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111.
112.
Luisa Patiño Maria Isabel Velez Marion Weber César A. Velásquez-r Santiago David Manuela Rueda Ivonne Castañeda Diana Arboleda 《第四纪科学杂志》2020,35(8):1046-1056
This study presents the first multi-proxy palaeoenvironmental and palaeoclimatic history for northern South America based on the palaeolimnological reconstruction of a pond located in a dry paramo at 3570 masl. During the Last Glacial Maximum (LGM), the study area was under glacial conditions, then during global events Heinrich Stadial 1 (HS1), Bølling–Allerød (BA), and the Younger Dryas (YD), the pond expanded, accumulation rates and proxies for erosion reached the highest values, indicative of humid conditions, with maxima in humidity during the BA and YD. Dry conditions and pond desiccation occurred in the Greenlandian–Northgrippian and by 6010 cal a bp the area was transformed into the mire of today. Comparisons with records from other sites in South America indicate that changes in humidity are most likely controlled by the Intertropical Convergence Zone, mainly during the glacial and postglacial, and by changes in the Pacific Ocean, more pronounced after the YD. 相似文献
113.
Edward Olsen Andrew Davis Roy S. Clarke Ludolf Schultz Hartwig W. Weber Robert Clayton Toshiko Mayeda Eugene Jarosewich Paul Sylvester Lawrence Grossman Ming-Sheng Wang Michael E. Lipschutz Ian M. Steele James Schwade 《Meteoritics & planetary science》1994,29(2):200-213
Abstract— Watson, which was found in 1972 in South Australia, contains the largest single silicate rock mass seen in any known iron meteorite. A comprehensive study has been completed on this unusual meteorite: petrography, metallography, analyses of the silicate inclusion (whole rock chemical analysis, INAA, RNAA, noble gases, and oxygen isotope analysis) and mineral compositions (by electron microprobe and ion microprobe). The whole rock has a composition of an H-chondrite minus the normal H-group metal and troilite content. The oxygen isotope composition is that of the silicates in the HE iron meteorites and lies along an oxygen isotope fractionation line with the H-group chondrites. Trace elements in the metal confirm Watson is a new HE iron. Whole rock Watson silicate shows an enrichment in K and P (each ~2X H-chondrites). The silicate inclusion has a highly equilibrated igneous (peridotite-like) texture with olivine largely poikilitic within low-Ca pyroxene: olivine (Fa20), opx (Fs17Wo3), capx (Fs9Wo41) (with very fine exsolution lamellae), antiperthite feldspar (An1–Or5) with <1 μm exsolution lamellae (An1–3Or>40), shocked feldspar with altered stoichiometry, minor whitlockite (also a poorly characterized interstitial phosphate-rich phase) and chromite, and only traces of metal and troilite. The individual silicate minerals have normal chondritic REE patterns, but whitlockite has a remarkable REE pattern. It is very enriched in light REE (La is 720X C1, and Lu is 90X C1, as opposed to usual chonditic values of ~300X and 100–150X, respectively) with a negative Eu anomaly. The enrichment of whole rock K is expressed both in an unusually high mean modal Or content of the feldspar, Or13, and in the presence of antiperthite. Whole rock trace element data for the silicate mass support the petrography. Watson silicate was an H-chondrite engulfed by metal and melted at > 1550 °C. A flat refractory lithophile and flat REE pattern (at ~1x average H-chondrites) indicate that melting took place in a relatively closed system. Immiscible metal and sulfide were occluded into the surrounding metal host. Below 1100 °C, the average cooling rate is estimated to have been ~1000 °C/Ma; Widmanstätten structure formed, any igneous zoning in the silicates was equilibrated, and feldspar and pyroxene exsolution took place. Cooling to below 300 °C was completed by 3.5 Ga B. P. At 8 Ma, a shock event took place causing some severe metal deformation and forming local melt pockets of schreibersite/metal. This event likely caused the release of Watson into interplanetary space. The time of this event, 8Ma, corresponds to the peak frequency of exposure ages of the H-chondrites. This further confirms the link between HE irons and the H-chondrites, a relationship already indicated by their common oxygen isotope source. Watson metal structures are very similar to those in Kodaikanal. Watson, Kodaikanal and Netschaëvo form the young group of HE meteorites (ages 3.7 ± 0.2 Ga). They appear to represent steps in a chain of events that must have taken place repeatedly on the HE parent body or bodies from which they came: chondrite engulfed in metal (Netschaëvo); chondrite melted within metal (Watson); and finally melted silicate undergoing strong fractionation with the fractionated material emplaced as globules within metal (Kodaikanal). Watson fills an important gap in understanding the sequence of events that took place in the evolution of the IIE-H parent body(ies). This association of H-chondrite with HE metal suggests a surface, or near surface process-a suggestion made by several other researchers. 相似文献
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115.
Problems concerning the resettlement of those made homeless by the construction of dams to create reservoirs in Thailand are considered. The authors attempt "firstly, to examine the rationale for spontaneous and planned resettlement in Thailand. Secondly, the determinants of the success or failure of resettlers are explored with reference to selected planned resettlement projects. Finally, resettlement alternatives for prospective reservoir evacuees are proposed." 相似文献
116.
D. Kesten M. Weber Ch. Haberland Ch. Janssen A. Agnon Y. Bartov I. Rabba The DESERT Group 《International Journal of Earth Sciences》2008,97(1):153-169
The left-lateral Dead Sea Transform (DST) in the Middle East is one of the largest continental strike-slip faults of the world.
The southern segment of the DST in the Arava/Araba Valley between the Dead Sea and the Red Sea, called Arava/Araba Fault (AF),
has been studied in detail in the multidisciplinary DESERT (DEad SEa Rift Transect) project. Based on these results, here,
the interpretations of multi-spectral (ASTER) satellite images and seismic reflection studies have been combined to analyse
geologic structures. Whereas satellite images reveal neotectonic activity in shallow young sediments, reflection seismic image
deep faults that are possibly inactive at present. The combination of the two methods allows putting some age constraint on
the activity of individual fault strands. Although the AF is clearly the main active fault segment of the southern DST, we
propose that it has accommodated only a limited (up to 60 km) part of the overall 105 km of sinistral plate motion since Miocene
times. There is evidence for sinistral displacement along other faults, based on geological studies, including satellite image
interpretation. Furthermore, a subsurface fault is revealed ≈4 km west of the AF on two ≈E–W running seismic reflection profiles.
Whereas these seismic data show a flower structure typical for strike-slip faults, on the satellite image this fault is not
expressed in the post-Miocene sediments, implying that it has been inactive for the last few million years. About 1 km to
the east of the AF another, now buried fault, was detected in seismic, magnetotelluric and gravity studies of DESERT. Taking
together various evidences, we suggest that at the beginning of transform motion deformation occurred in a rather wide belt,
possibly with the reactivation of older ≈N–S striking structures. Later, deformation became concentrated in the region of
today’s Arava Valley. Till ≈5 Ma ago there might have been other, now inactive fault traces in the vicinity of the present
day AF that took up lateral motion. Together with a rearrangement of plates ≈5 Ma ago, the main fault trace shifted then to
the position of today’s AF. 相似文献
117.
The International GLONASS Service – Pilot Project (IGLOS-PP), a project of the International GPS Service, was launched in
order to underscore the importance and benefits of integrating data from multiple systmes and techniques within IGS products.
At first this article summarizes the contributing organizations and the available infrastructure. Later on the GLONASS related
modeling techniques at the involved IGS Analysis Centers are described and we conclude with some remarks concerning the advantages
for the expected user commmunity. ? 2001 John Wiley & Sons, Inc. 相似文献
118.
Evaluation and comparison of spatial interpolators 总被引:16,自引:0,他引:16
This study evaluates 15 different estimators to determine their relative merits in estimating block concentrations at contaminant waste sites. The evaluation was based on 54 subsets of data drawn from an exhaustive set of 19,800 data. For each subset, 198 block estimates were made with each estimator. The measurements of estimation quality were a linear loss function and a more standard statistic, the mean square error. The linear loss function showed that seven of the estimators produced scores close enough to be within the same statistical population. Results based on the mean square error were similar. The surprising results of this study were that inverse distance and inverse distance squared both produced better scores than kriging. 相似文献
119.
120.
A three-dimensional dam-reservoir system under seismic load is analysed. The dam is assumed to be rigid. The reservoir is an infinite channel with semi-circular cross-section. The exact analytical solution, based on the assumption of potential fluid motion is presented, as well as numerical results for selected parameters.The most significant parameters are: the direction and frequency content of the seismic input; the radiation damping at the reservoir bottom; and the compressibility of the fluid. The response of the system depends strongly on the direction of the input ground motion. This is shown by the transfer functions as well as by the pressure time histories due to two earthquakes with different frequency content. The energy absorption at the reservoir bottom is important. A simple plane-wave model shows, that even for a rock foundation, the amount of transmitted energy can reach up to 80%. For comparison the case without bottom absorption is also shown. Compressbility has to be included to capture the resonance effects. The exact analytical solution is also used to verify numerical results obtained by a new method that combines a finite element model with a rigorous radiation boundary for the infinite channel in the time domain. 相似文献