a recipe for microcontinent formation accreted slivers of continental margins are common in the geologic record but the processes that lead to their formation are poorly understood we observe an association of plume related microcontinent isolation and subsequent long term asymmetries in oceanic crustal accretion based on four recent examples the seychelles in the indian ocean jan mayen in the norwegian greenland sea and the east tasman plateau and the gilbert seamount complex in the tasman sea these microcontinents formed by rerifting of a young continental margin 25 m y old in the vicinity of a mantle plume stem followed by asymmetric seafloor spreading two dimensional numerical stochastic basin modeling suggests that a yield strength minimum along the landward edge of a rifted margin thermally enhanced by heating from a mantle plume may cause a spreading ridge to jump onto this zone of weakness this action isolates a passive margin segment the association of large igneous provinces and microcontinents should be useful for identifying similar events in the geological record

why did arabia separate from africa insights from 3 d laboratory experiments abstract we have performed 3 d scaled lithospheric experiments to investigate the role of the gravitational force exerted by a subducting slab on the deformation of the subducting plate itself experiments have been constructed using a dense silicone putty plate to simulate a thin viscous lithosphere floating in the middle of a large box filled with glucose syrup simulating the upper mantle we examine three different plate configurations i subduction of a uniform oceanic plate ii subduction of an oceanic continental plate system and iii subduction of a more complex oceanic continental system simulating the asymmetric africa eurasia system each model has been performed with and without the presence of a circular weak zone inside the subducting plate to test the near surface weakening effect of a plume activity our results show that a subducting plate can deform in its interior only if the force distribution varies laterally along the subduction zone i e by the asymmetrical entrance of continental material along the trench in particular extensional deformation of the plate occurs when a portion of the subduction zone is locked by the collisional process the results of this study can be used to analyze the formation of the arabian plate we found that intraplate stresses similar to those that generated the africa arabia break up can be related to the neogene evolution of the northern convergent margin of the african plate where a lateral change from collision mediterranean and bitlis to active subduction makran has been described second intraplate stress and strain localization are favored by the presence of a weakness zone such as the one generated by the afar plume producing a pattern of extensional deformation belts resembling the red sea gulf of aden rift system

robust characteristics method for modelling multiphase visco elasto plastic thermo mechanical problems abstract we have extended our previous 2d method gerya t v yuen d a 2003 characteristics based marker in cell method with conservative finite differences schemes for modeling geological flows with strongly variable transport properties phys earth planet interiors 140 295 320 which is a combination of conservative finite differences with marker in cell techniques to include the effects of visco elasto plastic rheology self gravitation and a self consistently derived evolving curvilinear planetary surface this code is called i2elvis and can solve a new class of computationally challenging problems in geodynamics such as shear localization with large strains crustal intrusion emplacement of magmas bending of realistic visco elasto plastic plates and core formation by vigorous shell tectonics activities related to a global rayleigh taylor instability of a metal layer formed around silicate rich lower density primordial core during planetary accretion we discuss in detail the computational strategy required the rheological constraints to be satisfied at each time step and spatial location we show analytical benchmarks and examples drawn from comparing between numerical and analogue experiments in structural geology subducting slab bending with a visco elasto plastic rheology and equilibrium spherical configurations from self gravitation we have also tested possibilities of future applications by addressing 3d geometries based on multigrid method and including inertial effects in the momentum equation with tracers in order to simulate meteoritic impact events and eventually earthquake instabilities

the southernmost margin of the tethys realm during the mesozoic and cenozoic initial geometry and timing of the inversion processes 1 along the northern border of africa pangea breakup has been diachronic during the jurassic the alpine tethys propagated northeastward from the atlantic to the alps during the permian the neo tethys propagated westward from oman to northwestern arabia then a secondary and late branch of neo tethys gave birth to the east mediterranean basin finally the two oceans connected at end of jurassic times achieving the development of africa northern plate boundary by the late cretaceous convergence between africa and eurasia led to the progressive closure of the tethys realm the continental collision is not completely achieved and the different segments of the confrontation zone maghreb central and east mediterranean zagros and oman expose different stages of the process however we emphasize the existence of synchronous geodynamic events from one end of the system to the other although they do not have the same meaning two of them are particularly important the campanian santonian c s event corresponds to 1 obduction and exhumation of high pressure low temperature metamorphic rocks around the arabian promontory 2 inversion along the margins of the east mediterranean basins and 3 lithosphere buckling in the atlas system maghreb and adjacent sahara platform the middle late eocene mle event corresponds to 1 the onset of collision at the northern corner of arabia 2 the onset of slab retreat in the mediterranean and 3 inversion along the margin of the east mediterranean as well as in the atlas the c s event coincides with a change in plate kinematics resulting in an abrupt increase of convergence velocity the mle event coincides with a period of strong coupling between the africa and eurasia plates and an abrupt decrease of convergence velocity in the middle of the system the central mediterranean seems to escape to the effects of convergence and is the site of quite permanent extensional movements since the triassic

geodynamic regimes of subduction under an active margin effects of rheological weakening by fluids and melts the dynamics of subduction under an active margin are analysed by using a 2d coupled petrological thermomechanical numerical model of an oceanic continental subduction system the model includes spontaneous slab bending dehydration of the subducted crust aqueous fluid transport partial melting of both crustal and mantle rocks as well as melt extraction processes resulting in magmatic arc crust growth based on our models the following five geodynamic regimes of subduction which may potentially form at active margins are identified i stable subduction with no backarc spreading centre and without plumes in the mantle wedge ii retreating subduction with a focused backarc spreading centre and without plumes iii retreating subduction with distributed intra arc extension and trans lithospheric sedimentary plumes iv advancing subduction with underplating laterally extending sub lithospheric plumes and v stable to advancing subduction with stationary laterally limited sub lithospheric plumes transitions between these different regimes are mainly caused by the concurrence of rheological weakening effects of i aqueous fluids percolating from the subducting slab into the mantle wedge and ii melts propagating from the partially molten areas formed in the mantle wedge towards the surface the aqueous fluids mainly affect the forearc region strong fluid related weakening promotes plate decoupling and reduces subduction drag and thus results in stacking of sediments in the accretion prism in contrast reduced weakening by fluids results in strong coupling of the plates and leads to advancing collision like subduction with enhanced subduction erosion thickening of the overriding plate and large sedimentary plumes in the mantle wedge are the consequences on the other hand melts extracted from the hot regions above the slab rheologically weaken the lithosphere below the arc which thus controls overriding plate extension and shortening strong rheological weakening by melts in combination with weak plate coupling trigger retreating subduction with a pronounced backarc spreading centre also weakening of the continental lithosphere by melts extracted from trans lithospheric sedimentary plumes generate a weak channel through which these structures may be emplaced into subarc crust if there is insufficient melt related weakening plumes cannot ascend but extend horizontally and thus underplate the lithosphere

mid ocean ridge jumps associated with hotspot magmatism abstract hotspot ridge interaction produces a wide range of phenomena including excess crustal thickness geochemical anomalies off axis volcanic ridges and ridge relocations or jumps ridges are recorded to have jumped toward many hotspots including iceland discovery galapagos kerguelen and tristan de cuhna the causes of ridge jumps likely involve a number of interacting processes related to hotspots one such process is reheating of the lithosphere as magma penetrates it to feed near axis volcanism we study this effect by using the hybrid finite element code flac to simulate two dimensional 2 d cross section viscous mantle flow elasto plastic deformation of the lithosphere and heat transport in a ridge setting near an off axis hotspot heating due to magma transport through the lithosphere is implemented within a hotspot region of fixed width to determine the conditions necessary to initiate a ridge jump we vary four parameters hotspot magmatic heating rate spreading rate seafloor age at the location of the hotspot and ridge migration rate our results indicate that the hotspot magmatic heating rate required to initiate a ridge jump increases non linearly with increasing spreading rate and seafloor age models predict that magmatic heating itself is most likely to cause jumps at slow spreading rates such as at the mid atlantic ridge on iceland in contrast despite the higher magma flux at the galapagos hotspot magmatic heating alone is probably insufficient to induce a ridge jump at the present day due to the intermediate ridge spreading rate of the galapagos spreading center the time required to achieve a ridge jump for fixed or migrating ridges is found to be on the order of 105 106 years simulations that incorporate ridge migration predict that after a ridge jump occurs the hotspot and ridge migrate together for time periods that increase with magma flux model results also suggest a mechanism for ridge reorganizations not related to hotspots such as ridge jumps in back arc settings and ridge segment propagation along the mid atlantic ridge

deformation during terrane accretion in the saint elias orogen alaska the saint elias orogen of southern alaska and adjacent canada is a complex belt of mountains formed by collision and accretion of the yakutat terrane into the transition zone from transform faulting to subduction in the northeast pacific the orogen is an active analog for tectonic processes that formed much of the north american cordillera and is also an important site to study 1 the relationships between climate and tectonics and 2 structures that generate large to great magnitude earthquakes the yakutat terrane is a fragment of the north american plate margin that is partly subducted beneath and partly accreted to the continental margin of southern alaska interaction between the yakutat terrane and the north american and pacific plates causes significant differences in the style of deformation within the terrane deformation in the eastern part of the terrane is caused by strike slip faulting along the fairweather transform fault and by reverse faulting beneath the coastal mountains but there is little deformation immediately offshore the central part of the orogen is marked by thrusting of the yakutat terrane beneath the north american plate along the chugach saint elias fault and development of a wide thin skinned fold and thrust belt strike slip faulting in this segment may be localized in the hanging wall of the chugach saint elias fault or dissipated by thrust faulting beneath a north northeast trending belt of active deformation that cuts obliquely across the eastern end of the fold and thrust belt superimposed folds with complex shapes and plunging hinge lines accommodate horizontal shortening and extension in the western part of the orogen where the sedimentary cover of the yakutat terrane is accreted into the upper plate of the aleutian subduction zone these three structural segments are separated by transverse tectonic boundaries that cut across the yakutat terrane and also coincide with the courses of piedmont glaciers that flow from the topographic backbone of the saint elias mountains onto the coastal plain the malaspina fault pamplona structural zone separates the eastern and central parts of the orogen and is marked by reverse faulting and folding onshore most of this boundary is buried beneath the western or agassiz lobe of the malaspina piedmont glacier the boundary between the central fold and thrust belt and western zone of superimposed folding lies beneath the middle and lower course of the bering piedmont glacier

a comparison of numerical surface topography calculations in geodynamic modelling an evaluation of the sticky air method summary calculating surface topography in geodynamic models is a common numerical problem besides other approaches the so called sticky air approach has gained interest as a free surface proxy at the top boundary the often used free slip condition is thereby vertically extended by introducing a low density low viscosityfluid layer this allows the air crust interface to behave in a similar manner to a true free surface we present here a theoretical analysis that provides the physical conditions under which the sticky air approach is a valid approximation of a true free surface two cases are evaluated that characterize the evolution of topography on different timescales 1 isostatic relaxation of a cosine perturbation and 2 topography changes above a rising plume we quantitatively compare topographies calculated by six different numerical codes using finite difference and finite element techniques using three different topography calculation methods i direct calculation of topography from normal stress ii body fitting methods allowing for meshing the topography and iii lagrangian tracking of the topography on an eulerian grid it is found that the sticky air approach works well as long as the term st ch hst l 3 is sufficiently small where st and hst are the viscosity and thickness of the sticky air layer and ch and l are the characteristic viscosity and length scale of the model respectively spurious lateral fluctuations of topography as observed in some marker based sticky air approaches may effectively be damped by an anisotropic distribution of markers with a higher number of markers per element in the vertical than in the horizontal direction

factors influencing magmatism during continental breakup new insights from a wide angle seismic experiment across the conjugate seychelles indian margins we present a model of the northern seychelles continental margin derived from controlled source wide angle seismic traveltime inversion and teleseismic receiver functions this margin has been widely cited as a classic example of rifting in association with a continental flood basalt province the deccan traps however we do not find the typical set of geophysical characteristics reported at other margins linked to continental flood basalts such as those of the north atlantic the oceanic crust formed immediately after breakup and throughout the first 3 ma of seafloor spreading is just 5 2 km thick less than half that typically seen at other volcanic margins the continent ocean transition zone is narrow and while two packages of seaward dipping reflectors are imaged within this transition they are weakly developed beneath the thinned continental crust there is an approximately 4 km thick layer of high velocity material 7 5 7 8 km s that we interpret as mafic material intruded and underplating the lower crust however we believe that this underplating most likely happened prior to the breakup overall the observations show that the rifting of india from the seychelles was characterized by modest magmatism the spatial extent of the deccan flood basalt province is therefore smaller than previously thought we speculate that either the lateral flow of deccan related hot material beneath the breakup region was hampered perhaps as the rifted margins did not intersect the center of the deccan source or there was incomplete melt extraction from the wide melting region that formed between the rapidly diverging plates if the latter explanation is correct then the rate of plate separation as indicated by the initial seafloor spreading rate is more important in controlling the volume of magmatism generated during continental rifting than has been previously recognized

gondwana derived microcontinents the constituents of the variscan and alpine collisional orogens abstract the european variscan and alpine mountain chains are collisional orogens and are built up of pre variscan building blocks which in most cases originated at the gondwana margin such pre variscan elements were part of a pre ordovician archipelago like continental ribbon in the former eastern prolongation of avalonia and their present day distribution resulted from juxtaposition through variscan and or alpine tectonic evolution the well known nomenclatures applied to these mountain chains are the mirror of variscan resp alpine organization it is the aim of this paper to present a terminology taking into account their pre variscan evolution at the gondwana margin they may contain relics of volcanic islands with pieces of cadomian crust relics of volcanic arc settings and accretionary wedges which were separated from gondwana by initial stages of rheic ocean opening after a short lived ordovician orogenic event and amalgamation of these elements at the gondwanan margin the still continuing gondwana directed subduction triggered the formation of ordovician al rich granitoids and the latest ordovician opening of palaeo tethys an example from the alps external massifs illustrates the gradual reworking of gondwana derived pre variscan elements during the variscan and alpine tertiary orogenic cycles

subduction history of the tethyan region derived from seismic tomography and tectonic reconstructions 1 in the mantle underneath the tethyan suture zone large volumes of positive velocity anomalies have been imaged by seismic tomography and interpreted as the present day signature of subducted tethyan lithosphere we investigate the mesozoic cenozoic subduction history of the region by integrating independent information from mantle tomography and tectonic reconstructions three different subduction scenarios for the tethyan oceanic lithosphere representative for the available tectonic reconstructions are used to predict the present thermally anomalous volumes associated with the lithospheric surface subducted since the late mesozoic next these predicted thermal volumes and their expected positions are compared to the relevant anomalous volumes derived from seismic tomographic images in this analysis we include among others the possible effects of ridge subduction and slab detachment after the cenozoic continental collisions absolute plate motion and slab thickening in the mantle our preferred subduction model comprises the opening of large back arc oceanic basins within the eurasian margin the model points to slab thickening by a factor of 3 in the mantle in which case the estimated volumes allow for active oceanic spreading 1 2 5 cm yr in the tethyan lithosphere during convergence our results further indicate the occurrence of early oligocene slab detachment underneath the northern zagros suture zone followed by both westward and eastward propagation of the slab tear and diachronous eocene to miocene slab detachment below the eastern to western himalayas free sinking rates of the detached material of 2 cm yr in the lower mantle provide the best fit between the tomographic mantle structure and our tethyan subduction model

repeat ridge jumps associated with plume ridge interaction melt transport and ridge migration 1 repeated shifts or jumps of mid ocean ridge segments toward nearby hot spots can produce large long term changes to the geometry and location of the tectonic plate boundaries ridge jumps associated with hot spot ridge interaction are likely caused by several processes including shear on the base of the plate due to expanding plume material as well as reheating of lithosphere as magma passes through it to feed off axis volcanism to study how these processes influence ridge jumps we use numerical models to simulate 2 d in cross section viscous flow of the mantle viscoplastic deformation of the lithosphere and melt migration upward from the asthenospheric melting zone laterally along the base of the lithosphere and vertically through the lithosphere the locations and rates that magma penetrates and heats the lithosphere are controlled by the time varying accumulation of melt beneath the plate and the depth averaged lithospheric porosity we examine the effect of four key parameters magmatic heating rate of the lithosphere plate spreading rate age of the seafloor overlying the plume and the plume ridge migration rate results indicate that the minimum value of the magmatic heating rate needed to initiate a ridge jump increases with plate age and spreading rate the time required to complete a ridge jump decreases with larger values of magmatic heating rate younger plate age and faster spreading rate for cases with migrating ridges models predict a range of behaviors including repeating ridge jumps much like those exhibited on earth repeating ridge jumps occur at moderate magmatic heating rates and are the result of changes in the hot spot magma flux in response to magma migration along the base of an evolving lithosphere the tendency of slow spreading to promote ridge jumps could help explain the observed clustering of hot spots near the mid atlantic ridge model results also suggest that magmatic heating may significantly thin the lithosphere as has been suggested at hawaii and other hot spots

mid cenozoic post breakup deformation in the passive margins bordering the norwegian greenland sea abstract since the initial breakup of the norwegian greenland sea in early eocene time chron 24b 53 7 ma the conjugate passive margins have been subject to compression extension magmatism and broad uplifts and subsidence mid to late cenozoic compressional doming basin inversion and reverse faulting occurred predominantly offshore within the rheologically weak deep cretaceous depocenters on the norwegian margin the domes seem to have formed primarily in middle eocene to early oligocene and in early miocene while doming in the faroes rockall region developed in late paleocene to early eocene oligocene and mid to late miocene we suggest that the main driving force was plume enhanced ridge push a testable working hypothesis is that discrete phases of compression were associated with periods of high plume flux in addition the oligocene chron 13 35 ma change in plate motion appears to have generated local shear adjustments along pre existing basement weaknesses forming compressional structures in the overlying sedimentary section this change in plate motion was first manifest by significant extension between the sw barents sea and the conjugate nne greenland margin and led to spreading along the knipovitch ridge mid cenozoic extension and magmatism also preceded the development of the kolbeinsey ridge the associated separation of the jan mayen microcontinent from east greenland must have been strongly influenced by the position of the iceland plume center in addition to the change in extension direction with respect to initial breakup of the norwegian greenland sea in early eocene time the mid cenozoic extension and magmatism is a post breakup phenomena widely spaced areas of neogene uplift occurred along all bordering margins these enigmatic uplifted areas acted as nucleation sites for growth of ice caps and initiated large glacial deposits that built out on the adjacent shelves

mesozoic tectono stratigraphic evolution of the seychelles microcontinent abstract the seychelles region developed as a unique continental sliver through the three phases of rift tectonism that since the late permian created the western indian ocean the history of rifting in seychelles can perhaps be traced back to 700 ma when the granites that form the central islands were emplaced the low 18 o of the high temperature minerals within these slightly alkaline granites on mahe indicate an intraplate origin and the fracturing of the lithosphere consequent to their emplacement created a locus of weakness for future rift tectonism to exploit thermally induced extensional rifting initiated during the carboniferous and rekindled in the late permian 225 ma eventually severed super gondwana in the middle jurassic 160 ma into east and west gondwana a proto indian ocean the somali basin which separated east and west gondwana ceased to expand in the early cretaceous 115 ma this rift drift event is recorded in seychelles by block faulted sequences of distal fluviatile through near shore to open marine deposits along its western margin and possibly at farquhar within east gondwana transform rifting then separated madagascar and seychelles india in the late cretaceous at 84 ma a spreading ridge developed between these blocks forming the mascarene basin as a new arm of the evolving indian ocean a thick progradational wedge of sediment initially alluvial followed by lacustro marine and eventually open marine resulted from this event along the southwest seychelles margin finally hotspot related thermally induced rifting causing block faulting and fluviatile to marine deposition eventually separated seychelles from india at the cretaceous tertiary boundary this separation coincided with the deccan volcanic event and the development of the carlsberg spreading ridge which replaced the mascarene spreading ridge and initiated the opening of the northwestern indian ocean basin sedimentation on the seychelles microcontinent throughout the tertiary produced predominantly shelf carbonates

episodicity in back arc tectonic regimes abstract the evolution of back arc basins is tied to the development of the dynamics of the subduction system they are a part of we present a study of back arc basins and model their development by implementing 3d time dependant computer models of subduction including an overriding plate we define three types of episodicity pseudo quasi and hyper episodicity and find evidence of these in nature observations of back arc basin ages histories of spreading quiescence and compression in the overriding plate give us an understanding of the time development of these subduction zones and back arc basins across the globe today a number of trenches are advancing the izu bonin trench the mariana trench the japan trench the java sunda trench and the central portion of the peru chile trench the andes subduction zone the izu bonin mariana and japan all have established back arc basins while the others have documented episodes of spreading quiescence compression or a combination of these the combination of advancing and retreating trench motion places these subduction zones in the category of hyper episodicity quasi episodicity in which the back arc shifts between phases of rifting spreading and quiescence is the dominant form of episodic back arc development in the present we find this type of episodicity in models for which the system is dynamically consistent that we have allowed the subducting plate s velocity to be determined by the sinking slabs buoyancy quasi and hyper episodicity are only found in subduction zones with relatively high subducting plate velocities between 6 and 9 cm year finally those subduction zones for which the subducting plate is moving slowly such as in the mediterranean or the scotia sea experience only pseudo episodicity where the spreading moves linearly towards the trench but often does so in discrete ridge jump events

revision of the timing magnitude and distribution of neogene rotations in the western aegean region to evaluate the dimension and the timing of the clockwise rotating domain and the nature of the structures that accommodate the rotating domain in the western aegean region paleomagnetic analyses were carried out in northern western and southwestern greece the results show that the rotating domain covers an area including the external albanides western mainland greece including evia and probably at least partly the peloponnesos smaller clockwise rotations on the order of 30 408 were reported previously from the chalkidiki peninsula and the islands of skyros and limnos previously two phases of approximately 258 of rotation were suggested the last one during the plio pleistocene our analysis shows that the western aegean domain rotated approximately 408 clockwise between 15 13 and 8 ma followed by an additional 108 after 4 ma the rotating domain is accommodated in the north by deformation associated with the scutari pec fault zone and in the west by the ionian thrust and the hellenic subduction zone to the south no rocks older than 10 ma are available so no conclusive data are obtained to the east of the rotating domain extensional detachment systems of the cyclades and rhodope areas were active during the rotation phase and may explain at least part of the differences in finite amounts of rotation between nonrotation or counterclockwise rotations observed in northern and eastern greece and the large clockwise rotations in western greece d 2004 elsevier b v all rights reserved

volcanism jump and propagation on the sheba ridge eastern gulf of aden segmentation evolution and implications for oceanic accretion processes the rifting between arabia and somalia which started around 35 ma was followed by oceanic accretion from at least 17 6 ma leading to the formation of the present day gulf of aden bathymetric gravity and magnetic data from the encens sheba cruise are used to constrain the structure and segmentation of the oceanic basin separating the conjugate continental margins in the eastern part of the gulf of aden between 51 degrees e and 55 5 degrees e data analysis reveals that the oceanic domain along this ridge section is divided into two distinct areas the eastern area is characterized by a shorter wavelength variation of the axial segmentation and an extremely thin oceanic crust in the western segment a thicker oceanic crust suggests a high melt supply this supply is probably due to an off axis melting anomaly located below the southern flank of the sheba ridge 75 km east of the major alula fartak transform fault this suggests that the axial morphology is produced by a combination of factors including spreading rate melt supply and the edge effect of the alula fartak transform fault as well as the proximity of the continental margin the oceanic domains have undergone two distinct phases of accretion since the onset of seafloor spreading with a shift around 11 ma at that time the ridge jumped southwards in response to the melting anomaly propagating ridges were triggered by the melting activity and propagated both eastward and westward the influence of the melting anomaly on the ridges decreased stopping their propagation since less than 9 ma from that time up to the present the n025 degrees e trending socotra transform fault developed in association with the formation of the n115 degrees e trending segment 2 in recent times a counter clockwise rotation of the stress field associated with kinematic changes could explain the structural morphology of the alula fartak and socotra hadbeen fracture zones

40ar 39ar ages of the sill complex of the karoo large igneous province implications for the pliensbachian toarcian climate change 1 reliable geochronological results gathered so far n 76 have considerably constrained the timing of the emplacement of the karoo large igneous province lip yet strikingly missing from this dating effort is the huge southern sill complex cropping out in the 0 6 106 km2 main karoo sedimentary basin we present 16 new 40ar 39ar analyses carried out on fresh plagioclase and biotite separates from 15 sill samples collected along a n s trend in the eastern part of the basin the results show a large range of plateau and miniplateau ages 176 2 1 3 to 183 8 2 4 ma with most dates suggesting a 3 ma 181 184 ma duration for the main sill events the available age database allows correlation of the karoo lip emplacement with the pliensbachian toarcian second order biotic extinction the global warming and the toarcian anoxic event provided that adequate calibration between the 40k and 238u decay constant is made the mass extinction and the isotopic excursions recorded at the base of the toarcian appear to be synchronous with both the increase of magma emission of the karoo lip and the emplacement of the sills the co2 and so2 derived from both volcanic emissions as well as carbon rich sedimentary layers intruded by sills might be the main culprits of the pliensbachian toarcian climate perturbations we propose that the relatively low eruption rate of the karoo lip is one of the main reasons explaining why its impact on the biosphere is relatively low contrary to e g the camp triassic jurassic and siberia permo triassic lips

plume induced breakup of a subducting plate microcontinent formation without cessation of the subduction process separation of microcontinents is explained by a ridge jump toward the passive margin as a possible consequence of plume induced rheological weakening ultimately leading to breakup followed by accretion of the oceanic crust along a new spreading center in contrast to such a purely extensional case the separation of continental microblocks from the main body of the african plate during its continuous northward motion and subduction under eurasia is still poorly understood our numerical experiments show the thermal and buoyancy effects of mantle plume impingement on the bottom of the continental part of a subducting plate are sufficient to induce separation of an isolated microcontinental block from the main subducting continent even during induced plate motion necessary for uninterrupted oceanic and continental subduction subsequent continental accretion occurs by decoupling upper crustal nappes from the newly formed subducting microcontinent which is in agreement with the late cretaceous eocene evolution of the eastern mediterranean

influences on the positioning of mantle plumes following supercontinent formation several mantle convection studies analyzing the effects of supercontinent formation and dispersal show that the genesis of subcontinental plumes results from the formation of subduction zones at the edges of the supercontinent rather than from the effect of continental thermal insulation or thermochemical piles however the influence of subduction zone location on the position of subcontinental plumes has received little attention this study analyzes 2 d and 3 d numerical models of supercontinent formation in an isochemical mantle to assess the role of subduction and mantle viscosity contrast in the generation of subcontinental mantle plumes we find that once a critical supercontinent width is reached plumes do not form under the center of a supercontinent in studies featuring a low viscosity lower mantle the surface positions of the initial plumes arriving within 90 myr of supercontinent assembly become locked beneath the continent at a distance 2000 3000 km from the continental margin however the broad downwellings in simulations that feature a high viscosity lower mantle trigger plumes at a greater distance from the continental margin subduction for all mantle viscosity profiles subcontinental plumes show dependence on the location of supercontinent margin subduction as theories differ on the role of core mantle boundary chemical piles in plume formation it is significant that our isochemical models show that the formation of subduction zones at the margins of a supercontinent has a profound effect on subcontinental mantle dynamics our results may help to explain what determined the eruption sites of past and future large igneous provinces

basinal autoclastic mass flow regime in the precambrian chanda limestone formation adilabad india abstract the precambrian chanda limestone formation in adilabad district andhra pradesh india transcribes carbonate mass flow deposition in an extensional basin within the godavari rift valley system in the lower part of the formation conglomerate beds which commonly interrupt the sequence of thin bedded lime mud turbidites register pulsatory reinvigoration of mass flow processes these gravelly mass flow products are significant because they indicate i deposition far below the wave base ii intrabasinal origin iii disassociation with any depositional slope like reef margins iv occurrence in discrete vertical packages v clear signals for sediment gravity flows and vi invariable facies successions the conglomerate bodies are extensive parallel to the depositional strike but restricted across the latter the main mode of accretion is dominantly vertical aggradation only the muddy turbidites spreading far and wide into the basin the course of temporal evolution of the mass flows are also interpreted from vertical facies transitions although every flow eventually gave rise to turbidity currents their initial states differred in three distinct ways which are correlated with gradient of the translational slope gradual decrease in declivity of the depositional substrate through time is interpreted

preferential rifting of continents a source of displaced terranes lithospheric rifting while prevalent in the continents rarely occurs in oceanic regions to explain this preferential rifting of continents we compare the total strength of different lithospheres by integrating the limits of lithospheric stress with depth comparisons of total strength indicate that continental lithosphere is weaker than oceanic lithosphere by about a factor of 3 also a thickened crust can halve the total strength of normal continental lithosphere because the weakest area acts as a stress guide any rifting close to an ocean continent boundary would prefer a continental pathway this results in the formation of small continental fragments or microplates that once accreted back to a continent during subduction are seen as displaced terranes in addition the large crustal thicknesses associated with suture zones would ironically make such areas likely locations for future rifting episodes this results in the tendency described as the wilson cycle of new oceans to open along the suture where a former ocean had closed

magnetite microexsolutions in silicate and magmatic flow fabric of the goyozan granitoid ne japan significance of partial remanence anisotropy 1 anisotropy of magnetic susceptibility ams has been widely used to infer magmatic flow patterns of granitoids where an appropriate ams axis is parallel to an alignment of mafic minerals or magnetite the magmatic flow fabric in cretaceous granitic plutons from northeastern japan was verified using an analysis of anisotropy of partial anhysteretic remanent magnetization aparm which further isolates the magnetite subfabrics according to magnetite grain size the preferred orientation of polysynthetic twins in plagioclase laths and clinopyroxene is discordant with the bulk ams fabric along outer marginal zones of the granitoid as shown by image analysis of microphotographs from thin sections cut in orthogonal planes this suggests that the uncorroborated use of bulk ams to detect flow fabric in granitoids has risks scanning electron microscopy sem reveals that submicroscopic needle shaped magnetite inclusions exsolved in anhedral plagioclase and clinopyroxene may explain such anomalous exceptions to the validity of ams fabrics our aparm measurements show that the aparm alignment of relatively high coercive submicroscopic magnetite inclusions is concordant to the linear orientation of anhedral plagioclase and clinopyroxene the combination of sem ams and aparm was required to confirm the magmatic and submagmatic flow pattern of granitoids in this study and is generally preferable to the use of ams alone