The varved sediment of Lake Suigetsu (central Japan) provides a valuable opportunity to obtain high‐resolution, multi‐proxy palaeoenvironmental data across the last glacial/interglacial cycle. In order to maximize the potential of this archive, a well‐constrained chronology is required. This paper outlines the multiple geochronological techniques being applied – namely varve counting, radiocarbon dating, tephrochronology (including argon–argon dating) and optically stimulated luminescence (OSL) – and the approaches by which these techniques are being integrated to form a single, coherent, robust chronology. Importantly, we also describe here the linkage of the floating Lake Suigetsu (SG06) varve chronology and the absolute (IntCal09 tree‐ring) time scale, as derived using radiocarbon data from the uppermost (non‐varved) portion of the core. This tie‐point, defined as a distinct (flood) marker horizon in SG06 (event layer B‐07–08 at 1397.4 cm composite depth), is thus derived to be 11 255 to 11 222 IntCal09 cal. years BP (68.2% probability range). 相似文献
The major scope of the study is the assessment of landslide susceptibility of Flysch areas including the Penninic Klippen in the Vienna Forest (Lower Austria) by means of Geographical Information System (GIS)-based modelling. A statistical/probabilistic method, referred to as Weights-of-Evidence (WofE), is applied in a GIS environment in order to derive quantitative spatial information on the predisposition to landslides. While previous research in this area concentrated on local geomorphological, pedological and slope stability analyses, the present study is carried out at a regional level. The results of the modelling emphasise the relevance of clay shale zones within the Flysch formations for the occurrence of landslides. Moreover, the distribution of mass movements is closely connected to the fault system and nappe boundaries. An increased frequency of landslides is observed in the proximity to drainage lines, which can change to torrential conditions after heavy rainfall. Furthermore, landslide susceptibility is enhanced on N-W facing slopes, which are exposed to the prevailing direction of wind and rainfall. Both of the latter geofactors indirectly show the major importance of the hydrological conditions, in particular, of precipitation and surface runoff, for the occurrence of mass movements in the study area. Model performance was checked with an independent validation set of landslides, which are not used in the model. An area of 15% of the susceptibility map, classified as highly susceptible, “predicted” 40% of the landslides. 相似文献
Oxygen isotope analyses of 101 samples from the Marcy Anorthosite Massif (61 from this study, 40 from Taylor 1969), indicate that two major and distinct processes of crustal contamination have affected the massif. Ninety percent of the 93 samples with over 65% plagioclase are enriched in 18O by 2.6 relative to normal anorthosites or gabbros: the average 18O for 83 enriched samples is 9.5 Depletions in 18O occur in 8% of the samples which have values ranging from 3.0 to 5.8 Only 2 of the samples fall within the normal magmatic range for anorthosites.Low 18O values of 3.0 to 5.8 in the anorthosite occur only near contacts, and a gradient in 18O occurs near the contact within the border zone of the massif. Low 18O values in both the anorthosite and adjacent wollastonite skarns (with 18O down to –1.3) were probably caused by isotopic exchange with heated meteoric water when the anorthosite intruded at shallow levels, prior to Grenvilleage ( 1.1 by) granulite facies metamorphism.The 18O-enrichment was ascribed to exchange between anorthosite and 18O-rich marble by means of a pervasive, H2O-CO2 fluid during the regional metamorphism by Taylor (1969). However, a number of lines of evidence argue against this hypothesis: 1) the preservation of premetamorphic low 18O values in anorthosite from the border zone as well as preserved gradients in 18O from a number of localities, 2) mass balance calculations of the amount of marble necessary to produce the 18O enrichment 3) metamorphic phase equilibria which buffer
and
to low values, and, 4) recent oxygen isotope analyses show homogeneity which indicates that magmatic oxygen isotope compositions have been preserved. We evaluated the importance of magmatic assimilation of country rock at the present level of intrusion as an alternative cause of the 18Oenrichment. Samples from 2 distinct lobes of the massif were analyzed: the NE lobe where xenoliths of metasedimentary country rock are common, and the NW lobe, where xenoliths are scarce and the country rock is dominantly granitic. The mean values of 18O for these two lobes are 9.6 in the NE and 9.3 in the NW. Thus, magmatic assimilation at the present level of exposure probably had only localized and relatively minor effects on the oxygen isotope composition of the massif. This conclusion is supported by Rb/Sr data: variations in Rb content and (87Sr/ 86Sr)i show that such crustal contamination is localized, generally occurring only in samples near the border zone. All of the available results suggest that the 18O-enrichment is a magmatic feature, acquired prior to intrusion at the present level of exposure. 相似文献
Associated syenitic rocks and carbonatites from Ihouhaouene, Algeria, have been investigated for their Sr and Nd isotope and trace element geochemistry. A zircon U-Pb emplacement age (1994 +22 -17 Ma) has been obtained from the carbonatites. The REE characteristics, among which the significant and approximately constant negative Eu anomaly and the evolution of (La/Ce)N and (Yb/Lu)N ratios which increase sympathetically with total REE abundances, are considered to be of purely magmatic origin. They are used to constrain the genetic links between syenites and carbonatites. Sr and Nd isotopes suggest a similar source for carbonatites and syenites, which is enriched compared to a chondritic reference: Nd(T)=-6.4 to -8.6 and ISr(T)=0.7097. These features are interpreted as evidence of contamination of a mantle-derived magmatic precursor by continental crust, occurring in a magmatic chamber. 相似文献
The main structures of a subduction zone are as follows.
1. (1) On the outer wall: faults, formed either by reactivation of the structural grain of the oceanic plate, when the latter is slightly oblique to the trench, or by a new fault network parallel to the trench, or both. The width of the faulted zone is about 50 miles.
2. (2) On the inner wall: either an accretionary prism or an extensional fault network, or both; collapsed structures and slumps are often associated, sometimes creating confusion with the accretionary structures.
3. (3) The overall structure of the trench itself is determined by the shape of the edge of the continental crust or of the island arc. Its detailed structure, however, is related to the oceanic plate, namely when the structural grain of the latter is slightly oblique to the trench, which then takes an “en echelon” form. Collapsed units can fill up the trench which is, in that case, restricted to an irregular narrow depression; the tectonic framework of the trench can be buried under a sedimentary blanket when the sedimentation rate is high and the trench bottom is a large, flat area.
Two extreme types of active margins can be distinguished: convergent compressive margins, when the accretionary mechanism is strongly active; and convergent extensional margins where the accretionary mechanism is absent or only weakly active.
The status of a given margin between these two extreme types is related to the convergence rate of the plates, the dip of the subduction zone, the sedimentation activity and the presence of a continental obstacle, because oceanic seamounts and aseismic ridges are easily subducted.
Examples are taken from the Barbados, Middle America, Peru, Kuril, Japan, Nankai, Marianna, Manila, New Hebredes and Tonga trenches. 相似文献
The carrier of the natural magnetization of deep sea sediments was characterized by mineralogical, electron microscopic, and rock magnetic investigations. Magnetic single domain (SD) and pseudo single domain (PSD) particles which are most important for the stable remanent magnetization were separated from the magnetic »coarse fraction« and concentrated as magnetic »fine fraction«. The magnetic coarse fraction consists of lithogenic magnetite and titanomagnetite, which often contains exsolution-lamellae of ilmenite. Both minerals are partially maghematized and occur isolated in the sediment or embedded in rock particles, in regionally different concentrations. The magnetic fine fraction consists of lithogenic magnetite and titanomagnetite and biogenic magnetite (magnetofossils = fossil bacterial magnetosomes), the latter generally maghematized.A graphical method is described which allows the classification and characterization of the magnetic fine fraction by demagnetization of the anhysteretic remanent magnetization (ARM) of whole sediment samples. Three groups with different magnetic properties can be distinguished, characterized by three ARM type-curves: Type A curves are associated with sediments from abyssal plaines. They show nearly identical ARM properties and are typical for magnetofossils.Type B curves are produced by sediments from the vicinity of volcanic regions. Their shapes are variable to a certain degree and indicate two lithogenic magnetic phases.Type C curves are found for sediments from submarine ridges and regions with input of terrigenous detritus. These curves have the largest deviations among each other indicating a magnetic multi-phase assemblage including magnetofossils.
Zusammenfassung Die Träger der Magnetisierung von Tiefseesedimenten wurden mineralogisch, elektronenmikroskopisch und gesteinsmagnetisch untersucht. Magnetische Eindomänen (SD) und Pseudo-Eindomänen (PSD) Partikel, die für eine stabile remanente Magnetisierung wichtig sind, wurden als magnetische »Feinfraktion« von der magnetischen »Grobfraktion« abgetrennt. Die magnetische Grobfraktion besteht aus lithogenem Titanomagnetit und Magnetit die teilweise maghemitisiert sind und teilweise auch Ilmenit-Entmischungslamellen aufweisen. In regional unterschiedlichen Konzentrationen liegen sie frei im Sediment oder in silikatischer Matrix eingebettet vor. Die magnetische Feinfraktion besteht sowohl aus lithogenem Titanomagnetit und Magnetit, als auch aus biogenem Magnetit (Magnetofossilien = fossile bakterielle Magnetosomen); letzterer ist größtenteils maghemitisiert.Es wird eine grafische Darstellungsmethode beschrieben, die anhand von Untersuchungen der anhysteretischen remanenten Magnetisierung (ARM) von Sedimentproben eine Charakterisierung der magnetischen Feinfraktion erlaubt. Es lassen sich dadurch drei Gruppen mit unterschiedlichen magnetischen Eigenschaften unterscheiden, die durch drei Gruppen von ARM-Kurventypen charakterisiert sind.Kurventyp A wird bei Sedimenten aus Tiefsee-Ebenen beobachtet. Die ARM-Daten sind nahezu identisch und zeigen ein Verhalten, wie es für Magnetofossilien typisch ist. Kurventyp B tritt bei Sedimenten aus dem Einzugsbereich vulkanischer Gebiete auf. Er zeigt eine größere Variation und die Form der Kurven spricht für ein System aus zwei lithogenen magnetischen Komponenten.Kurventyp C gehört zu Sedimenten aus submarinen Rücken und dem Einzugsgebiet terrigener Schüttungen. Die Kurvenverläufe sind uneinheitlich und sprechen für ein magnetisches Mehrkomponenten-System mit Beteiligung von Magnetofossilien.
Résumé Les minéraux porteurs du magnétisme dans les sédiments de mer profonde ont été explorés par les méthodes de la minéralogie, de la microscopie électronique et du magnétisme des roches. Les particules qui correspondent à un domaine magnétique unique (SD) et pseudo-unique (PSD), significatives pour un magnétisme rénanent stable, ont été concentrées comme «fraction magnétique fine» après séparation de la «fraction magnétique grossière». Cette dernière consiste en magnétite et titanomagnétite lithogéniques, qui renferment souvent des lamelles d'exsolution d'ilménite. Ces deux minéraux sont partiellement maghémitisés; ils se présentent isolés ou inclus dans des fragments de roches, avec des concentrations régionales diverses. La fraction magnétique fine consiste en magnétite et titanomagnétite lithogéniques, ainsi qu'en magnétite biogénique (magnétofossile = magnétosome fossile bactérien), cette dernière ordinairement maghemitisée.Les auteurs présentent une méthode graphique qui permet de caractériser la fraction magnétique fine à partir de l'examen du magnétisme rémanent anhystérique (ARM) de l'échantillon de sédiment. Cette méthode permet de distinguer trois groupes de propriétés magnétiques différentes, caractérisés par trois types de courbes ARM. Les courbes de type A caractérisent les sédiments de plaines abyssales; elles montrent des propriétés ARM presque identiques et sont typiques pour les magnétofossiles. Les courbes de types B sont fournies par les sédiments voisins des régions volcaniques; leurs formes varient dans une certaine mesure et indiquent un système à deux composants magnétiques lithogéniques. Les courbes de type C correspondent aux sédiments des crêtes sous-marines et des régions à apports terrigènes; ces courbes présentent entre elles des différences plus marquées, ce qui indique un système magnétique à composants multiples, comportant des magnétofossiles.
In this paper, the well-established multi-layer model originally devised by Waggoner and Reifsnyder (1968) is used. This steady-state model based on an electrical analogue simulates the energy exchange between the vegetation and the atmosphere. A purely mathematical development of the basic equations of this model yields explicit expressions of the total fluxes of sensible and latent heat at the top of the canopy as a function of the net radiation absorbed in each layer, the soil heat flux, the water vapour pressure deficit at a reference height and the whole set of elementary conductances (stomatal, boundary-layer and aerodynamic). These new equations can be considered as a generalization of the familiar Penman's formulae to a multi-layer model. 相似文献