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1.
Sediment archives from a mountain lake are used as indicators of seismotectonic activity in the Grenoble area (French western Alps, 45°N). Sedimentological analysis (texture and grain-size characteristics) exhibits several layers resulting from instantaneous deposits in Lake Laffrey: six debris flow events up to 8 cm thick can be attributed to slope failure along the western flank of the basin. Dating with 210Pb and 137Cs gamma counting techniques and the reconnaissance of historical events, provide a constrained age-depth model. Over the last 250 years, five of such debris flow deposits could be related to historical earthquakes of MSK intensities greater than VI over an area of <60 km. One debris flow deposit triggered at the beginning of the last century can be related to an historical landslide possibly triggered by the artificial regulation of the lake level.  相似文献   
2.
The 1990 edition of the National Building Code of Canada (Associate Committee of the National Building Code, National Research Council, Ottawa, 1990) makes a clear distinction between eastern and western Canada in terms of seismic acceleration and velocity zones. While it is well established that ground motions can be amplified significantly through loose clay deposits, no results are available that take into consideration the typical high frequency content of ground motions in eastern Canada. This paper develops ground amplification curves for clays having depths between 10 and 70 m excited by typical eastern Canadian ground motions scaled to two different values of peak horizontal accelerations. Simplified free-field spectral design curves, which could be used by structural designers, are proposed. The curves show that maximum spectral accelerations occur for structural periods between 0.2 and 0.5 s. In addition, soil depth does not appear to be an important parameter controlling the response of typical clay deposits in eastern Canada.  相似文献   
3.
Mine development along a 15-mile (24 km) section of the Warfield Fault in Mingo County, West Virginia has broadened the geological understanding of the fault and its related structures. The fault has been exposed in two new road cuts, one in the northeast-trending segment at Neely Branch and one in the eastern east-trending segment at the head of Marrowbone Creek. Both exposures show a well-defined normal fault with a 45° to 55° N dip, juxtaposing sandstone/shale packages from the roof and the floor of the Coalburg seam. The fault is associated with a thin gouge zone, some drag folding, and parallel jointing. Its trace tends to run parallel to the crest of the adjacent Warfield Anticline. Based on underground mine development and detailed core drilling, the vertical offset along the fault plane ranges from a maximum of 240 ft (73 m) in the central part of the area near the structural bend to less than 100 ft (30 m) in western and eastern directions. The fault is located along the relatively steeply dipping (locally in excess of 25%) southern limb of the Warfield Anticline, and appears related to a late phase of extension involving folded Pennsylvanian strata. On a regional scale, the lithological variations across the fault do not suggest any appreciable strike-slip component.Underground room and pillar mines in the Coalburg seam north and south of the fault have been greatly impacted by the Warfield structures. Due to the combined (and opposite) effects of the folding and faulting, the northern mines are located up to 400 ft (125 m) higher in elevation than the southern ones. Overland conveyor belts connect mining blocks separated by the fault. The practical mining limit along the steep slopes toward the fault is around 15%. Subsidiary normal faults with offsets in the 5- to 15-ft (1.5–4.5 m) range are fairly common and form major roof control and production hurdles. Overall, the Warfield structures pose an extra challenge to mine development in this part of the Appalachian Coalfields.  相似文献   
4.
Segregation of incompatible elements at grain interfaces may have considerable influence on the physical and chemical properties of mantle rocks. Using a recently developed predictive model to estimate the interface enrichment of elements based on their mineral/melt partitioning (Hiraga and Kohlstedt, companion paper), we consider interface enrichment for a simplified model peridotite consisting of olivine, orthopyroxene, and clinopyroxene. Our calculated results reveal the following: (1) Significant amounts of heavy alkali elements and rare gases likely reside at grain-grain interfaces, whereas interface concentrations of less incompatible are less pronounced. (2) The contribution of the chemical components stored at interfaces to whole-rock chemistry strongly depends on mineral mode and, most importantly, on grain size. (3) Grain size reduction resulting from dynamic recrystallization can increase the total storage of highly incompatible elements on grain interfaces and thereby will diminish their concentration in mineral grains. (4) Analysis of Cs concentrations in mantle clinopyroxenes potentially provides estimates of the grain size of mantle rocks. (5) Transport through peridotite will be dominated by diffusion along interfaces rather than through grain interiors for elements less compatible than Lu.  相似文献   
5.
Natural Hazards - This paper studies different machine learning methods for solving the regression problem of estimating the marine surge value given meteorological data. The marine surge is...  相似文献   
6.
Oued Awlitis 001 is a highly feldspathic, moderately equilibrated, clast‐rich, poikilitic impact melt rock lunar meteorite that was recovered in 2014. Its poikilitic texture formed due to moderately slow cooling, which judging from textures of rocks in melt sheets of terrestrial impact structures, is observed in impact melt volumes at least 100 m thick. Such coherent impact melt volumes occur in lunar craters larger than ~50 km in diameter. The composition of Oued Awlitis 001 points toward a crustal origin distant from incompatible‐element‐rich regions. Comparison of the bulk composition of Oued Awlitis 001 with Lunar Prospector 5° γ‐ray spectrometer data indicates a limited region of matches on the lunar farside. After its initial formation in an impact crater larger than ~50 km in diameter, Oued Awlitis 001 was excavated from a depth greater than ~50 m. The cosmogenic nuclide inventory of Oued Awlitis 001 records ejection from the Moon 0.3 Ma ago from a depth of at least 4 m and little mass loss due to ablation during its passage through Earth's atmosphere. The terrestrial residence time must have been very short, probably less than a few hundred years; its exact determination was precluded by a high concentration of solar cosmic ray‐produced 14C. If the impact that excavated Oued Awlitis 001 also launched it, this event likely produced an impact crater >10 km in diameter. Using petrologic constraints and Lunar Reconnaissance Orbiter Camera and Diviner data, we test Giordano Bruno and Pierazzo as possible launch craters for Oued Awlitis 001.  相似文献   
7.
Pseudodiaptomus hessei is a key species in many water bodies in the Senegal River hydrosystem but it became rare or completely disappeared from two ecosystems (Lake Guiers and Dakar Bango Reservoir; Senegal, West Africa) after major hydrological changes caused by human action, mainly impoundments on the river in 1985, and the opening of a new estuary mouth in 2003. Kâ et al. [Kâ, S., Pagano, M., Ba, N., Bouvy, M., Leboulanger, C., Arfi, R., Thiaw, O.T., Ndour, E.H.M., Corbin, D., Defaye, D., Cuoc, C., Kouassi, E., 2006. Zooplankton distribution related to environmental factors and phytoplankton in a shallow tropical lake (Lake Guiers, Senegal, West Africa). International Review of Hydrobiology 91(5), 389–405] put forward several hypotheses to explain the reasons for this decline: salinity and chemical changes in the water, predation by a cyclopid predator Mesocyclops ogunnus and/or the inhibiting effects of cyanobacteria and/or diatoms (allelopathy). This study assessed these hypotheses by studying the distribution of P. hessei in 13 stations (including the Dakar Bango reservoir and Lake Guiers) in relation to physical, chemical and biological (phyto- and zooplanktons) factors at each station. We produced a distribution pattern for this species in the Senegal River hydrosystem. Rank correlations and principal component analysis showed that P. hessei was not correlated with conductivity but was positively correlated with pH and alkalinity, suggesting chemical effects. The clear association with two filamentous cyanobacteria (Cylindrospermopsis raciborskii and Anabaena sp.) did not appear to support the hypothesis of cyanobacteria inhibition but blooming conditions were never encountered during the study. Negative correlation with diatoms (especially with Fragilaria sp.) suggested that aldehyde producing diatoms had a negative effect. Negative correlations with cyclopids such as Mesocyclops supported the hypothesis of cyclopid predation to explain the decline of P. hessei. This study proposes several lines of research for future studies to test these hypotheses.  相似文献   
8.
We use a secular model to describe the non-resonant dynamics of trans-Neptunian objects in the presence of an external ten-Earth-mass perturber. The secular dynamics is analogous to an “eccentric Kozai mechanism” but with both an inner component (the four giant planets) and an outer one (the eccentric distant perturber). By the means of Poincaré sections, the cases of a non-inclined or inclined outer planet are successively studied, making the connection with previous works. In the inclined case, the problem is reduced to two degrees of freedom by assuming a non-precessing argument of perihelion for the perturbing body. The size of the perturbation is typically ruled by the semi-major axis of the small body: we show that the classic integrable picture is still valid below about 70 AU, but it is progressively destroyed when we get closer to the external perturber. In particular, for \(a>150\) AU, large-amplitude orbital flips become possible, and for \(a>200\) AU, the Kozai libration islands at \(\omega =\pi /2\) and \(3\pi /2\) are totally submerged by the chaotic sea. Numerous resonance relations are highlighted. The most large and persistent ones are associated with apsidal alignments or anti-alignments with the orbit of the distant perturber.  相似文献   
9.
Résumé L'activité magmatique ophiolitique du géosynclinal alpin (diabases, gabbros, serpentines, etc.) a été suivie par une activité à caractère volcanique moins bien connue. En effet, les appareils correspondant à cette activité ont complètement disparu; nous devons nous contenter pour tous renseignements de l'étude des fragments de roches contenus dans des grauwackes tertiaires appartenant au Flysch (grès de Taveyanne, grès d'AItdorf pro parte, grès du Champsaur).La détermination de la nature originelle des laves est, en outre, rendue difficile par le fait, découvert récemment, que ces grauwackes ont subi un métamorphisme régional les plaçant dans le faciès à zéolites; on peut raisonnablement admettre qu'il s'agissait d'andésites basaltiques.L'áge des épanchements est encore indéterminé, il doit être compris entre le Crétacé supérieur et la fin de l'Eocène. L'hypothèse la plus plausible consiste à admettre que les volcans, aujourd'hui complètement érodés se trouvaient dans la partie la plus interne du domaine pennique. Toutefois au moment du dépôt des grès de Taveyanne, les coulées ne se trouvaient plus dans leur position initiale, elles avaient glissé vers l'avant-pays sous forme d'une nappe.Il est très probable que cette activité volcanique post-ophiolitique n'est pas restreinte au segment franco-suisse des Alpes occidentales mais que des formations analogues aux grès de Taveyanne se retrouvent ailleurs, notamment en Sicile et dans les Apennins.
The magmatic activity which gave birth to the ophiolites (diabases, gabbros, serpentinites) of the alpine geosyncline was followed by subaerial volcanism. This volcanic activity is not well known as the volcanoes were completely destroyed by erosion. Our only source of information is to be found in fragments of volcanic rocks which are part of Tertiary Flysch graywackes (Taveyanne sandstones, part of the Altorf sandstones, Champsaur sandstones).The determination of the initial composition of the lavas is further complicated by metasomatic transformations; it has been recently shown that the Taveyanne graywackes were submitted to a light regional metamorphism corresponding to the zeolitic facies ofCoombs. However, it seems that these lavas were originally basaltic andesites.The age of this volcanism is not precisely known, it cannot be later than Upper Eocene as the time of deposition of the Taveyanne sandstones is Uppermost Eocene-Lower Oligocene; it is probably post-Cenomanian. It is likely that the volcanoes were located in the southern part of the Penninic zone; however at the time of deposition of the graywackes the volcanic flows had already left their initial location, gliding toward the Foreland as part of a Nappe.Very probably, remnants of this post-ophiolitic volcanism are not restricted to the French-Swiss segment of the Western Alps, but will be found elsewhere, particularly in the Apennine Mountains and in Sicily.

Zusammenfassung Die magmatische Tätigkeit, die Ophiolithe (Diabase, Gabbros, Serpentinite) der alpinen Geosynklinale entstehen ließ, wurde von subärischem Vulkanismus abgelöst. Diese Vulkantätigkeit ist wenig bekannt, da die Vulkane durch Erosion völlig zerstört wurden. Unsere einzige Informationsquelle findet sich in vulkanischen Gesteinsfragmenten, die Bestandteile der Tertiär-Flysch-Grauwacken sind.Die Bestimmung der ursprünglichen Zusammensetzung der Laven wird weiter durch metasomatische Umwandlungen erschwert. Kürzlich wurde gezeigt, daß die Taveyanne-Grauwacken einem regionalen Metamorphismus ausgesetzt waren, welcher der zeolithischen Fazies von Coombs entspricht. Es scheint jedoch, daß diese Laven ursprünglich basaltische Andésite waren.Das Alter dieses Vulkanismus ist nicht genau bekannt; es kann aber nicht später sein als das Obere Eozän, da die Ablagerungszeit der Taveyanne-Sandsteine Oberstes Eozän—Unteres Oligozän ist. Wahrscheinlich lagen die Vulkane im südlichen Teil der penninischen Zone; zur Zeit der Ablagerung der Grauwacken waren die Vulkanite bereits in die Überschiebungsmassen mit einbezogen.Sehr wahrscheinlich sind die Überreste dieses nach-ophiolithischen Vulkanismus nicht auf den französisch-schweizerischen Abschnitt der Westalpen beschränkt, sondern werden sich auch andernorts speziell auf dem Apennin und in Sizilien finden lassen.

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10.
The natural thermal evolution of type III coals (Humic origin) is expressed during diagenesis by a loss of oxygen as CO2 and H2O. Other phenomena such as oxidation can cause extensive geochemical modifications and may complicate the effects of simple maturation.Humic coals from the Jurassic in southeastern Utah were studied by elemental analysis, Rock-Eval pyrolysis and infrared spectroscopy. In a van Krevelen diagram (atomic H/C vs atomic O/C), the samples fall within the envelope defined by 860 reference humic coals covering the entire range of diagenesis. Nevertheless, various criteria (geochemical, petrographic, geological and microscopic) cast doubt upon the interpretation that such a distribution of coal composition results from thermal maturation.The same criteria indicate the intervention of redox phenomena. Comparison of our results with those from artificial and natural oxidation shows that these coals were subjected to an oxidation process different from ordinary late alteration. This process was probably due to circulation of highly oxidizing saline water causing oxygen fixation and the transformation of carboxyls into carboxylate anions. The cations that were fixed are oxygenated and certainly contain calcium, but also uranium and perhaps several other cations (V, Mo, Fe...). Emphasis is placed on possible mechanisms that cause such phenomena.  相似文献   
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