Thermal and rheological state of the lithosphere and specific features of structuring in the rift zone of the Reykjanes Ridge (from the results of numerical and experimental modeling)     

E. P. Dubinin  A. L. Grokhol’skii  A. V. Kokhan  A. A. Sveshnikov 《Izvestiya Physics of the Solid Earth》2011,47(7):586-599

Specific features of the bottom topography structure and the character of morphostructural segmentation of the rift zone of the Reykjanes Ridge change substantially along the ridge strike with increasing distance from Iceland’s hotspot. A clearly pronounced regularity of changes is observed in the rift zone’s morphology from the axial uplift (in the northern part of the ridge) to the rift valleys (in the southern part of the ridge) through an intermediate or transitional type of morphology. The results of numerical modeling showed that changes in the rift zone’s morphology along the Reykjanes Ridge strike are largely caused by changes in the degree of mantle heating and depend on the intensity of magma supply. It is shown that under conditions of ultraslow spreading, it is these parameters that control the presence or absence of crustal magma chambers, as well as the thickness of the effectively-elastic layer of the axial lithosphere. The experimental modeling of topography-forming deformations and structuring on the Reykjanes Ridge showed that under oblique extension, specific features of the formation of axial fractures and the character of their segmentation mainly depend on the thickness of the axial lithosphere, its heating zone width, and the kinematics of spreading. The experiments also showed that the tendency of fractures to develop obliquely to the extension axis is caused by the action of the inclined zone of the location of the deformation, and shear deformations play a substantial role in the lithosphere’s destruction as the inclination angle increases.  相似文献   

Off-axis structures of spreading zones according to results of experimental modeling     

A. L. Grokholsky  E. P. Dubinin  A. V. Kokhan  A. V. Petrova 《Geotectonics》2014,48(2):87-103

The off-axis topography of spreading ridges is a result of tectonic and magmatic processes occurring in the axial zone and operating off the ridge axis during further evolution of the crust. The results of physical and numerical simulations have shown that differences in topography roughness, rift valley depth, frequency and amplitude of normal faults, and geometric stability of the rift axis are determined by (a) the rate of extension and accretion of the new crust, (b) the thickness of the brittle lithospheric layer, and (c) the temperature of the underlying asthenosphere. Under conditions of the fast spreading, the stationary axial magma chamber in the crust predetermines the existence of the thinner and weakened lithosphere. As a result, the axis jumps for a short distance and the axis geometry remains almost rectilinear. The destruction of the thin axial lithosphere with a low mechanical strength results in formation of frequent and low-amplitude normal faultings. All these factors lead to the formation of the characteristic poorly dissected topography of fast-spreading ridges. Without a stationary axial magmatic chamber in the crust of slow-spreading ridges and with a thick and strong lithosphere, a deeply dissected axial and off-axis topography arises. The axis jumps for a significant distance within the rift valley, giving rise to geometric instability of the axis and development of transform and nontransform offsets.  相似文献   

Observations of outflowing ion beams on auroral field lines at altitudes of many earth radii     

R. Lunpin  B. Hultqvist  E. Dubinin  A. Zackarov  N. Pissarenko 《Planetary and Space Science》1982,30(7):715-726

The composition, energy and angular characteristics of upward flowing ionospheric ions at altitudes greater than ～ 20,000 km have been studied by means of the PROGNOZ-7 ion composition experiment. Very narrow beams, having widths corresponding to a mirroring altitude of the order a few thousand kilometers or less, may be found up to altitudes exceeding 30,000 km on the nightside. At much higher altitudes and in regions connected to the dayside/flank boundary layer and plasma mantle, the beams are much broader than expected from adiabatic particle motions from an ionospheric source/acceleration region, suggesting that pitch angle scattering or transverse acceleration processes are present there. Considerable mass dispersion effects have also been observed in some upward flowing ionospheric ion beams. The peak energy for the O⁺ ions may differ by several keV compared to that for the H⁺ ions in one and the same ion beam at altitudes above ～ 20,000 km. The O⁺ ions in these beams have gained considerably more energy than H⁺ in the acceleration process. Many examples with a much higher O⁺ than H⁺ content in the beam have been observed. Possible mechanisms giving rise to the observed effects are discussed, one being several kV of potential drop below the neutral H, O-crossover altitude (500–1500 km). At altitudes where the upflowing ionospheric ions are intermixed with magnetosheath ions, mass dispersion effects are also observed. This dispersion often appears to be the result of a velocity filtering effect caused by the dawn-dusk electric field (earthward convection).  相似文献   

Solar wind energy transfer regions inside the dayside magnetopause: Accelerated heavy ions as tracers for MHD-processes in the dayside boundary layer     

R. Lundin  E.M. Dubinin 《Planetary and Space Science》1985,33(8):891-907

Plasma and magnetic field data from PROGNOZ-7 have revealed that solar wind (magnetosheath) plasma elements may penetrate the dayside magnetopause surface and form high density regions with enhanced cross-field flow in the boundary layer.The injected magnetosheath plasma is observed to have an excess drift velocity as compared to the local boundary layer plasma, comprising both “cold” plasma of terrestrial origin and a hot ring current component. A differential drift between two plasma components can be understood in terms of a momentum transfer process driven by an injected magnetosheath plasma population. The braking action of the injected plasma may be described as a dynamo process where particle kinetic energy is transferred into electromagnetic energy (electric field). The generated electric field will force the local plasma to $\text{ε×}\text{B}\text{-drift}$, and the dynamo region therefore also constitutes an accelerator region for the local plasma. Whenever energy is dissipated from the energy transfer process (a net current is flowing through a load), there will also be a difference between the induced electric field and the $\text{v}\text{×}\text{B}$ term of the generator plasma. Thus, the local plasma will drift more slowly than the injected generator plasma.We will present observations showing that a relation between the momentum transferred, the injected plasma and the momentum taken up by the local plasma exists. For instance, if the local plasma density is sufficiently high, the differential drift velocity of the injected and local plasma will be small. A large fraction of the excess momentum is then transferred to the local plasma. Conversely, a low local plasma density results in a high velocity difference and a low fraction of local momentum transfer.In our study cases the “cold” plasma component was frequently found to dominate the local magnetospheric plasma density in the boundary layer. Accordingly, this component may have the largest influence on the local momentum transfer process. We will demonstrate that this also seems to be the case. Moreover we show that the accelerated “cold” plasma component may be used as a tracer element reflecting both the momentum and energy transfer and the penetration process in the dayside boundary layer.The high He⁺ percentage of the accelerated “cold” plasma indicates a plasmaspheric origin. Considering the quite high densities of energetic He⁺ found in the boundary layer, the overall low abundance of He⁺ (as compared to e.g. O⁺) found in the plasma sheet and outer ring current evidently reduces the importance of the dayside boundary layer as a plasma source in the large scale magnetospheric circulation system.  相似文献   

Location of the bow shock and ion composition boundaries at Venus—initial determinations from Venus Express ASPERA-4     

C. Martinecz  M. Fränz  N. Krupp  E. Dubinin  S. Barabash  M. Holmström  M. Yamauchi  Y. Futaana  H. Gunell  J.D. Winningham  J. Scherrer  D.R. Linder  E. Kallio  W. Schmidt  H.E.J. Koskinen  J. Luhmann  E.C. Roelof  C.C. Curtis  B.R. Sandel  J.-A. Sauvaud  J.-J. Thocaven  S. McKenna-Lawler  R. Cerulli-Irelli  A. Mura  P. Wurz  P. Bochsler  K. Szego  T.L. Zhang 《Planetary and Space Science》2008,56(6):780-784

For the first time since 1992 when the Pioneer Venus Orbiter (PVO) ceased to operate, there is again a plasma instrument in orbit around Venus, namely the ASPERA-4 flown on Venus Express (inserted into an elliptical polar orbit about the planet on April 11, 2006). In this paper we report on measurements made by the ion and electron sensors of ASPERA-4 during their first five months of operation and, thereby, determine the locations of both the Venus bow shock (BS) and the ion composition boundary (ICB) under solar minimum conditions. In contrast to previous studies based on PVO data, we employ a 3-parameter fit to achieve a realistic shape for the BS. We use a different technique to fit the ICB because this latter boundary cannot be represented by a conic section. Additionally we investigate the dependence of the location of the BS on solar wind ram pressure (based on ASPERA-4 solar wind data) and solar EUV flux (using a proxy from Earth).  相似文献   

Structure formation in areas of nontransform offsets of axial spreading zones (analog modeling)     

A. L. Grokholskii  Ye. P. Dubinin  I. V. Shapovalova 《Moscow University Geology Bulletin》2010,65(3):185-193

The results of experimental modeling and features of structure formation in the zones of nontrans-form offsets (NTOs) of spreading axes are presented. The experiments were performed on materials that are colloidal systems based on liquid and solid hydrocarbons, taking into account the similarity of conditions. The following parameters were changed during the experiments: (1) the thickness of the model lithosphere of the rift zone, (2) the thickness of the lithosphere in the zone of nontransform offsets between the rift segments; (3) the spreading velocity. The critical values of offsets for the spreading axes at which a character of structure formation in the zones of NTOs is changed were established.  相似文献   

Experimental modeling of structure-forming deformations in rift zones of mid-ocean ridges     

A. L. Grokholskii  E. P. Dubinin 《Geotectonics》2006,40(1):64-80

The modern methods of physical modeling of structure-forming deformations in extension zones of oceanic lithosphere are discussed; the methods differ in their experimental equipment, model material, and experimental techniques. The simulation performed with an elastic-ductile model has demonstrated that extension of a brittle lithospheric layer results in disruption of its continuity and in formation of a rift valley according to the mechanism of running fracture propagation. The modeling results provide insights into qualitative pattern of faulting and fracturing within a rift zone, specific features of rift segmentation, and development of various structural elements (axis bends, echelons of fractures, nontransform offsets, small and large overlaps, etc.) under various geodynamic conditions of spreading. The modeling has shown that origination and evolution of structures of various types depend on the lithosphere’s thickness beneath the rift axis; the width of the lithosphere’s heating zone; the spreading orientation; and, to a lesser degree, on the spreading rate. A relatively rectilinear rift broken into particular segments bounded by small-amplitude offsets with or without minor overlaps arises in the case of both a small width of the heating zone, closely related to the axial magma chamber, and a small thickness of the lithosphere (fast-spreading conditions). In the case of a wide heating zone caused by ascent of an asthenospheric wedge or a mantle plume, offsets of rift are more pronounced and deformations embrace a wider region. If, as a result, the thickness of the lithosphere increases, the rift will be less linear and the structural heterogeneity will become more contrasting. In addition to the thickness of the lithosphere, the angle between the rift zone and the extension axis also controls the rift configuration: the greater the angle, the more conspicuous the en echelon arrangement of fractures. For any spreading type, the propagating front of linear microfractures that disrupt the upper brittle layer of the lithosphere predates the origin of mesoscopic fractures and predetermines a general trend of the rift zone. This indicates that the fractures of various sizes propagate simultaneously.  相似文献   

Geochemistry of the authigenic ferromanganese ore formation in sediments of the Northeast Pacific Basin     

A. V. Dubinin  V. N. Sval’nov  T. Yu. Uspenskaya 《Lithology and Mineral Resources》2008,43(2):99-110

Authigenic ferromanganese formations in sediments from two horizons (0–10 and 240–250 cm) located in the low/high bioproductive transitional zone of the Pacific Ocean were studied. In addition to the compositionally different two types of micronodules, crusts and ferromanganese nodules were detected in the surface horizon (0–1 cm). Three size fractions (50–100, 100–250, and 250–500 μm) of manganese micronodules were investigated. In terms of surface morphology, color, and shape, the micronodules are divided into the dull round (MN1) and angular lustrous (MN2) varieties with different mineral and chemical compositions. The dull MN1 are enriched in Mn and depleted in Fe as compared with the lustrous MN2. The Mn/Fe value in the dull MN1 varies from 13 to 14. Asbolane-buserite and birnessite are the major manganese minerals in them. The lustrous MN2 is mainly composed of vernadite with Mn/Fe = 4.3–4.8. Relative to the dull MN1, fraction 50–100 μm of the lustrous MN2 is enriched in Fe (2.6 times), W (1.8), Mo (3.2), Th (2.3), Ce (5.8), and REE (1.2–1.8). Relative to counterparts from the dull MN1, separate fractions of the lustrous MN2 are characterized by a greater compositional difference. For example, increase in the size of micronodules leads to decrease in contents of the following elements: Fe (by 10 rel %), Ce (2 times), W (2.1 times), Mo (2.2 times), and Co (1.5 times). At the same time, one can see increase in contents of other elements: Th and Cu (2.1 times), Ni (1.9 times), and REE (1.2–1.6 times). Differences in the chemical and mineral compositions of MN1 and MN2 fractions can be related to alternation of oxidative and suboxidative conditions in the sediments owing to the input of a labile organic matter, which serves as the major reducer, and the allochthonous genesis of MN2.  相似文献   

Rheological layering of the oceanic lithosphere in rift zones of mid-oceanic ridges     

Yu. I. Galushkin  E. P. Dubinin  A. A. Sveshnikov 《Doklady Earth Sciences》2008,418(1):114-117

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Regional and local magmatic anomalies and tectonics of rift zones between the Antarctic and South American plates     

N. M. Sushchevskaya  N. A. Migdisova  E. P. Dubinin  B. V. Belyatsky 《Geochemistry International》2016,54(6):494-508

The study provides new understanding of magmatism at extinct and modern spreading zones around the western margin of East Antarctica from Bransfield Strait to the Bouvet Triple Junction (BTJ) in the Atlantic Ocean and reveals causes of geochemical heterogeneity of mantle magmatism during the early opening of the Southern Ocean. The results indicate the involvement of an enriched source component in the generation of parental melts, which was formed in several tectonic stages. The enriched (metasomatized) mantle generated at rift zones has geochemical characteristics typical of the western Gondwana lithosphere (with isotopic compositions similar to those inferred for the enriched HIMU and EM-2 sources). This mantle source may have been produced by the thermal erosion of the continental mantle during the early stages of the Karoo–Maud–Ferrar superplume activity. This enriched mantle generated in the apical parts of the plume (sub-oceanic) began to melt during tectonic displacement and fragmentation of Gondwana. The Bouvet Triple Junction, located along modern spreading zones between the Antarctic and South American plate, is characterized by a greater depth of melting and a higher degree of enrichment of primary tholeiitic magmas. The highest enrichment of magmas in this region is controlled by a contribution from a pyroxenite-rich component, which was also identified in the extinct spreading center in Powell Basin.  相似文献