특성은 추가적인 부화된 근원 맨틀 성분의 존재를 나타낸다. 이 부화된 근원 맨틀 성분은 FOZO와 유사한 특성을 가지고 있으며, 이는 연약권 변칙성(마스카렌 분지 연약권 저장소, Mascarene Basin Asthenosphere Reservoir)의 영향으로 설명될 수 있다. 본 연구에서는 이러한 유사-플룸 변칙성이 하부 맨틀에 위치한 아프리카 LLSVP로부터 기원하는 광범위한 상승 구조와 연결된 중단된 플룸 현상이라고 제안한다.

    따라서 이 연구는 인도양 맨틀에서의 지구동역학 및 MORB의 지구화학적 특성에 미치는 영향, 인도양 중앙해령을 따라 일어나는 해저면 확장에 대한 영향 뿐만이 아니라중앙해령에 영향을 미치는 다양한 요소들에 대한 전반적 통찰을 제공한다.
    번역하기

    중앙해령(Mid-Ocean Ridges, MOR)은 지구 표면의 65%를 구성하는 해양 지각을 해저면 확장을 통해 형성하는 지구에서 가장 큰 규모의 화산 활동이다. 이 현상은 지각판들이 서로 멀어지면서 그 아래...

    중앙해령(Mid-Ocean Ridges, MOR)은 지구 표면의 65%를 구성하는 해양 지각을 해저면 확장을 통해 형성하는 지구에서 가장 큰 규모의 화산 활동이다. 이 현상은 지각판들이 서로 멀어지면서 그 아래에 존재하는 맨틀이 상승하여 용융한 결과물이며, 용융된 맨틀 물질은 해령의 축을 따라 중앙해령 현무암(Mid-Ocean Ridge Basalts, MORB)의 형태로 분출된다. 분출된 용암의 지구화학적 특성을 이해하는 것은 다른 방법으로는 접근하기 어려운 상부 맨틀에서의 용융 조건과 지구화학적 특성에 대한 중요한 정보를 제공한다. 판의 확장 속도, 해령에 대한 맨틀 플룸의 영향, 또는 상부 맨틀에 내재된 구성적 이질성과 같은 다양한 요소들이 해령의 일부분에서 그 형태학적 특성 및 지구화학적 변화를 초래할 수 있다. 그러므로 해저 확장의 방식, 해령의 형태학, MORB의 지구화학적 특성은 맨틀과 그 상승 과정의 동역학에 대한 정보를 제공한다.

    이 연구에서는 남위 8°에서 17° 사이의 인도양 중앙해령(Central Indian Ridge, CIR) 을 따라 획득한 MORB의 지구화학적 특성과 및 동위원소 구성을 조사하여 서로 다른 맨틀 근원의 용융을 연구하였다. 새로운 미량 원소와 동위원소 분석 결과는 연구 지역의 해령의 각 구간에서 MORB의 지구화학적 특성이 서로 다르다는 것을 지시한다. 남위 12°에서 17° 사이, 특히 남위 14°에서 16° 사이에 위치한 구역에서는 세 가지 근원맨틀 성분들(결핍된 인도양 MORB 맨틀, 레위니옹 플룸, 세이셸/마다가스카르 대륙 지각)로 설명될 수 있는 부화된 MORB를 확인하였다. 또한, 동 구역에 대한 지구물리학적 연구를 통해 구역의 지구조적 특성, 중력 이상, 그리고 MORB 부화 정도가 가지는 상관 관계를 규명하였다. 이 상관 관계는 해령의 불연속적 단절에 의해 구분되는 구역의 한 구간에서 맨틀 부화도의 이질성이 용융에 미치는 영향에 의해 잘 설명될 수 있다. 더 나아가, 이러한 지구화학 및 지구물리학을 통한 다학제적 분석 결과는 이 구역에서 발생하는 마그마 축적이 주로 부력에 의해 집중된 맨틀 용승 모델을 따르고 있음을 시사한다. 남위 8°에서 12° 사이에서 두 구역으로 나뉘어진 인도양 중앙해령의 또 다른 구간에서의 MORB의 지구화학적 특성은 추가적인 부화된 근원 맨틀 성분의 존재를 나타낸다. 이 부화된 근원 맨틀 성분은 FOZO와 유사한 특성을 가지고 있으며, 이는 연약권 변칙성(마스카렌 분지 연약권 저장소, Mascarene Basin Asthenosphere Reservoir)의 영향으로 설명될 수 있다. 본 연구에서는 이러한 유사-플룸 변칙성이 하부 맨틀에 위치한 아프리카 LLSVP로부터 기원하는 광범위한 상승 구조와 연결된 중단된 플룸 현상이라고 제안한다.

    따라서 이 연구는 인도양 맨틀에서의 지구동역학 및 MORB의 지구화학적 특성에 미치는 영향, 인도양 중앙해령을 따라 일어나는 해저면 확장에 대한 영향 뿐만이 아니라중앙해령에 영향을 미치는 다양한 요소들에 대한 전반적 통찰을 제공한다.

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    목차 (Table of Contents)

    • Abstract i
    • Aknowledgements . iii
    • Table of Contents v
    • Abstract i
    • Aknowledgements . iii
    • Table of Contents v
    • Table of Figures ix
    • Chapter 1. Introduction 1
    • References 15
    • Chapter 2. Heterogeneous Fossil Réunion Plume Component in
    • the Source Region of Enriched MORB Along the Central Indian
    • Ridge Between 12° and 17°S . 28
    • Abstract 28
    • 2.1. Introduction . 29
    • 2.2. Geological Setting and Background 33
    • 2.3. Sampling and Analytical Methods 34
    • 2.4. Results 47
    • 2.4.1. Major and Trace Elements . 47
    • 2.4.2. Isotopic Compositions and Correlations 48
    • 2.5. Discussion 56
    • 2.5.1. Latitudinal Variation in MORB Geochemistry
    • and Ridge Segmentation 56
    • 2.5.2. Origin of the MORB Enrichment Along the Segments 5 and 6 (CIR From 14° to 17°S . 60
    • 2.5.2.1. Contamination of the Réunion Plume by a Continental
    • Crust Component as a Source of the MORB Enrichment Along
    • Segment 5? . 61
    • 2.5.2.2. Origin of the Crustal Component. 64
    • 2.5.2.3. The Geochemical Discrepancy Between E-MORB
    • From Segments 5, 6 and Rodrigues Segment . 66
    • 2.6. Conclusion 67
    • References 68
    • Chapter 3. Relationships Between Mantle Chemical
    • Compositions Variations and Magmatic Accretion Processes
    • Along a Segment of the Central Indian Ridge (14°-16°S) . 79
    • Abstract 79
    • 3.1. Introduction . 80
    • 3.2. Tectonic Context and Study Area 82
    • 3.3. Data and Methodology 88
    • 3.3.1. Multibeam Bathymetry Analysis . 88
    • 3.3.2. Gravity Data Processing and Modelling . 89
    • 3.3.3. Sampling and Analytical Methods: Helium
    • Analysis 91
    • 3.4. Results 94
    • 3.4.1. Structure of the Segment 5 of the Central
    • Indian Ridge 94
    • 3.4.1.1. The Segment 5-1 94
    • 3.4.1.2. The Segment 5-2 96
    • 3.4.1.3. The Segment 5-3 98
    • 3.4.2. Tectonic Strain and Magmatic Extension
    • Estimates . 100
    • 3.4.3. The Gravity Anomaly Along the Segment 5..
    • 102
    • 3.4.4. Helium Isotopes Ratios of MORB from the
    • Segment 5 103
    • 3.5. Discussion 105
    • 3.5.1. The Helium Signature Along Segment 5 . 105
    • 3.5.2. Relationships Between Along-Axis Geophysics
    • and MORB Geochemistry 110
    • 3.5.3. Implications for the Magma Supply Along
    • Segment 5 119
    • 3.6. Conclusion 125
    • References 126
    • Chapter 4. Mascarene Basin Asthenosphere Reservoir source
    • and composition revealed by Central Indian Ridge basalt
    • geochemistry 138
    • Abstract . 138
    • 4.1. Introduction 139
    • 4.2. Geological Setting 140
    • 4.3. Sampling and Analytical Methods . 142
    • 4.4. Results 145
    • 2.4.1. Major and Trace Elements 145
    • 2.4.2. Isotopes 148
    • 4.5. Discussion . 148
    • 4.5.1. MORB enrichment characteristics and origin
    • along segments 2 and 3 . 149
    • 4.5.1.1. Segments 2 and 3 MORB characteristics 149
    • 4.5.1.2. Two or three components in the melting regime? . 156
    • 4.5.1.3. Origin of the “High 206Pb/204Pb Group” 157
    • 4.5.2. Relationship between the MBAR anomaly and
    • the Réunion plume (RP) 160
    • 4.5.3. The African LLSVP as a possible origin for the
    • MBAR 163
    • 4.5.4. The influence extent of the MBAR along the
    • CIR: Are there other ridge portions influenced by the
    • MBAR? . 170
    • 4.6. Conclusion 173
    • References 177
    • Chapter 5. General Conclusions 186
    • 5.1. Summary and Future Perspective 186
    • References 196
    • A. Supplementary Material 203
    • B. Supplementary Material for Chapter 2 . 218
    • C. Supplementary Material for Chapter 4 . 222
    • Abstract in Korean 232
    • Table of Figures
    • Figure 1. Map of the global mid-ocean ridge system 1
    • Figure 2. Schematic diagrams showing the mantle upwelling beneath
    • mid-ocean ridges and the thermodynamic processes involved 3
    • Figure 3. Primitive-mantle normalized spider diagram for typical
    • signature of N-MORB, E-MORB and OIB . 4
    • Figure 4. Systematics isotopic variability in global OIB and MORB . 6
    • Figure 5. Schematic illustrations of the neovolcanic zone at various
    • spreading rates 7
    • Figure 6. Proposed hierarchy of ridge segmentation at fast-spreading
    • and slow-spreading ridges 8
    • Figure 7. General Map of the Indian Ocean showing its spreading
    • ridges . 9
    • Figure 8. Geological setting map of the Central Indian Ridge (CIR)
    • region and bathymetric map of the middle part of the CIR. 11
    • Figure 9. Geological setting map of the CIR region and sample
    • locations along the CIR from 12°S to 17°S analyzed in this study .. 32
    • Figure 10. Pictures presenting an overview of the Mid Oceanic Ridge
    • Basalt (MORB) samples 38
    • Figure 11. Harker diagram of MORB along the segments 5 and 6 of
    • the CIR (from 14°S to 17°S) 39
    • Figure 12. Na8 variation in function of MgO (wt. %), latitude and
    • bathymetry of CIR MORB glasses from segments 5 and 6 . 40
    • Figure 13. Trace element normalized to primitive mantle of basaltic
    • glasses from segment 5 41
    • Figure 14. Latitudinal variations along the ridge axis of the CIR
    • segments between 12° and 21°S in chemical compositions of
    • (La/Sm)N, Nb/U, Ce/Pb, Nd/Pb, and Sr, Nd and Pb isotopes of
    • submarine basalt . 42
    • Figure 15. Latitudinal variations along the ridge axis of (La/Sm)N,
    • strontium isotopes ratios and lead isotopes ratios of submarine basalt
    • from segment 5 (14° to 16.2°S) 51
    • Figure 16. 143Nd/144Nd versus 87Sr/86Sr, 87Sr/86Sr versus Δ8/4,
    • 207Pb/204Pb versus 206Pb/204Pb, 208Pb/204Pb versus 206Pb/204Pb
    • covariation diagrams . 53
    • Figure 17. (La/Sm)N versus
    • 206Pb/204Pb and Nb/U, Ce/Pb and Nd/Pb
    • versus 87Sr/86Sr for the Central Indian MORB samples 55
    • Figure 18. 207Pb/206Pb versus 208Pb/206Pb, 87Sr/86Sr versus 208Pb/206Pb
    • and 143Nd/144Nd versus 208Pb/206Pb covariation diagrams presenting
    • the mixing model between a «pure» Réunion Plume (RP) component, a
    • Seychelles/Madagascar-like continental crust component and a
    • depleted CIR MORB mantle 58
    • Figure 19. Shaded bathymetric map of segment 5 and its second-
    • order segments with the locations of samples analyzed in this study
    • 84
    • Figure 20. Detailed structural maps interpreted from bathymetry of
    • the axial valley and ridge flanks of the segment 5 (CIR) 85
    • Figure 21. Backscatter image of the segment 5 (CIR), from multibeam
    • echosounder data 87
    • Figure 22. Free air anomaly and mantle Bouguer gravity anomaly
    • maps of the segment 5 (CIR) 90
    • Figure 23. Along-axis variations of bathymetry, MBA variations, axial
    • valley width, total accumulated tectonic strain (T) and inferred
    • magmatic extension (M) as well as Latitudinal variations along the
    • ridge axis in He isotopes and chemical compositions of (La/Sm)N, Na8
    • and Fe8 of submarine basalts from segment 5 (13.82° to 16.05°S) 93
    • Figure 24. Methodology employed in this study to estimate both
    • tectonic strain (T) and magmatic accretion (M) 99
    • Figure 25. Latitudinal variations along the ridge axis of (La/Sm)N and
    • Sr, Nd, Pb and He isotopes ratios of submarine basalt from segment
    • 5 (13.82° to 16.05°S) . 107
    • Figure 26. 3He/4He (R/RA) versus (La/Sm)N,
    • 87Sr/86Sr, 143Nd/144Nd and 208Pb*/206Pb* for basalts from segment 5 108
    • Figure 27. Na8 variation versus bathymetry and (La/Sm)N of CIR
    • MORB glasses from segment 5 . 112
    • Figure 28. Plots of (a) latitude versus MORB samples depth, (b)
    • La/Sm versus depth, (c) (La/Sm)N versus (Tb/Yb)N, (d) Sm/Yb versus
    • Sm, (e) La/Sm versus Sm/Yb for MORB lavas sampled along segment
    • 5 113
    • Figure 29. Schematic model of the melt delivery system along
    • segment 5 of the CIR . 123
    • Figure 30. Bathymetric and topographic map of the western part of
    • the Indian Ocean and the East African Rift System as well as the
    • bathymetric map of segments 2 and 3 141
    • Figure 31. Harker diagram of MORB along the segments 2 and 3 of
    • the CIR (from 8°S to 12°S) 146
    • Figure 32. Trace element normalized to primitive mantle of basaltic
    • lavas from segment 2 and 3 147
    • Figure 33. 143Nd/144Nd versus 87Sr/86Sr, 207Pb/204Pb versus 206Pb/204Pb,
    • 208Pb/204Pb versus 206Pb/204Pb covariation diagrams for the CIR
    • MORB samples from segments 2 and 3. 150
    • Figure 34. (La/Sm)N versus
    • 206Pb/204Pb, Nb/U versus 87Sr/86Sr, Ba/La
    • versus 206Pb/204Pb, Nd/Pb versus 87Sr/86Sr and, 206Pb/204Pb as well as
    • 143Nd/144Nd for the MORB samples from segments 2 and 3 152
    • Figure 35. 207Pb/206Pb versus 208Pb/206Pb, 87Sr/86Sr versus 208Pb/206Pb and
    • 143Nd/144Nd versus 208Pb/206Pb covariation diagrams comparing the MORB from the
    • CIR between 8° and 12°S (segments 2 and 3) with the different lavas related to
    • plumes sourced in the African LLSVP . 154
    • Figure 36. 3He/4He (R/RA) versus
    • 206Pb/204Pb of MORB glasses along
    • segments 2 and 3 of the CIR (from 8°S to 12°S) 159
    • Figure 37. Principal component analysis projections of the MORB Pb
    • isotope dataset from the segments 2 and 3 of the CIR (from 8°S to
    • 12°S) 167
    • Figure 38. Schematic map comparing the location of the MBAR, the
    • segments 2 and 3, the African LLSVP and the related Indo-African
    • volcanic settings investigated in this study 169
    • Figure 39. 207Pb/206Pb versus 208Pb/206Pb, 87Sr/86Sr versus 208Pb/206Pb
    • covariation diagrams comparing the MORB from the CIR between 8°
    • and 12°S (segments 2 and 3) with the MORB from the CIR and
    • Carlsberg ridge . 172
    • Figure 40. Map showing the spatial extent of the three geochemical
    • enrichment groups observed along the Central Indian Ridge and
    • variations diagram between 206Pb/204Pb versus 87Sr/86Sr highlighting
    • the three geochemical enrichment groups observed along the Central
    • Indian Ridge 194
    • Table 1. Sr, Nd, and Pb Isotopic Compositions in MORB from the CIR
    • Between 12° and 17°S . 44
    • Table 2. He Isotopic Compositions in MORB from the CIR Between
    • 13.8° and 16.1°S . 92
    • Table 3. Sr, Nd, and Pb Isotopic Compositions in MORB From the CIR
    • Between 8° and 12°S . 144
    더보기

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