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Snow avalanches are a major natural hazard for road users and infrastructure in northern Gaspésie. Over the past 11 years, the occurrence of nearly 500 snow avalanches on the two major roads servicing the area was reported. No management program is currently operational. In this study, we analyze the weather patterns promoting snow avalanche initiation and use logistic regression (LR) to calculate the probability of avalanche occurrence on a daily basis. We then test the best LR models over the 2012–2013 season in an operational forecasting perspective: Each day, the probability of occurrence (0–100%) determined by the model was classified into five classes avalanche danger scale. Our results show that avalanche occurrence along the coast is best predicted by 2 days of accrued snowfall [in water equivalent (WE)], daily rainfall, and wind speed. In the valley, the most significant predictive variables are 3 days of accrued snowfall (WE), daily rainfall, and the preceding 2 days of thermal amplitude. The large scree slopes located along the coast and exposed to strong winds tend to be more reactive to direct snow accumulation than the inner-valley slopes. Therefore, the probability of avalanche occurrence increases rapidly during a snowfall. The slopes located in the valley are less responsive to snow loading. The LR models developed prove to be an efficient tool to forecast days with high levels of snow avalanche activity. Finally, we discuss how road maintenance managers can use this forecasting tool to improve decision making and risk rendering on a daily basis.  相似文献   

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Ocean plate stratigraphy (OPS) is essential to understanding accretionary wedges and complexes along convergent plate margins. Mélanges within accretionary wedges and complexes are the products of fragmentation and mixing processes during and following OPS accretion. A new term, ‘OPS mélange’, is proposed here for mélanges composed mostly of blocks of OPS with an argillaceous matrix, and for a mixture of mélanges of multiple origins with either broken or coherent formations. An OPS mélange results from the fragmentation and disruption of OPS, without admixing of other components. Three major types of OPS mélange can be distinguished on the basis of their components: turbidite type, chert–turbidite type, and limestone–basalt type. These three types potentially form similar mélanges, but they are derived from different parts of the OPS, depending on the level of the decollement surface. The concept of ‘OPS mélange’ can be applied to most of the mélanges in accretionary prisms and complexes worldwide. In addition, this proposal recognizes a distinction between processes of fragmentation and mixing of OPS components, and mixing of ophiolite components, the latter of which results in serpentinite mélanges, not OPS mélanges. Mélanges composed of OPS sequences occur worldwide. The recognition of OPS mélanges is a key aspect of understanding tectonic processes at convergent margins, which result in mélange formation in orogenic belts globally.  相似文献   

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ABSTRACT

The Franciscan Complex comprises the largely sedimentary basement of the California Coast Ranges. This classic trench deposit has undergone a series of superimposed tectonic events since the end of Jurassic time, involving accretion, high-pressure (HP) recrystallization, buoyancy and wedge-driven exhumation, and transcurrent slip. Processes reflect plate convergence, transpressive-orthogonal subduction, and transpressive–transtensive offset. Besides stratigraphically intact strata, the Franciscan displays widespread mélanges of four main types: diapiric serpentinite intrusions, sedimentary olistostromes, broken formations, and tectonic block-in-matrix units. In the northern Coast Ranges, mélanges are especially prevalent in the Central Belt, but also occur in the Eastern and Coastal belts. Diapirs show upward, buoyant flow relative to wall rocks, but some also appear to have involved wedge-driven thrusting. Many serpentinite diapirs and tectonic mélanges contain exotic metamafic inclusions rimmed by actinolite–chlorite reaction rinds. Olistostromes include gravity slump blocks and conglomeratic lenses; petrologically similar to larger slide blocks, pebble layers document a surficial, sedimentary origin, as does the presence of volcanic arc clasts. Broken formations grade by degrees from intact stratal continuity to disrupted units; they only contain cognate boudins of rocks present in the ductile matrix. Some tectonic mélanges are simply intensely disaggregated broken formations, and include rock types of the stratigraphic host. Other tectonic mélanges carry exotic HP blocks of diverse lithologies, generally reflecting higher pressures than attended recrystallization of the low-density matrix. The four mélange types formed through diverse convergent plate-tectonic processes. Many were subjected to a multi-stage overprint; most are strongly deformed, obscuring original textures and structures. Broken formations are the most common disrupted units, accompanied by lesser amounts of tectonic mélanges, olistostromes, and ductile-matrix diapirs. In aggregate, these units reflect the operation of contrasting processes that attest to plate-tectonic evolution of the Franciscan Complex. Strong deformation accompanied oceanic plate underflow, but also took place during coeval HP metamorphism and surfaceward return of accretionary packets, then transitioned to long-sustained, chiefly dextral slip.  相似文献   

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Iron-titanium rich grains (‘ilmenites’ to a various degree of weathering) occuring along the coast line of Senegal and deriving from various parent units are characterized from their size, texture, magnetic and geochemical properties. Both the corresponding data and their multivariate analysis lead to the conclusion that the ‘ilmenite’ grains derive from various sources, mainly local ones, except in the area of Saint-Louis where occur more distal grains from Mauritania. In the North of Cap Vert and in the South of Gambia, the ‘Continental Terminal’ formation represents the main source of the ‘ilmenite’ grains. Along the ‘Petite Côte’, ‘ilmenites’ derive mainly from the Maastrichtian formations of the ‘Massif de Ndiass’. Volcanic formation of the Cap Vert area does not represent a major source, except in the area of the extremity of the peninsula. The old ferricretes do not significantly contribute to the recent accumulation. The ‘ilmenites’ concentration along the beach lineis controlled by the different sedimentary cycles; the nouakchottian transgression beeing probably the most important event. In the Senegalese basin, a significant amount of the ‘ilmenites’ originated from the ‘Continental Terminal’ formation appears to derive from basic metamorphic rocks of the Mauritanide orogen. In the northern part of the basin, ‘ilmenite’ assemblage contains grains suggesting intermediate to acidic magmatic parental rocks. The calc-alkaline igneous complex from the structural units emplaced in the late Paleozoic on the NW margin of the Mauritanide orogen, and the Reguibat uplift, are two possible sources. The ‘ilmenite’ association found in the Maastrichtian formation probably derives from various paleozoic formations but its primary origin can not be deciphered.  相似文献   

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