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91.
Agnieszka Gil Gennady A. Kovaltsov Vladimir V. Mikhailov Alexander Mishev Stepan Poluianov Ilya G. Usoskin 《Solar physics》2018,293(11):154
A usual event, called anisotropic cosmic-ray enhancement (ACRE), was observed as a small increase (\({\leq}\,5\%\)) in the count rates of polar neutron monitors during 12?–?19 UT on 07 June 2015. The enhancement was highly anisotropic, as detected only by neutron monitors with asymptotic directions in the southwest quadrant in geocentric solar ecliptic (GSE) coordinates. The estimated rigidity of the corresponding particles is \({\leq}\,1\) GV. No associated detectable increase was found in the space-borne data from the Geostationary Operational Environmental Satellite (GOES), the Energetic and Relativistic Nuclei and Electron (ERNE) on board the Solar and Heliospheric Observatory (SOHO), or the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) instruments, whose sensitivity was not sufficient to detect the event. No solar energetic particles were present during that time interval. The heliospheric conditions were slightly disturbed, so that the interplanetary magnetic field strength gradually increased during the event, followed by an increase of the solar wind speed after the event. It is proposed that the event was related to a crossing of the boundary layer between two regions with different heliospheric parameters, with a strong gradient of low-rigidity (\({<}\,1\) GV) particles. It was apparently similar to another cosmic-ray enhancement (e.g., on 22 June 2015) that is thought to have been caused by the local anisotropy of Forbush decreases, with the difference that in our case, the interplanetary disturbance was not observed at Earth, but passed by southward for this event. 相似文献
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Renaud E. Merle Alexander A. Nemchin Martin J. Whitehouse Robert T. Pidgeon Marion L. Grange Joshua F. Snape Fiona Thiessen 《Meteoritics & planetary science》2017,52(5):842-858
In this paper, we compare the U‐Pb zircon age distribution pattern of sample 14311 from the Apollo 14 landing site with those from other breccias collected at the same landing site. Zircons in breccia 14311 show major age peaks at 4340 and 4240 Ma and small peaks at 4110, 4030, and 3960 Ma. The zircon age patterns of breccia 14311 and other Apollo 14 breccias are statistically different suggesting a separate provenance and transportation history for these breccias. This interpretation is supported by different U‐Pb Ca‐phosphate and exposure ages for breccia 14311 (Ca‐phosphate age: 3938 ± 4 Ma, exposure age: ~550–660 Ma) from the other Apollo 14 breccias (Ca‐phosphate age: 3927 ± 2 Ma, compatible with the Imbrium impact, exposure age: ~25–30 Ma). Based on these observations, we consider two hypotheses for the origin and transportation history of sample 14311. (1) Breccia 14311 was formed in the Procellarum KREEP terrane by a 3938 Ma‐old impact and deposited near the future site of the Imbrium basin. The breccia was integrated into the Fra Mauro Formation during the deposition of the Imbrium impact ejecta at 3927 Ma. The zircons were annealed by mare basalt flooding at 3400 Ma at Apollo 14 landing site. Eventually, at approximately 660 Ma, a small and local impact event excavated this sample and it has been at the surface of the Moon since this time. (2) Breccia 14311 was formed by a 3938 Ma‐old impact. The location of the sample is not known at that time but at 3400 Ma, it was located nearby or buried by hot basaltic flows. It was transported from where it was deposited to the Apollo 14 landing site by an impact at approximately 660 Ma, possibly related to the formation of the Copernicus crater and has remained at the surface of the Moon since this event. This latter hypothesis is the simplest scenario for the formation and transportation history of the 14311 breccia. 相似文献
94.
Wangcheng Zhang Dong Wang Mark F. Randolph Alexander M. Puzrin 《国际地质力学数值与分析法杂志》2016,40(17):2312-2338
Quantitative assessment of the risk of submarine landslides is an essential part of the design process for offshore oil and gas developments in deep water, beyond the continental shelf. Landslides may be triggered by a reduction in shear strength of subsea sediments over a given zone, caused for example by seismic activity. Simple criteria are then needed to identify critical conditions whereby the zone of weakness could grow catastrophically to cause a landslide. A number of such criteria have been developed over the last decade, based either on ideas drawn from fracture mechanics, or considering the equilibrium of the initial weakened zone and adjacent process zones of gradually softening material. Accounting for the history of the weak zone initiation is critical for derivation of reliable propagation criteria, in particular considering dynamic effects arising from accumulating kinetic energy of the failing material, which will allow the failure to propagate from a smaller initial zone of weakened sediments. Criteria are developed here for planar conditions, taking full account of such dynamic effects, which are shown to be capable of reducing the critical length of the softened zone by 20% or more compared with criteria based on static conditions. A numerical approach is used to solve the governing dynamic equations for the sliding material, the results from which justify assumptions that allow analytical criteria to be developed for the case where the initial softening occurs instantaneously. The effect of more gradual softening is also explored. Copyright © 2016 John Wiley & Sons, Ltd. 相似文献
95.
Terra Nova, 22, 390–395, 2010 Abstract We present the results of coupled analogue and numerical models that provide new insights into the relationships between volcanoes and thrusts. The effects of both upper‐crustal magma chambers and the load of volcanoes on the geometry of thrust systems were investigated. Analogue modelling points to a strong influence exerted by a magma chamber on thrust geometry, which, as suggested by the numerical models used to rationalize these results, is related to the stress redistribution around the weak heterogeneity. The low‐viscosity body below a volcanic edifice localizes compressional deformation and causes a curvature of the thrusts towards the magma chamber, opposite to the direction of tectonic transport. In these conditions, the volcanic load has a negligible effect on the structural geometry. These results are in contrast with those of previous studies, where intrusions or the load of major volcanoes generated a curvature of the thrusts away from volcanic edifices in the direction of tectonic transport. 相似文献
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Hydrophobic and electrostatic parameters in bacterial adhesion 总被引:5,自引:0,他引:5
Mark C. M. van Loosdrecht Willem Norde Johannes Lyklema Alexander J. B. Zehnder 《Aquatic Sciences - Research Across Boundaries》1990,52(1):103-114
Recently it has been shown that the initial stages of bacterial adhesion to a model-surface of sulphated polystyrene can best be described using hydrophobic and electrostatic parameters. In the present study it is tested whether these parameters can generally be applied to predict bacterial adhesion by using (i) glass, as a model for hydrophilic and natural surfaces of silicates and oxides, (ii) polystyrene coated with proteins, as a model for a surface coated with an organic layer, and (iii) river Rhine sediment, as an example of a natural surface. Adhesion to glass was dominated by electrostatic interaction, whereas adhesion to polystyrene coated with various types of proteins depended on the surface characteristics of the bacteria and the type of protein. By relating Van der Waals interactions to hydrophobicity of the interacting species, the adhesion of bacteria to the various surfaces including the river Rhine sediments could be interpreted in terms of the DLVO-theory. It is therefore concluded that the conceptual principles of the DLVO-theory (interplay of Van der Waals and electrostatic interactions) are suitable to describe, at least qualitatively, the initial processes of bacterial adhesion to a wide range of surfaces. 相似文献
100.
Doz. Dr. Edith Kristan-Tollmann Prof. Dr. Alexander Tollmann 《International Journal of Earth Sciences》1982,71(3):987-1019
Zusammenfassung Es wird zunächst ein kurzer Überblick über die stratigraphische und fazielle Entwicklung der Trias im Gesamtraum der Tethys zwischen Betischer Kordillere in Spanien und Timor gegeben. Hierbei zeigt sich, daß im Westabschnitt, besonders im mediterranen Raum, eine mio- und aristogeosynklinale und nur untergeordnet eugeosynklinale Entwicklung der Trias vorliegt, in Ostasien (Himalaya, China) auch eugeosynklinal entwickelte Trias vermehrt auftritt. Die europäische Entwicklung der Tethystrias ist durch ihre vielfältige Individualisierung von der asiatischen Trias, die in ihrem Oberteil weiträumig durch eine detritische Fazies beherrscht ist, unterschieden, was besonders auf den Einfluß der indosinischen Faltung in Ostasien zurückgeht. Nord- und Südast der Tethys aber deshalb und auf Grund eines verschiedenartigen Erbes als Paläo- und Neotethys zu bezeichnen, geht zu weit, da die Einheit der gesamten Tethys hierdurch begrifflich zerrissen werden würde.Besonders hervorzuheben ist die Tatsache, daß zahlreiche typische Triasschichtglieder in verschiedenen Abschnitten des Gesamtraumes der Tethys auftreten, nach Litho- und Biofazies und Altersstellung eindeutig als gleichartig identifiziert werden können und demnach im gesamten Raum mit gleichen Namen belegt werden sollen. Das gilt besonders für Reichenhaller Rauhwacke, Gutensteiner Kalk, Reiflinger Kalk, Wettersteinkalk, Hallstätter Kalk, Dachsteinkalk, Kössener Schichten, Rhätoliaskalk — um nur einige Glieder zu nennen, die vom gesamten Raum vom mediterranen Gebiet bis über China hinaus, und zwar z. T. bis Timor — und im Falle des Hallstätter Kalkes bis Südamerika -, verfolgt werden können. Die Ursache liegt im gleichen Schicksal der Kontinentrandgebiete, teils durch Eustatik, teils durch die Mobilität des Schelfs, teils durch die gleichartigen Gesteinsbildner in Fauna und Flora bewirkt.Die Gemeinsamkeit von entscheidenden Faunenelementen über den gesamten Raum der Tethys hin ist ein nächstes, besonders ins Auge stechendes Merkmal. Sie bezieht sich nicht nur auf planktonische und pelagische Elemente, sondern auch auf vagil-benthonische, ja sessile Organismen und umfaßt überraschend viele Arten der Makro- und Mikrofauna, darunter viele Leitfossilien. Zahlreiche Formen sind bisher unter verschiedenen Lokalnamen beschrieben worden, deren Nachuntersuchung nun die Gleichartigkeit über den gesamten Raum der Tethys bestätigt hat. Natürlich bezieht sich diese Feststellung nur auf einen Teil der Fauna, daneben erscheinen auch an Faunenprovinzen gebundene Elemente.Schließlich werden Überlegungen über die Herkunft der Tethysfauna angestellt. Als Heimat eines wesentlichen überregional verbreiteten Anteils wird der ostpazifische Raum am amerikanischen Kontinentalrand, besonders der Raum von Britisch-Kolumbien abgeleitet. Als Gründe sprechen dafür: 1. Reichliche Beteiligung von Tethyselementen an der Fauna dieser ostpazifischen Provinz, 2. Fehlen eines Meeresweges quer durch (Mittel-) Amerika nach Osten zur Tethys in der Zeit der Trias, 3. Rekonstruktion eines Paläowind- und Meeresströmungssystems auf Grund der Triaspaläogeographie und aktualistischer Prinzipien, das eine Drift von Osten nach Westen durch Pazifik und Tethys bewirkt haben muß, 4. Die Möglichkeit dieser Wanderung von Faunenelementen über den Pazifik auch für vagiles und sessiles Benthos mit Hilfe von Larvenstadien und in pseudoplanktonischer Form auf Tang und Treibholz. Abgesehen von diesem über den gesamten tropischen bis tropennahen Raum von Pazifik und Tethys verbreiteten Anteil kommt naturgemäß noch ein autochthoner Anteil der Fauna hinzu, der sich in den einzelnen Faunenprovinzen jeweils autonom entwickelt hat — besonders begünstigt im asiatischen Teil der Tethys. Schließlich liegt nach der Verbreitung bestimmter Arten und Artgruppen noch die Möglichkeit der Wanderung eurasiatischer Formen in höheren Breiten mit den ostgerichteten Gegenströmungen von Tethys und Pazifik nahe.
Arbeit im Rahmen des Int. Geol. Correl. Programme, Projekt 73/I/4, Triassic of the Tethys Realm, durchgeführt. 相似文献
The development of the Triassic within the Tethys realm and the origin of its fauna
Summary This paper gives at first a survey about the stratigraphy and facies of the Triassic within the Tethys realm between Betic Cordillera in Spain and Timor in Indonesia. This review shows that the western part of the Tethys in the Mediterranean region comprises a mio-, (eu-)and aristogeosynclinal facies of the Triassic and prooves that the eugeosynclinal facies is more significant for the central- and eastasiatic part of the Tethys realm.The European development is characterized by an extreme individualisation of faciestypes and a hight specification of Triassic formations, whilst the Asiatic region is dominated by an extensive spreading of immense masses of detritus in the Upper Triassic — particularly in the northern branch of Tethys -, in dependence on the Indosinic orogenesis at the end of the Middle Triassic. The distinction of a northern Paleotethys and a southern Neotethys during the Mesozoic era with regard to this event can't be sanctioned, respecting the integrity of the Tethys as a whole.The following chapter stresses the fact that many alpine formations are spreaded whole over the Tethys realm, identic in lithofacies, biofacies, fauna, flora and stratigraphic position, so that one must not hesitate denominating the same formations with the same name (Lugeon/Andrusov-principle). Those formations and members, identical all over the Tethys region, are e. g. Reichenhaller cellular dolomite, Gutenstein Wurstel-limestone, Reifling-, Wetterstein-, Hallstatt- and Dachstein-limestone, which can be observed from the Mediterranean region up to China and Timor — the Hallstatt limestone as fare as Southern America. The reason of this surprisingly fact is caused by the same conditions of the plate margins during the Triassic tectonic history, moreover by the same conditions for the formation of organogeneous limestone by time-specific organismes and in some cases also in eustatic movements of the sea level.The next fact shown in this paper is the result that a lot of characteristic alpin fauna elements are spreaded all over the Tethys area, from the Alps to Indonesia. This statement concerns not only planctonic and pseudoplanctonic taxa, but also many bentonic elements living in a vagil or sessil manner within the macro- and microfauna — comprisingly also many index-fossils. Hitherto a lot of those species have been described under local names. The revision of the fossil material, collected directly by the authors in many sectors of the Tethys has confirmed this result of widespread species whole over the Tethys ocean.Finally some reflections are made about the origin of the Tethys fauna. A part of the Tethys fauna which is common with the fauna of the Eastern Pacific region, is regarded as originally developed in Western America, particularly in the territory of British Columbia, and transported by the Pacific ocean currents westwards into the Tethys. A short connection between Eastern Pacific and Western Tethys by a Protoatlantic (Poseidon) did not existe in consequence of the existence of Pangea during the Triassic time. Therefore the communication of the identic faunistic elements of Eastern Pacific and Tethys must have be realized by transpacific way: New observations about the longevity of larval stages, also of recent benthic organisms and reflections about the Triassic paleocurrent system in the Panthalassa established on actualistic principles (Fig. 2) proove the feasibility of such a theory. By the counter-current in high latitudes the transport of Tethyal elements to eastern areas along the shore of America could be effected.
Résumé Cet article donne premièrement un résumé de la stratigraphie et du faciès du Trias de la région mesogéenne entre la Cordillère Bétique et Timor en Indonésie. Il apparaît ainsi qu'on trouve dans les régions méditerranéennes notamment un faciès mio- et aristogéosynclinal, tandis que le faciès eugéosynclinal est plus fréquent dans la partie centrale et orientale de la Téthys asiatique.La partie européenne de la Téthys est caractérisée par une individualisation extrême des types de faciès et des formations. Au contraire, le faciès de la région asiatique est dominé par des masses détritiques dans le Trias supérieur, comme conséquence de la phase orogénique indosinienne dans l'Asie orientale.Par la suite on démontre que bien des formations alpines sont répandues dans toute la région de la Téthys, identiques en lithofaciès, biofaciès, faunes, flores et dans leur position stratigraphique — en conséquence, il ne faut pas hésiter d'employer les mêmes désignations pour les mêmes formations dans tout le territoire en question. On retrouve par exemple les cargnieules de Reichenhall, les calcaires vermiculés de Gutenstein, les calcaires de Reifling, du Wetterstein, de Hallstatt et du Dachstein etc. à partir de la région méditerranéenne jusqu' en Chine et à Timor; d'autre part, les calcaires de Hallstatt se retrouvent jusqu' en Amérique méridionale. Ce fait étonnant tient à des conditions identiques valables pour les bords des plaques continentales pendant le Triassique, ainsi qu'à une formation identique des calcaires organogènes provoquée par l'existence simultanée des mêmes organismes et aussi par des oscillations eustatiques de l'océan.Un autre résultat que nous aimerions mentionner dans cet article est le fait qu' un nombre assez grand des éléments de la faune alpine est répandu dans tout le territoire de la Téthys. Cette constatation ne concerne pas seulement les éléments (pseudo-)planctoniques, mais aussi beaucoup d'organismes bentoniques (vagiles et sessiles) de la macroet microfaune. Jusqu' à présent, beaucoup de ces espèces sont décrites sous des noms locaux. La révision des suites des fossiles, collectionnées par les auteurs eux-mêmes dans les différents secteurs de la Téthys, a confirmé ce fait.Enfin des réflexions sont faites sur l'origine de la faune téthysienne. Une partie de cette faune de la Téthys, celle qui correspond à la faune de la région pacifique orientale, se serait développée d'abord en Amérique septentrionale, notamment en Colombie britannique, et aurait été transportée par le courant pacifique central vers l'ouest, dans la Téthys. Une communication directe, pendant le Trias, entre le Pacifique et la Téthys occidentale, par un Protoatlantique («Poseidon») n'existait pas du fait que la Pangéa était intacte. La migration des éléments faunistiques dans le Pacifique oriental et dans la Téthys n'était possible que le long de la route transpacifique. Des observations nouvelles sur la longue durée des stades larvales des organismes bentoniques ainsi que des réflexions concernant les paléocourants de la Panthalassa (Fig. 2) prouvent le bien-fondé de cette théorie. Par des contre-courants dans des latitudes supérieures, le transport des éléments faunistiques de la Téthys dans des régions arctiques et antarctiques de l'Amérique était possible.
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Arbeit im Rahmen des Int. Geol. Correl. Programme, Projekt 73/I/4, Triassic of the Tethys Realm, durchgeführt. 相似文献