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991.
Donaldo Mauricio Bran Jorge Gabriel Lozano Dario Civile Emanuele Lodolo María E. Cerredo Alejandro Tassone Luca Baradello Maurizio Grossi Juan Vilas 《第四纪科学杂志》2020,35(3):396-409
Lago Roca/Acigami is a “fjord-type” lake located in the southernmost part of South America, in the proximity of the Beagle Channel. A high-resolution seismic survey was carried out to analyse the seismic stratigraphy of the lake and to shed some light on the post-Last Glacial Maximum history of the area. Six seismic units were recognised, and their nature and depositional context were interpreted using seismic stratigraphy and acoustic facies analysis. A buried large ridge was identified within the glacial unit (SU1), interpreted as a frontal moraine that indicates a stabilisation phase. After retreat of the glacier from the basin, the trough was flooded by meltwater and a lake developed (SU2). The seismic facies, from bottom to top, depict a transition from ice-contact (SU2; SU3) to ice-distal proglacial conditions (SU4). A thick draping unit (SU5) marks a marine transgressive event and the instauration of a fjord environment in the basin. The marine transgression was a rapid event preceded by a fall in the lake level that caused an erosional unconformity. During the fjord phase the sedimentation remained controlled by meltwater discharge. Sea level fall, and subsequent disconnection from the Beagle Channel was accompanied by a progradation of the glaciofluvial deltaic sediments and the occurrence of several mass-wasting deposits (SU6). © 2019 John Wiley & Sons, Ltd. 相似文献
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Prof. Juan L. de Vivero Suárez 《GeoJournal》1990,22(2):220-220
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Starting from the Hamiltonian model for a solid Earth with an elastic mantle previously developped by the authors, analytical expressions are derived which give the nutation series corresponding to the plane perpendicular to the angular momentum vector, to the plane perpendicular to the rotational axis and to the equator of figure, as well as the series that give the polar motion. The effects of the different perturbations — solid Earth, centrifugal and tidal potentials — are calculated separately. The corrections due to the elasticity of the mantle, which mostly correspond to the Oppolzer terms, are calculated with an accuracy of 10–6 arc sec., given that the intrinsic observational accuracy has reached 0.01 mas. 相似文献
998.
Andrés E. Piatti Ata Sarajedini Doug Geisler Juan Seguel David Clark 《Monthly notices of the Royal Astronomical Society》2005,358(4):1215-1230
Colour–magnitude diagrams (CMDs) are presented for the first time for 10 star clusters projected on to the Small Magellanic Cloud (SMC). The photometry was carried out in the Washington system C and T 1 filters allowing the determination of ages by means of the magnitude difference between the red giant clump and the main-sequence turnoff (MSTO), and metallicities from the red giant branch (RGB) locus. The clusters all have ages in the range 1.5–4 Gyr and metallicities between −1.3 < [Fe/H] < −0.6 , with respective errors of ∼0.5 Gyr and 0.3 dex. This increases substantially the sample of intermediate-age clusters in the SMC with well-derived parameters. We combine our results with those for other clusters in the literature to derive as large and homogeneous a data base as possible (totalling 26 clusters) in order to study global effects. We find evidence for two peaks in the age distribution of SMC clusters, at ∼6.5 and 2.5 Gyr, in good agreement with previous hints involving smaller samples. The most recent peak occurs at a time that corresponds to a very close encounter between the Large Magellanic Cloud (LMC) and the SMC according to the recent dynamical models of Bekki et al. that they used to explain the enhancement of LMC clusters with this age. It appears cluster formation may have been similarly stimulated in the SMC by this encounter as well. We also find very good agreement between cluster ages and metallicities and the prediction from a bursting model from Pagel and Tautvaišienė with a burst that occurred 3 Gyr ago. These two lines of evidence together favour a bursting cluster formation history as opposed to a continuous one for the SMC. 相似文献
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利用秦巴山区88个气象站1975—2016年的逐日气温数据,结合16个极端气温指数分析了秦巴山区极端气温阈值的空间分布及极端气温事件变化趋势的海拔依赖性。结果表明:极端气温阈值存在明显的空间分布差异,表现为极端低温阈值与极端高温阈值由西北向东南均有增温趋势;总体来看,极端气温暖事件(SU25、TR20、TX90P、TN90P、WSDI)增加幅度大于冷事件(FD0、ID0、TX10P、TN10P、CSDI)减少幅度,且变化趋势较冷事件更显著;全区霜冻日数、夏日日数、冷夜日数、暖昼日数及高温极值(TXx、TXn)变化均比较显著;区域作物生长期西部增长趋势较东部显著,多数站点变化幅度在3~6 d/10a之间;海拔越高发生极端低温事件的气温越低,极端低温阈值变化趋势为-0.36℃/100m;海拔越低发生极端高温事件的气温越高,极端高温变化趋势达0.5℃/100m,且均通过99%的信度检验;区域极端气温极值指数的变化趋势与海拔呈显著正相关,具有明显的海拔依赖性,表现为海拔越高,极值指数增加趋势越明显。 相似文献