Movement of lithospheric plates relative to subduction zones: Formation of marginal seas and active continental margins

Subduction zones with deep seismicity are believed to be associated with the descending branches of convective flows in the mantle and are subordinated to them. Therefore, the position of subduction zones can be considered as relatively fixed with respect to the steady-state system of convective flows. The lithospheric plate overhanging a subduction zone (as a rule of continental type) may:

1. (1) either move away from the subduction zone; or

2. (2) move onto it. In the first case extensional conditions originate behind the subduction zone and the new oceanic crust of back-arc basins forms. In the second case active Andean-type continental margins with thickening of the crust and lithosphere are observed.

Behind the majority of volcanic island-arcs, along the boundary with marginal-sea basins, independent shallow seismicity belts can be traced. They are parallel to the main seismicity belts coinciding with the Benioff zones. The seismicity belts frame island-arc microplates. Island-arc microplates are assumed to be a frame of reference to calculate relative movements of the consuming and overhanging plates. Using slip vector azimuths for shallow seismicity belts in the frontal parts of the Kurile, Japan, Izu-Bonin, Mariana and Tonga—Kermadec arcs, the position of the pole of rotation of the Pacific plate with respect to the western Pacific island-arc microplates was computed. Its coordinates are 66.1°N, 119.2°W. From the global closure of plate movements it has been determined that for the past 10 m.y. the Eurasian and Indian plates have been moving away from the Western Pacific island-arc system, both rotating clockwise, around poles at 31.1°N, 164.2°W and 1.3°S, 157.5°W, respectively. This provides for the opening of the back-arc basins. At the same time South America is moving onto the subduction zone at the rate of 4 cm/yr. Some “hot spots”, such as Hawaiian, Tibesti, and those of the South Atlantic, are moving relative to the island-arc system at a very low rate, viz. 0.5–0.7 cm/yr. Presumably, the western Pacific subduction zone and “hot spots” form a single frame of reference which can generally be used for the analysis of absolute motions.     

The Pelusium Line—a major transcontinental shear

The Pelusium Line, which was defined by Neev (1975) off the Mediterranean coast of Israel, is suggested to form a transcontinental arcuate shear which extends along the following three segments:

1. (A) from Anatolia along the eastern Mediterranean down to the eastern limit of the Nile Delta;

2. (B) across Africa down to the Niger Delta; and

3. (C) across the Mid-Atlantic Ridge along the equatorial fracture zones.

A “Central Plate”, composed of South and East Africa and the Arabian and Sinai subplates, has been left laterally shifted along the Pelusium Line relative to the Northwest African Plate.     

Rheologic properties of the lithosphere and applications to passive continental margins

Thermal and petrologic models of the crust and upper mantle are used for calculating effective viscosities on the basis of constant creep rates. Viscosity—depth models together with pressure—depth models are calculated for continental and oceanic blocks facing each other at continental margins. It is found from these “static models” that the overburden pressure in the lower crust and uppermost mantle causes a stress which is directed from the ocean to the continent. The generally low viscosity of 10²⁰–10²³ poise in this region should permit a creep process which could finally lead to a “silent” subduction. In the upper crust static stresses act in the opposite direction, i.e. from the continent to the ocean, favouring tension which could produce normal faulting in the continent. Differences between observations and the results obtained from the static models are attributed to dynamical forces.     

Diffuse magnetic anomalies in marginal basins: Their possible tectonic and petrologic significance

Marginal basins, areas of oceanic lithosphere peripheral to large ocean basins, may be formed by several processes, but the young active marginal basins have the geophysical and geochemical characteristics of young normal oceanic lithosphere. We recognize two distinct tectonic settings in which new oceanic lithosphere may be formed in areas which would be termed marginal basins:

1. (1) Upwelling of fractional melts of mantle material from the region above subducted lithospheric slabs leads to the generation of new oceanic lithosphere behind island arcs. The general case for this tectonic setting involves random location of magma leaks and does not produce correlatable magnetic anomalies. In special cases, an orthogonal ridge—transform system may duplicate the magnetic patterns found on ocean-basin crust.

2. (2) The second tectonic setting develops on very long “leaky” transform faults separating spreading ridges. In areas where the transform has dislocated a block of continental crust, or an island arc, the map view of the resulting marginal basin may resemble the setting of a basin behind an active island arc. However, the “leaky” transform setting is unrelated to active plate convergence or to Benioff zones.

At “normal” ridge-crests, and possibly in some marginal basins, basalt is erupted on long linear magma leaks and rapid cooling forms thick lithosphere with correlatable linear magnetic anomalies. Some marginal basins have high thermal flux, spread slowly and may have thick sediment cover. Slow cooling, numerous point-source magma leaks and extensive hydrothermal alteration diminish magnetic intensities and cause diffuse magnetic patterns. The correlation problems caused by diffuse magnetic anomalies make interpretations of spreading rates and directions in young marginal basins a difficult, if not futile, task.It is likely that fragments of marginal-basin lithosphere form some of the ophiolite complexes; their recognition is critical to paleo-tectonic interpretations. The geochemical characteristics of marginal-basin basalts do not appear to be useful criteria for distinguishing them from ocean-ridge basalts. However, the abundance of short ridges and seamounts in many young marginal basins suggests that an abundance of seamount material, as well as differentiated volcanic and plutonic rocks, in ophiolites may be an indication of derivation from marginal-basin lithosphere.     

Statistical analysis of geodetic measurements for the investigation of crustal movements

Geodetic networks are designed to obtain data that can be used to monitor crustal movements. The relative position on the earth's surface is determined from these networks by means of coordinates. The coordinates of stations and its variance—covariance matrix are based on the computational model. In spatial networks at least three points, the base points, should be chosen to define the coordinate system “fixed” to the earth. In monitoring crustal movements these base points are considered to be stationary over the time span of the motion involved. A procedure for testing the stability of the base points, together with other stable points, is described.The coordinate differences between two time epochs, t₀ and t₁ are considered to investigate crustal movements. A statistical test is introduced to determine whether crustal movements have actually occurred.The reliability, i.e., the influence, of nondetected errors in the observations or computations, should be considered. Two types of decisions can be made which may lead to incorrect conclusions. These conclusions are as follows:

1. (1) That no movement has taken place, although a nondetected error leads to the opposite conclusion.

2. (2) That a movement has occurred, although a nondetected error in the observations leads to the opposite conclusion.

The chance of arriving at these conclusions can be computed. Boundary values for assumed crustal motion in specified latitudinal and longitudinal directions give a better insight into the desired specifications for geodetic networks.The testing procedure and the above-mentioned method of computing boundary values can be used for all types of networks e.g., those obtained by conventional triangulation or by a satellite-borne ranging system.     

Stress and viscosity in the asthenosphere

Stresses and effective viscosities in the asthenosphere to a depth of 400 km are calculated on the basis of Weertmans “temperature method” i.e., on relating viscosity to the ratio of the temperature to the melting point (=homologous temperature). Some oceanic and continental geotherms and two melting point—depth curves, the dry pyrolite solidus and the forsterite₉₀ melting curve are used for the conversion of the homologous temperature to the effective viscosity. Two creep laws are considered, the linear, grain-size-dependent Nabarro—Herring (NH) creep law, and a power creep law, in which the creep rate is proportional to the third power of the stress. A plate tectonic model yields creep rates of 2 · 10⁻¹⁴ s⁻¹ for the oceanic and 3 · 10⁻¹⁵ s⁻¹ for the continental asthenosphere. These values are held constant for the calculations and may be valid for regions inside plates.The dry pyrolite mantle model results in high homologous temperatures in the asthenosphere below oceans (0.9), very low stresses (a few bars and lower) and shows a low viscosity “layer” of about 200-km thickness. Below continental shields the homologous temperature has a maximum value of 0.73, stresses are around 5–20 bar and the low-viscosity region is thicker and less pronounced than in the oceanic case. The Fo₉₀ mantle model generally gives lower homologous temperatures (maximum value below oceans beside active ridges 0.75). The stresses in the asthenosphere beneath oceans vary from a few bars to about 50 bar and below continents to about 100 bar. The low-viscosity region seems to reach great depths without forming a “channel”. The Figs. 1 and 2 show the approximate viscosity—depth distribution for the two mantle models under study.Assuming a completely dry mantle and a mean grain size of 5 mm, power law creep will be the dominating creep process in the asthenosphere. However, grains may grow in a high-temperature—low-stress regime (i.e., below younger oceans), an effect which will further diminish the influence of NH creep. In the upper 100–150 km of the earth some fluid phases may affect considerably creep processes.     

Physical conditions producing slab stagnation: Constraints of the Clapeyron slope, mantle viscosity, trench retreat, and dip angles

Recent seismic tomography has revealed various morphologies in the subducted lithosphere. In particular, significant flattening and stagnation of slabs around the 660-km boundary are seen in some areas beneath the northwestern Pacific subduction zones. We examined the cause of slab stagnation in terms of the Clapeyron slope of the phase transformation from ringwoodite to perovskite + magnesiowüstite, trench retreat velocity, dip angles, and high viscosity of the lower mantle based on two-dimensional (2-D) numerical simulations of thermal convection. In particular, we examined the conditions necessary for slab stagnation assuming a very small absolute value of the Clapeyron slope, which were proposed based on recent high-pressure, high-temperature (high P–T) experiments. Our calculations show that slabs tend to stagnate above the 660-km boundary with an increasing absolute value of the Clapeyron slope, viscosity jump at the boundary, and trench retreat velocity and a decreasing initial dip angle. Stagnant slabs could be obtained numerically for a realistic range of parameters obtained from high P–T experiments and other geophysical observations combining buoyancy, high lower-mantle viscosity, and trench retreat. We found that a low dip angle of a descending slab at the bottom of the upper mantle plays an important role in slab stagnation. Two main regimes underlie slab stagnation: buoyancy-dominated and viscosity-dominated regimes. In the viscosity-dominated regime, it is possible for slabs to stagnate above the 660-km boundary, even when the value of the Clapeyron slope is 0 MPa/K.     

Experimental deformation of diopside and websterite

Diopside single-crystals, oriented favorably for twin gliding on both systems: (001) [100] and (100)[001] have been deformed in a Griggs apparatus using talc as pressure medium. The latter mechanism is dominant at temperatures (T) below 1050° C at strain rates () of 10⁻³ sec⁻¹, and below 800° C at ; at higher temperatures translation gliding on (100)[001] accompanied by syntectonic recrystallization is dominant but other glide systems also operate. Tests at a single set of conditions, T- and -incremental tests and stress-relaxation experiments have been carried out on websterite (68% CPX, 32% OPX), both in talc (“wet”) and talc-AlSiMag (“dry”) assemblies. Most tests were performed in the high-T regime, where syntectonic recrystallization and “relatively nonselective” glide are dominant. The mean size of recrystallized clinopyroxenes (D, μm) appears to be related to stress (σ, kb) as D = 60σ^−0.9. The mechanical data fit the power law exp(-Q/RT)σⁿ, where for the “wet” experiments A = 10^5.9kb⁻ⁿsec⁻¹, Q = 91.2 kcal/mole, n = 5.3; for σ < 3.5 kb n appears to decrease to 3.3. For the “dry” experiments A = 10^2.2, Q = 77.9, and n = 4.3 for σ < 7.0 kb. Clinopyroxene in the upper mantle occurs as ca. 0–15% mixed phase in peridotites and websterites occur as thin layers. Stresses in these materials will then be near those in the olivine-rich matrix. At , the equivalent viscosity of dry websterite is less than that of dry dunite at depths to 60 km but it increases rapidly at higher pressures; at 240 km it is 10⁶ greater than that of dunite. This may account for the low strains and passive behavior observed for clinopyroxene crystals in most peridotites and websterites, that presumably have formed at great depth. Attenuated folds of websterite in peridotite—evidence of more ductile behavior—may then have formed at shallower levels; alternatively they may have formed under “wet” conditions.     

Gradational thresholds and landform singularity: Significance for Quaternary studies

Geomorphic threshold conditions have been identifed at which stream patterns change and gully initiation occurs. For both, the threshold conditions are defined by the parameter of “relative shear stress” which is a measure of the energy state of the system and is based on known values of stream slope and mean annual discharge (for patterns) or drainage area (for gullies). The probability of passing from a stream pattern to another, or from stable to gullied valley floors, is a smooth function of relative shear stress and so the thresholds separating the different states of the geomorphic systems are gradational. The singularity of landforms prevents the identification of a sharp threshold, and as a result landform sensitivity will differ within the same area and under the same conditions. Therefore, geomorphic predictions and postdictions will be uncertain, and Quaternary correlations will lack precision.     

Plate motion and thermal instability in the asthenosphere

This paper investigates the effect of shear heating in the asthenosphere on the thermal structure of the upper mantle. Equations describing the motion of the lithosphere over the asthenosphere in the presence of a strongly temperature-dependent stress-strain rate relation are derived and solved with the help of several approximations. These approximations are shown to be valid under conditions appropriate for the earth.Two sets of solutions are found. For one set (the “subcritical” solutions) a normal shear stress—velocity relation is found for small stresses. The velocity increases as the stress increases, reaching a maximum velocity σ_c for a critical stress σ_c. The subcritical solutions have a negligible effect on the thermal structure of the earth, even at the critical stress. The other set of solutions (the “supercritical” solutions) has the bizarre property that a decrease of applied shear stress leads to an increase of velocity. Thus, as the shear stress goes to zero, the velocity becomes infinite. At larger shear stresses the velocity decreases until it reaches σ_c at a stress σ_c (the two sets of solutions share this point in common). There are no steady solutions of any kind for shear stresses in excess of σ_c. We discard the supercritical solutions as candidates for the thermal structure of the earth on the basis of their instability to small perturbations of applied stress and temperature.The realm of subcritical solutions (stress less than σ_c, velocity less than σ_c) thus defines a regime of plate motion in which the thermal effects of shear heating are negligible. If the shear stresses acting on plates exceed σ_c, however, new physical processes must come into play to dissipate the excess heat generated. Assuming that the velocities of plates on the earth today are less than σ_c, relative to the deep mantle, a strict upper limit of a few tens of bars can be derived for σ_c, corresponding to effective viscosities of ca. 10¹⁹ poise in the asthenosphere.     

Transgressions-régressions, variations eustatiques et influences tectoniques de l'Aptien au Maastrichtien dans le Bassin de Paris occidental et sur la bordure du Massif armoricain

La série sédimentaire du Crétacé moyen et supérieur étudiée dans l'Ouest du Bassin de Paris et sur la bordure du Massif armoricain comporte sept pulsations transgressives qui peuvent être reconnues en fonction de la disposition géomètrique des dépôts et de l'enchaînement vertical des faciès.Les épisodes transgressifs atteignent leur phase paroxysmale, en alternance avec des stades de régression, successivement:

1. (1) à la fin de l'Aptien supérieur —(régression début Albien)

2. (2) au milieu de l'Albien supérieur —(régression fin Albien-début Cénomanien)

3. (3) au milieu du Cénomanien inférieur —(régression fin Cénomanien inférieur)

4. (4) à la fin du Cénomanien moyen —(régression fin Cénomanien)

5. (5) au milieu du Turonien inférieur —(régression du Coniacien)

6. (6) au Santonien puis Campanien —(régression fin Campanien)

7. (7) au Maestrichtien —(régression fin Maastrichtien)

Ces dépôts crétacés présentent une succession de séquences séparées par des discontinuités et des surfaces d'érosion plus ou moins marquées. Les caractères et la répartition de ces séquences sont analysés en domaine de sédimentation terrigène littorale et dans le bassin envahi par la craie. Il est alors tenté d'interpréter les variations bathymétriques d'une part en fonction d'évènements tectoniques locaux, d'autre part en relation avec des variations eustatiques plus générales.Middle and Upper Cretaceous deposits studied in the western Paris Basin and on the Armorican Massif margin show seven transgressive pulses that can be detected in the geometrical arrangement of the sedimentary bodies and the vertical succession of facies.The transgressive episodes, each delimited by a regressive phase, reached their peak during:

1. (1) late Late Aptian —(Early Albian regression)

2. (2) mid Late Albian —(Late Albian-Early Cenomanian regression)

3. (3) mid Early Cenomanian —(late Early Cenomanian regression)

4. (4) late Middle Cenomanian —(Late Cenomanian regression)

5. (5) mid Early Turonian —(Coniacian regression)

6. (6) Santonian-Campanian —(Late Campanian regression)

7. (7) Maastrichtian —(Late Maastrichtian regression)

The Cretaceous sediments occur as a series of sequences, separated by more or less important discontinuities and erosion surfaces. The features and distribution of these sequences have been studied in the nearshore region of terrigenous sedimentation and in the Chalk basin. An attempt is made to relate the bathymetric changes to either tectonic movements or more widespread eustatic oscillations.     

Evidence for cyclic reactions between andalusite, “sericite” and sillimanite, mount franks area, willyama complex N.S.W

In the Mt. Franks area of the Willyama Complex, microfabric evidence suggests that the alteration of andalusite to sillimanite has taken place by a process similar to that suggested by Carmichael (1969). Andalusite is pre- to syn-S₂ in age. Alteration to “sericite” has resulted in the formation of “sericite” laths, some of which are crenulated about S₂, and some which are syn- and post-S₂. “Fibrolite” occurs in these andalusite—“sericite” aggregates within the sillimanite zone and is wholly embedded in “sericite”. “Fibrolite” is pre- to syn-S₂ in age. This evidence is interpreted as suggesting that the formation of sillimanite from andalusite took place via a “sericite” phase.Further microfabric observations are interpreted to imply constant volume for the reaction aluminosilicate → “sericite”. This suggests a situation in which Al³⁺ is relatively mobile but Al⁴⁺ is relatively immobile. This suggestion differs from Carmichael's (1969) idea of Al³⁺ immobility.     

The Cenomanian/Turonian Boundary Event (CTBE) at Wunstorf, north-west Germany, as reflected by marine palynology

The Cenomanian/Turonian Boundary Event (CTBE) at Wunstorf, north-west Germany, has been analysed palynologically by high resolution sampling to reconstruct changes in relative sea-level and water mass character within photic zone waters. Based on changes in the ratio of terrigenous sporomorphs to marine palynomorphs (t/m index), the distribution of the organic-walled algal taxa as well as of selected dinocyst taxa and groups the section can largely be subdivided into pre-“plenus-bed” and post-“plenus-bed” intervals, reflecting different stages of third-order relative sea-level cycles and/or changes in water mass influence in the photic zone. Accordingly, the pre-“plenus-bed” interval is placed in a transgressive systems tract starting at the “facies change” event (C. guerangeri/M. geslinianum ammonite Zone boundary) with the maximum flooding surface at the top of the “Chondrites II” bed (top of R. cushmani Biozone). A highstand systems tract is suggested from the base of the “plenus-bed” up the base of the “fish-shale” event. Within the “fish-shale” event interval, a transgressive systems tract is suggested to start at the base of the thin, grey-green marly interbed. The Cenomanian/Turonian boundary proper, as defined by the first occurrence of Mytiloides spp., as well as the lowermost Turonian are located within the initial phase of a transgressive systems tract. With respect to water mass characteristics within photic-zone waters, the pre-“plenus-bed” interval is predominantly characterized by warm water masses that changed gradually towards the deposition of the “Chondrites II” bed, where a strong influence of cool and/or salinity-reduced waters is indicated by various palynological proxies. Within the post-“plenus-bed” interval a mixture and/or alternation of warmer and cooler waters is indicated, with the warmer water influence increasing gradually towards and within the Lower Turonian stage. The increased proportions of prasinophytes within the “Chondrites II” bed and parts of the “fish-shale” interval may indicate availability of reduced nitrogen chemospecies, especially ammonium, within photic-zone waters as a function of a vertical expansion of the oceanic O₂-minimum zone.     

Observations of the electrical asthenosphere beneath Scandinavia

The recent recognition that long period (i.e., of the order of hours) electromagnetic induction studies could play a major role in the detection of the asthenosphere has led to much interest amongst the geophysical and geological communities of the geomagnetic response functions derived for differing tectonic environments. Experiments carried out on the ocean bottom have met with considerable success in delineating the “electrical asthenosphere”, i.e., a local maximum in electrical conductivity (minimum in electrical resistivity) in the upper mantle.In this paper, observations of the time-varying magnetic field recorded in three regions of Scandinavia, northern Sweden (Kiruna—KIR), northern Finland/northeastern Norway (Kevo—KEV) and southern Finland (Sauvamaki—SAU), are analysed in order to obtain estimates of the inductive response function, C(ω), for each region. The estimated response functions are compared with one from the centre of the East European Platform (EEP), and it is shown that the induced eddy currents, at periods of the order of 10³–10⁴ s, in the three regions flow much closer to the surface than under the platform centre. Specifically, at a period of ~3000 s, these currents are flowing at depths of the order of: KEV—120 km; KIR—180 km; SAU—210 km; EEP—280 km; implying that the transition to a conducting zone, of σ -0.2 S/m, occurs at around these depths. One-dimensional inversion of and shows that there must exist a good conducting zone, of σ = 0.1–1.0 S/m, under each of the two regions, of 40 km minimum thickness, at depths of: KEV 105–115 km; KIR 160–185 km. This is to be contrasted with EEP, where the ρ-d profile displays a monotonically decreasing resistivity with depth, reaching σ~0.1 S/m at > 300 km.Finally, a possible temperature range for the asthenosphere, consistent with the deduced conducvitity, is discussed. It is shown that, at present, there is insufficient knowledge of the conditions (water content, melt fraction, etc.) likely to prevail in the asthenosphere to narrow down the probable range of 900°–1500°C.     

Facies and genesis of Carboniferous coal seams of Northwest Germany

In order to get detailed information about the facies and genesis of Upper Carboniferous coal seams of Northwest Germany, maceral analyses of complete seam profiles (Westphalian B-D, mainly Westphalian C) were carried out. Four main facies and twelve subfacies could be distinguished. The main facies are:

1. (1) The sapropelic-coal facies, consisting of fine-grained inertinite and liptinite, which forms from organic sediments deposited at the bottom of moor lakes.

2. (2) The densosporinite facies which is high in inertinite and liptinite and low in vitrinite. Syngenetic pyrites, clastic layers, thick vitrains and fusains do not occur. This facies originates from peats of ‘open mires’ with higher groundwater table and herbaceous vegetation. The ‘open mire’ was situated in the centre of extensive swamps. Consequently, clastic sedimentation did not affect this swamp type and nutrient supply and pH values were low.

3. (3) The vitrinite-fusinite facies, which is high in vitrinite. This is the result of abundant vitrains. Under the microscope, fusains were mostly identified as fusinite. The vitrinite-fusinite facies originates from a forest mire. More or less abundant seam splits and clastic layers show that rivers flowed in the neighbourhood of this area.

4. (4) The shaly-coal facies, which represents the most marginal part of the former swamp frequently affected by clastic sedimentation.

Within the Carboniferous of the Ruhr Region it seems unlikely that the thin coal seams of the Namurian C and Westphalian A1 contain a densosporinite facies. The swamps were situated in the lower delta plain where they were often affected by marine influences. Consequently, coals are high in minerals and sulfur and they are thin and discontinous. The best conditions for the formation of extensive swamps, with open mires (densosporinite facies) in their central parts, prevailed during Westphalian A2 and B1 times. Low contents of sulfur and minerals and high content of inertinite are typical for these coals. Sedimentation mainly took place in the transitional zone from the lower to the upper delta plain. During the Westphalian B2 and C fluvial sedimentation dominated. Within the coal seams minerals, sulfur and pseudovitrinite increase while inertinite decreases. This is the consequence of coal of the densosporinite facies occurring with increased rarity. The coal seams of the Westphalian C2 contain no densosporinite facies because peat formation was restricted by increasing fluvial sedimentation and by a better drainage. As a consequence, extensive swamps with ‘open mires’ in the centre were no longer formed after the formation of the “Odin” seams. Above the “Odin” seams coal of the vitrinite-fusinite facies contains thick-walled torisporinites. Variations and lowering of the groundwater table caused mild oxidative influences during peat formation. This is documented by an increase in pseudovitrinite, the occurrence of torisporinites and the absence of spheroidal sideritic concretions. Sulfur content increases in the absence of the low-ash and low-sulfur coal of the densosporinite facies.In Upper Carboniferous coal seams of the Ibbenbüren Region the inertinite and telocollinite contents are higher than in those of the Ruhr Region. Therefore, variations of the groundwater table have been more pronounced and resulting oxidative influences must have been more severe. Seldom occurring marine and brackish horizons and a higher fusinite (fusain) content indicate a slight elevation of this area. From Early Westphalian D times onward, peat formation was no longer possible because of the better drainage. This resulted in severe oxidative conditions which excluded peat formation.     

Lithosphere structure of European sedimentary basins from regional three-dimensional gravity modelling

A three-dimensional (3D) density model, approximated by two regional layers—the sedimentary cover and the crystalline crust (offshore, a sea-water layer was added), has been constructed in 1° averaging for the whole European continent. The crustal model is based on simplified velocity model represented by structure maps for main seismic horizons—the “seismic” basement and the Moho boundary. Laterally varying average density is assumed inside the model layers. Residual gravity anomalies, obtained by subtraction of the crustal gravity effect from the observed field, characterize the density heterogeneities in the upper mantle. Mantle anomalies are shown to correlate with the upper mantle velocity inhomogeneities revealed from seismic tomography data and geothermal data. Considering the type of mantle anomaly, specific features of the evolution and type of isostatic compensation, the sedimentary basins in Europe may be related into some groups: deep sedimentary basins located in the East European Platform and its northern and eastern margins (Peri-Caspian, Dnieper–Donets, Barents Sea Basins, Fore–Ural Trough) with no significant mantle anomalies; basins located on the activated thin crust of Variscan Western Europe and Mediterranean area with negative mantle anomalies of −150 to −200×10⁻⁵ ms⁻² amplitude and the basins associated with suture zones at the western and southern margins of the East European Platform (Polish Trough, South Caspian Basin) characterized by positive mantle anomalies of 50–150×10⁻⁵ ms⁻² magnitude. An analysis of the main features of the lithosphere structure of the basins in Europe and type of the compensation has been carried out.     

Structure of the lithosphere beneath the Eastern Alps (southern sector of the TRANSALP transect)

The interpretation of the seismic Vibroseis and explosive TRANSALP profiles has examined the upper crustal structures according to the near-surface geological evidences and reconstructions which were extrapolated to depth. Only the southern sector of the TRANSALP transect has been discussed in details, but its relationship with the whole explored chain has been considered as well. The seismic images indicate that pre-collision and deep collision structures of the Alps are not easily recognizable. Conversely, good records of the Neo-Alpine to present architecture were provided by the seismic sections.Two general interpretation models (“Crocodile” and “Extrusion”) have been sketched by the TRANSALP Working Group [2002]. Both illustrate the continental collision producing strong mechanical interaction of the facing European and African margins, as documented by giant lithosphere wedging processes. Arguments consistent with the “Extrusion” model and with the indentation of Adriatic (Southalpine) lithosphere underneath the Tauern Window (TW) are:

– According to the previous DSS reconstructions, the Bouguer anomalies and the Receiver Functions seismological data, the European Moho descends regularly attaining a zone south of the Periadriatic Lineament (PL). The Moho boundary and its geometry appear to be rather convincing from images of the seismic profile;

– the Tauern Window intense uplift and exhumation is coherent with the strong compression regime, which acted at depth, thus originating the upward and lateral displacement of the mobile and ductile Penninic masses according to the “Extrusion” model;

– the indentation of the Penninic mobile masses within the colder and more rigid Adriatic crust cannot be easily sustained. Wedging of the Adriatic stiffened lower crust, under high stresses and into the weaker Penninic domain, can be a more suitable hypothesis. Furthermore, the intrusion of the European Penninic crustal wedge underneath the Dolomites upper crust is not supported by any significant uplifting of the Dolomites. The total average uplift of the Dolomites during the Neogene appears to be 6−7 times smaller than that recognized in the TW. Markedly the northward dip of the PL, reaching a depth of approximately 20 km, is proposed in our interpretation;

– finally, the Adriatic upper crustal evolution points to the late post-collision change in the tectonic grow-up of the Eastern Alps orogenic chain. The tectonic accretion of the northern frontal zone of the Eastern and Central Alps was interrupted from the Late Miocene (Serravallian–Tortonian) onward, as documented by the Molasse basin evolution. On the contrary, the structural nucleation along the S-vergent tectonic belt of the eastern Southern Alps (Montello–Friuli thrust belt) severely continued during the Messinian and the Plio–Pleistocene. This structural evolution can be considered to be consistent with the deep under-thrusting and wedge indentation of the Adriatic lithosphere underneath the southern side of the Eastern Alps thrust-and-fold belt.

Similarly, the significance of the magmatic activity for the construction of the Southern Alps crust and for its mechanical and geological differentiation, which qualified the evolution of the thrust-and-fold belt, is highlighted, starting with the Permian–Triassic magmatism and progressing with the Paleogene occurrences along the Periadriatic Lineament and in the Venetian Magmatic Province (Lessini–Euganei Hills).     

Senescence- and death-related alteration of chlorophylls and carotenoids in marine phytoplankton

This report extends previous work ([Louda et al., 1998a] and [Louda et al., 1998b]. Chlorophyll degradation during senescence and death. Organic Geochemistry 29, 1233–1251.) in which we detailed type-I (alteration) and -II (destruction) degradation of chlorophyll with representative fresh water phytoplankton. The present study covers similar experiments with marine phytoplankton, namely, a cyanobacterium (“ANA” Anacystis sp), a coccolithophore (“COC” Coccolithophora sp.), a dinoflagellate (“GYM” Gymnodinium sp.) and two diatoms (“CYC” Cyclotella meneghiniana and “THAL” Thalassiosira sp.). Mg loss (‘pheophytinization') was rapid and continuous in all species under room-oxic conditions and slow or sporadic under anoxic conditions. The proportion of dephytylated pigments (pheophorbides-a, chlorophyllides-a), relative to the phytylated forms (chlorophyll-a, pheophytins-a), increased over the first year under room-oxic conditions and in room-anoxic conditions only in “CYC”. Pheophorbide-a was converted to pyropheophorbide-a within 15 months only in “THAL” and “ANA”, and slightly in “COC”. After 9–15 months of oxic incubation, “COC” was found to contain traces of purpurin-18 phytyl ester. Consideration of carotenoid pigments is also included herein. All fucoxanthin containing species, except “THAL”, exhibited conversion of fucoxanthin to fucoxanthinol in room-oxic conditions. Diadinoxanthin was rapidly de-epoxidized to give diatoxanthin within the first 2–4 weeks. Diatoxanthin then disappeared from all species by 15 months with a concurrent increase in a pigment which we tentatively identify as a cis-zeaxanthin. Incubations of pure cultures are found to be an effective way by which to model the early type-I reactions for both chlorophylls and carotenoids. The influence of oxygen during senescence-death and the onset of early diagenesis is of paramount importance. The absence of oxygen and, by inference, aerobic microbiota, retards the breakdown of these pigments dramatically.     

Late-Cenozoic Magnetostratigraphy : Comparisons with Bio-, Climato-, and Lithozones

A workshop conference entitled “Late Cenozoic Magnetostratigraphy: Comparisons with Bio-, Climato-, and Lithozones” took place in Tokyo and Otsu, Japan, between October 28 and November 1, 1974. It was organized by G. J. Kukla and H. Nakagawa as an outcome of the PA-70-17 Project of the International Geological Correlation Programme, launched in 1970 by the International Union of Geological Sciences. The workshop was supported by the Japanese Society for the Promotion of Science, by IGCP, and the National Science Foundation (of the United States). Out of 70 participating geophysicists, geologists, and paleontologists, 37 attended in person, while the remaining 33 contributed by mail.¹ Prior to the conference a questionnaire was distributed in order to collect opinions on several issues. The workshop's objective was to tackle problems in the recognition of depositional polarity and to review the relationship of magneto-stratigraphic units with radiometric data and with regional bio-, litho-, and climatostratigraphic systems of the Pliocene and Pleistocene. The principal conclusions of the conference were summarized as follows:

1. (1) The only practical (though not infallible) way of demonstrating the validity of interpreted depositional polarity and magnetostratigraphic zonation is to reproduce the results in parallel, widely separated sections with different lithology and sedimentation rates.

2. (2) The hazard of unrecognized postdepositional normal overprints must be recognized and considered in all attempted correlations. Multiple sampling of parallel sections and consistency checks of magnetic data are a prerequisite for correct results.

3. (3) Continuous sequences with high sedimentation rates, such as those which originated in subsiding basins, are viewed as prospective candidates for international stratotypes of the Pliocene and Pleistocene. The investigation of such deposits should be accelerated.

4. (4) Magnetostratigraphy must follow basic stratigraphic principles. Magnetic zones should be clearly defined and locally labeled, whether or not their correlation with paleomagnetic chronology appears possible.

5. (5) Improved data on absolute age of reversals are needed. For that purpose, multiple K/Ar and fission-track analyses of key volcanic layers should be performed on a continuing basis.

     

Results of Scripps long range profiles in the Pacific

During 1976 the first installment of a long range seismic profile was conducted in the North Pacific to a range of 600 km using shots to two tons in size. The line was shot to a closely-spaced array of Scripps ocean bottom seismographs and was parallel to magnetic anomaly 32 at an age of approximately 70 · 10⁶ yr. The line extended between the Clarion and Molokai Fracture Zones and did not cross any major topographic features. Linearized and extremal travel-time inversions were conducted to provide bounds on the compressional velocity as a function of depth. The velocity does not exceed 8.4 km s⁻¹ to a depth of 60 km at which point the data no longer provide any resolution. The constraints on the acceptable models were improved by using array processing methods to measure phase velocity and synthetic seismogram techniques to model phase and amplitude information. The oceanic crust is composed of a series of gradients with no first order discontinuities. The “Moho” is smeared out over a depth of 1.5–2.0 km even though “wide-angle reflections” from the Moho, the phase P_MP, are clearly seen in the data. The upper lithosphere is characterized by a general tendency for the velocity to decrease with depth and the tendency is occasionally overwhelmed (at about 27 and 52 km depth) by rapid velocity changes perhaps associated with phase or compositional changes.