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1.
J. C. Balanyá J. Galindo-Zaldívar A. Jabaloy G. Leitchenkov A. Maldonado J. Rodríguez-Fernández O. Vinnikovskaya 《Geo-Marine Letters》1999,18(3):215-224
The structure of the South Powell Ridge (SPR), separating the Late Cenozoic ocean-floored Powell Basin and the Mesozoic Weddell
Sea domain, is revealed by multichannel seismic data. The SPR appears as a basement high, bounded northward by transtensional
faults and by normal and major reverse faults to the south. These margin features seem to be linked to the Powell Basin southern
strike-slip margin and to the Jane Arc paleotrench, respectively. We suggest the ridge evolved from the Antarctic Peninsula
passive margin to become the deformational front of the Scotia/Antarctica Plate boundary, later being welded to the Antarctic
Plate.
Received: 18 August 1997 / Revision received: 4 May 1998 相似文献
2.
Yu. I. Galushkin G. L. Leitchenkov Yu. B. Guseva E. P. Dubinin 《Izvestiya Physics of the Solid Earth》2018,54(1):79-90
The burial history and thermal evolution of the lithosphere within the passive nonvolcanic Antarctic margin in the region of the Mawson Sea are numerically reconstructed for the margin areas along the seismic profile 5909 with the use of the GALO basin modeling system. The amplitudes of the lithosphere stretching at the different stages of continental rifting which took place from 160 to 90 Ma ago are calculated from the geophysical estimates of the thickness of the consolidated crust and the tectonic analysis of the variations in the thickness of the sedimentary cover and sea depths during the evolution of the basin. It is hypothesized that the formation of the recent sedimentary section sequence in the studied region of the Antarctic margin began ~140 Ma ago on a basement that was thinned by a factor of 1.6 to 4.5 during the first episode of margin stretching (160–140 Ma) under a fairly high heat flux. The reconstruction of the thermal regime of the lithosphere has shown that the mantle rocks could occur within the temperature interval of serpentinization and simultaneously within the time interval of lithospheric stretching (–160 < t <–90 Ma) only within separate segments of profile 5909 in the Mawson Sea. The calculations of the rock strength distribution with depth by the example of the section of pseudowell 4 have shown that a significant part of the crust and uppermost mantle fall here in the region of brittle deformations in the most recent period of lithosphere stretching (–104 to–90 Ma ago). The younger basin segments of profile 5909 in the region of pseudowells 5 and 6 are characterized by a high heat flux, and the formation of through-thickness brittle fractures in these zones is less probable. However, serpentinization could take place in these areas as in the other margin segments at the stage of presedimentation ultra slow basement stretching. 相似文献
3.
G. Leitchenkov J. Guseva V. Gandyukhin G. Grikurov Y. Kristoffersen M. Sand A. Golynsky N. Aleshkova 《Marine Geophysical Researches》2008,29(2):135-158
About 16,000 km of multichannel seismic (MCS), gravity and magnetic data and 28 sonobuoys were acquired in the Riiser-Larsen
Sea Basin and across the Gunnerus and Astrid Ridges, to study their crustal structure. The study area has contrasting basement
morphologies and crustal thicknesses. The crust ranges in thickness from about 35 km under the Riiser-Larsen Sea shelf, 26–28 km
under the Gunnerus Ridge, 12–17 km under the Astrid Ridge, and 9.5–10 km under the deep-water basin. A 50-km-wide block with
increased density and magnetization is modeled from potential field data in the upper crust of the inshore zone and is interpreted
as associated with emplacement of mafic intrusions into the continental margin of the southern Riiser-Larsen Sea. In addition
to previously mapped seafloor spreading magnetic anomalies in the western Riiser-Larsen Sea, a linear succession from M2 to
M16 is identified in the eastern Riiser-Larsen Sea. In the southwestern Riiser-Larsen Sea, a symmetric succession from M24B
to 24n with the central anomaly M23 is recognized. This succession is obliquely truncated by younger lineation M22–M22n. It
is proposed that seafloor spreading stopped at about M23 time and reoriented to the M22 opening direction. The seismic stratigraphy
model of the Riiser-Larsen Sea includes five reflecting horizons that bound six seismic units. Ages of seismic units are determined
from onlap geometry to magnetically dated oceanic basement and from tracing horizons to other parts of the southern Indian
Ocean. The seaward edge of stretched and attenuated continental crust in the southern Riiser-Larsen Sea and the landward edge
of unequivocal oceanic crust are mapped based on structural and geophysical characteristics. In the eastern Riiser-Larsen
Sea the boundary between oceanic and stretched continental crust is better defined and is interpreted as a strike-slip fault
lying along a sheared margin. 相似文献
4.
The Lambert Rift, which is a large intracontinental rift zone in East Antarctica, developed over a long period of geological time, beginning from the Late Paleozoic, and its evolution was accompanied by magmatic activity. The latest manifestation of magmatism is eruption of alkaline olivine–leucite basalts on the western side of the Lambert Rift; Rb–Sr dating referred its time to the Middle Eocene, although its genesis remained vague. In order to solve this problem, we found geochronometer minerals in basaltic samples and 68 apatite grains appeared to be suitable for analysis. Their ages and ages of host basalts, determined by the U–Pb local method on the SIMS SHRIMP-II, were significantly different (323 ± 31 Ma) from those assumed earlier. This age corresponds to the earliest stage of crustal extension in East Antarctica and to most of Gondwana. The new data crucially change the ideas about the evolution of Lambert Rift and demonstrate the ambiguity of К–Ar dates of the alkali effusive formed under long-term rifting. 相似文献
5.
G. L. Leitchenkov Yu. B. Guseva V. V. Gandyukhin S. V. Ivanov L. V. Safonova 《Geotectonics》2014,48(1):5-23
The Southern Indian Ocean comprises large sedimentary basins of the Riiser-Larsen Sea (western sector); the Cosmonauts, Cooperation (Commonwealth), Davis seas (central sector); and the Mawson-d’Urville seas (eastern sector). The main tectonic provinces of the Southern Indian Ocean (Antarctica) have been outlined as a result of comprehensive interpretation of the geophysical data. Special attention is paid to determining the boundary between the rifted continental and oceanic crust. The basin of the Riiser-Larsen Sea was formed in the Early Jurassic under the action of the Karoo mantle plume. The intrusive complex, as a remote manifestation of the mantle plume, occurs along the inner boundary of the marginal rift. Opening of the ocean in the basin of Riiser-Larsen Sea started about 160 Ma ago and was characterized by rearrangement of plate motion and intense volcanic activity at the early stage. In the basin of the Cosmonauts, Cooperation, and Davis seas, the final stage of rifting was accompanied by the rise of the lithospheric mantle and by intrusive magmatism. The opening of the ocean started here 134 Ma ago. Emplacement of the Kerguelen plume resulted in jumping of ridges and detachment of continental crustal blocks from the Indian margin with the formation of the Kerguelen Plateau (microcontinent). The basin of the Mawson-d’Urville seas has evolved under conditions of long-term rifting since the Late Jurassic and is characterized by an extended zone of mantle unroofing. Breakup of the lithosphere between Australia and Antarctica developed asynchronously over a time interval of 95–65 Ma ago with propagation of MOR from the west eastward. The research was carried out using a great body of geophysical information (～140000 km of CDP seismic profiling, more than 250 stations of seismic refraction sounding, and more than 250000 km of magnetic and gravity profiles) obtained by expeditions from many countries over more than 30 years. 相似文献
6.
Balanyá J. C. Galindo-Zaldívar J. Jabaloy A. Leitchenkov G. Maldonado A. Rodríguez-Fernández J. Vinnikovskaya O. 《Geo-Marine Letters》1998,18(3):215-224
The structure of the South Powell Ridge (SPR), separating the Late Cenozoic ocean-floored Powell Basin and the Mesozoic Weddell Sea domain, is revealed by multichannel seismic data. The SPR appears as a basement high, bounded northward by transtensional faults and by normal and major reverse faults to the south. These margin features seem to be linked to the Powell Basin southern strike-slip margin and to the Jane Arc paleotrench, respectively. We suggest the ridge evolved from the Antarctic Peninsula passive margin to become the deformational front of the Scotia/Antarctica Plate boundary, later being welded to the Antarctic Plate.
相似文献7.
8.
B. Kuvaas Y. Kristoffersen J. Guseva G. Leitchenkov V. Gandjukhin G. Kudryavtsev 《Marine Geophysical Researches》2004,25(3-4):247-263
Multichannel seismic reflection data from the Cosmonaut Sea margin of East Antarctica have been interpreted in terms of depositional
processes in the continental slope and rise area. A major sediment lens is present below the upper continental rise along
the entire Cosmonaut Sea margin. The lens probably consists of sediments supplied from the shelf and slope, being constantly
reworked by westward flowing bottom currents, which redeposited the sediments into a large scale drift deposit prior to the
main glaciogenic input along the margin. High-relief semicircular or elongated depositional structures are also found on the
upper continental rise stratigraphically above the regional sediment lens, and were deposited by the combined influence of
downslope and alongslope sediment transport. On the lower continental rise, large-scale sediment bodies extend perpendicular
to the continental margin and were deposited as a result of downslope turbidity transport and westward flowing bottom currents
after initiation of glacigenic input to the slope and rise. We compare the seismostratigraphic signatures along the continental
margin segments of the adjacent Riiser Larsen Sea, the Weddell Sea and the Prydz Bay/Cooperation Sea, focussing on indications
that may be interpreted as a preglacial-glaciomarine transition in the depositional environment. We suggest that earliest
glaciogenic input to the continental slope and rise occurred in the Prydz Bay and possibly in the Weddell Sea. At a later
stage, an intensification of the oceanic circulation pattern occurred, resulting in the deposition of the regional plastered
drift deposit along the Cosmonaut Sea margin, as well as the initiation of large drift deposits in the Cooperation Sea. At
an even later stage, possibly in the middle Miocene, glacial advances across the continental shelf were initiated along the
Cosmonaut Sea and the Riiser Larsen Sea continental margins. 相似文献
9.
Geotectonics - This study focuses on physical modeling of interaction between the Indian and Pacific spreading axes, which resulted in separation of the Tasmania and Adélie blocks during the... 相似文献
10.
K. Solli B. Kuvaas Y. Kristoffersen G. Leitchenkov J. Guseva V. Gandjukhin 《Marine Geophysical Researches》2008,29(1):51-69
A set of multi-channel seismic profiles (∼15,000 km) is used to study the depositional evolution of the Cosmonaut Sea margin
of East Antarctica. We recognize a regional sediment wedge, below the upper parts of the continental rise, herein termed the
Cosmonaut Sea Wedge. The wedge is situated stratigraphically below the inferred glaciomarine section and extends for at least
1,200 km along the continental margin with a width that ranges from 80 to about 250 km. The morphology of the wedge and its
associated depositional features indicate a complex depositional history, where the deep marine depositional sites were influenced
by both downslope and alongslope processes. This interaction resulted in the formation of several proximal depocentres, which
at their distal northern end are flanked by elongated mounded drifts and contourite sheets. The internal stratification of
the mounded drift deposits indicates that westward flowing bottom currents reworked the marginal deposits. The action of these
currents together with sea-level changes is considered to have controlled the growth of the wedge. We interpret the Cosmonaut
Sea Wedge as a composite feature comprising several bottom current reworked fan systems. The wide spectrum of depositional
geometries in the stratigraphic column reflects dramatic variations in sediment supply from the continental margin as well
as varying interaction between downslope and alongslope processes. 相似文献