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71.
72.
Short-term risk forecasts of point precipitation are obtained with COTREC/RainCast, a technique for extrapolation of radar images. The risk forecasts are updated every 5 min for the next 0–2 h. Risk levels are defined for moderate, heavy and extreme precipitation. Warning messages are generated if, at the locations of 23 rain gauges, these risk levels are reached or exceeded. The time-resolved gauge data are used to judge if the warning messages are in time, early or late.Data over a period of 4 months (summer 2002) are used for verification. The largest number of warnings (1790) was obtained for moderate precipitation. About 55% of these warnings were in time, 23% were early and 22% were late. This finding is in a good agreement with the defined risk level for warnings (50%), indicating that the model for calculating the risk factors is reliable. Less warnings in time, and more late warnings were found for heavy and extreme precipitation. Hence, the risk levels need to be lowered for heavy and extreme precipitation, in order to reduce the number of late warnings. 相似文献
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Marc Rütschlin Johannes H. Cloete Iain M. Mason Keith D. Palmer 《Journal of Applied Geophysics》2007,62(4):354-360
A new measurement technique enables the complex dielectric properties of the geological strata comprising the UG1–UG2 (Upper Group 1–Upper Group 2) unit of the Bushveld Complex in South Africa to be determined with unprecedented detail at radio frequencies (RF). Results of non-destructive laboratory measurements of representative diamond drill core samples from the UG1–UG2 unit are presented at 25 MHz. These data establish that the UG1 and UG2 chromitite layers are embedded in rock strata (norite, pyroxenite and anorthosite) which are translucent in the HF spectral band, whereas the chromitite layers themselves exhibit significant velocity contrast, making them good radar reflectors. The data presented here is useful for calibration of the radar system, and for predicting the range and resolution performance of borehole radars operating in both the hanging and footwalls of the economically important platiniferous UG2 reef. 相似文献
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Surface sediment samples were collected from the Squamish River Delta, British Columbia, in order to determine the role of sediment surface area in the preservation of organic matter (OM) in a paralic sedimentary environment. The Squamish Delta is an actively prograding delta, located at the head of Howe Sound.Bulk total organic carbon (TOC) values across the Squamish Delta are low, ranging from 0.1 to 1.0 wt.%. The carbon/total nitrogen ratio (Corg/N) ranges from 6 to 17, which is attributed to changes in OM type and facies variations. The <25-μm fraction has TOC concentrations up to 2.0 wt.%, and a Corg/N ratio that ranges from 14 to 16. The 53–106-μm fraction has higher TOC concentrations and Corg/N ratios relative to the 25–53-μm fraction. The Corg/N ratio ranges from 9 to 18 in the 53–106-μm fraction and 5.5–10.5 in the 25–53-μm fraction. Surface area values for bulk sediments are low (0.5–3.0 m2/g) due to the large proportion of silt size material. Good correlation between surface area and TOC in bulk samples suggests that OM is adsorbed to mineral surfaces. Similar relationships between surface area and TOC were observed in size-fractionated samples. Mineralogy and elemental composition did not correlate with TOC concentration.The relationships between surface area, TOC and total nitrogen (TN) can be linked to the hydrodynamic and sedimentological conditions of the Squamish Delta. As a result, the Squamish Delta is a useful modern analogue for the formation of petroleum source rocks in ancient deltaic environments, where TOC concentrations are often significantly lower than those in source rocks formed in other geological settings. 相似文献
77.
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.
, (, ) , . , . , . . , Taveyane ( Coombs'y), , . .相似文献
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Absarokites from the western Mexican Volcanic Belt: constraints on mantle wedge conditions 总被引:1,自引:1,他引:0
Marc?Hesse Timothy?L.?GroveEmail author 《Contributions to Mineralogy and Petrology》2003,146(1):10-27
We have investigated the near liquidus phase relations of a primitive absarokite from the Mascota region in western Mexico. Sample M.102 contains ~11.6 wt% MgO, Mg#=0.73 and the lava contains Fo90 olivine phenocrysts, indicating near equilibrium with the mantle. High-pressure experiments on a synthetic analogue of the absarokite composition containing low and high H2O abundances of (~2 and ~5 wt%, respectively) were performed in a piston cylinder apparatus over the pressure range of 1.2 to 2.0 GPa. The composition containing ~2 wt% H2O is multiply saturated with olivine and orthopyroxene at 1.6 GPa and 1,400 °C. At the same pressure, clinopyroxene appears 30 °C below the liquidus. At an H2O content of ~5 wt% the multiple saturation with olivine and orthopyroxene occurs at 1.7 GPa and 1,300 °C. Assuming a batch-melting process, we suggest that the primitive absarokite was segregated from a depleted lherzolite or harzburgite residue at ~50 km, placing the depth of origin well within the mantle wedge beneath the Jalisco Block. A low degree (<5 %wt%) batch-melt of an original metasomatized depleted lherzolite or harzburgite source would contain the observed trace element abundances found in M.102. The liquidus phase relations are not consistent with the presence of non-peridotitic veins at the depth of last equilibration. Therefore, we propose that the Mascota absarokites segregated at an apparent melt fraction of less than 5% from a depleted peridotitic source. Melting first began at a greater depth as a small degree H2O- and trace element- rich melt of a metasomatized peridotite that ascended into the overlying wedge and re-equilibrated with shallower, hotter mantle.Editorial responsibility: J. Hoefs 相似文献
80.
Near-photospheric flow fields on the Sun are deduced using two independent methods applied to the same time series of velocity images observed by SOI-MDI on SOHO. Differences in travel times between f modes entering and leaving each pixel measured using time-distance helioseismology are used to determine sites of supergranular outflows. Alternatively, correlation tracking analysis of mesogranular scales of motion applied to the same time series is used to deduce the near-surface flow field. These two approaches provide the means to assess the patterns and evolution of horizontal flows on supergranular scales even near disk center, which is not feasible with direct line-of-sight Doppler measurements. We find that the locations of the supergranular outflows seen in flow fields generated from correlation tracking coincide well with the locations of the outflows determined from the time-distance analysis, with a mean correlation coefficient after smoothing of
s=0.890. Near-surface velocity field measurements can be used to study the evolution of the supergranular network, as merging and splitting events are observed to occur in these images. The data consist of one 2048-min time series of high-resolution (0.6 pixels) line-of-sight velocity images taken by MDI on 1997 January 16–18 at a cadence of one minute. 相似文献