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41.
Robert L. Nowack Wang-Ping Chen Ulrich Kruse Saptarshi Dasgupta 《Pure and Applied Geophysics》2007,164(10):1921-1936
We carry out a sequence of numerical tests to understand conditions under which rapid changes in crustal thickness can be
reliably imaged by teleseismic body waves. Using the finite-difference method over a 2-D grid, we compute synthetic seismograms
resulting from a planar P-wavefield incident below the grid. We then image the Moho using a migration scheme based on the Gaussian beam representation
of the wavefield. The use of Gaussian beams for the downward propagation of the wavefield is particularly advantageous in
certain geologically critical cases such as overthrusting of continental lithosphere, resulting in the juxtaposition of high-velocity
mantle material over crustal rocks. In contrast to ray-based methods, Gaussian beam migration requires no special treatment
to handle such heterogeneities. Our results suggest that with adequate station spacing and signal-to-noise ratios, offsets
of the Moho, on the order of 10 km in height, can be reliably imaged beneath thickened crust at depths of about 50 km. Furthermore,
even sharp corners and edges are faithfully imaged when precise values of seismic wave speeds are available. Our tests also
demonstrate that flexibility in choices of different types of seismic phases is important, because any single phase has trade-offs
in issues such as spatial resolution, array aperture, and amplitude of signals. 相似文献
42.
Is pure groundwater safe to drink?: natural "contamination' of groundwater in Norway 总被引:1,自引:0,他引:1
David Banks Aase Kjersti Midtgrd Geir Morland Clemens Reimann Terje Strand Kjell Bjorvatn & Ulrich Siewers 《Geology Today》1998,14(3):104-113
The title of this article is designed to provoke. Naturally occurring parameters are, by definition, not contamination. Nevertheless, nature is not necessarily nice, and naturally occurring trace toxins can be every bit as undesirable as their counterparts derived from human pollution. 相似文献
43.
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45.
Dr. Ulrich Jux 《International Journal of Earth Sciences》1975,64(1):523-540
In the region of Bande Amir, located on the southern rim of the Tadschik basin, the Mesozoic section starts with detrital and conglomeratic limestones. These marine deposits of Upper Cretaceous age (Cenomanian-Turonian) disconformably cover a truncated complex of Upper Paleozoic rocks (Permian). After an interval of neritic sedimentation (Santonian, Campanian) the Upper Cretaceous sea (Maastrichtian) regressed from the Central Afghanian High. In the Hindukusch mountains the regression is related to crustal movements and regional uplifts, which hinged on the Herat lineament. Intermontane basins, developed on this mobile zone during mid-Tertiary time, gathered continental debris (Neogene conglomerates; Zohak-Formation) and led to the deposition of lacustrine sediments (Ghulghola-Formation). Orogenetic movements along the colliding edges of crustal blocks were rejuvenated in Plio-Pleistocene time, shifting the focus of deposition to the northwest. The basin was finally captured by the Amu Darja drainage system, leading to the development of canyon-like incisions. During warm periods of the Quaternary, fluviatile erosion in Bande Amir was interrupted at least four times by the retention of water behind large dams of travertine. 相似文献
46.
Dr. Richard F. Wright Prof. Albert Matter Marc Schweingruber Ulrich Siegenthaler 《Aquatic Sciences - Research Across Boundaries》1980,42(2):101-126
A 2-year study of sedimentation in Lake Biel reveals that three major factors can account for the spatial and temporal patterns
of tripton sedimentation. Allochthonous inputs of particulate matter mostly derived from the Aare river during spring snowmelt
and other high-water periods, provide about 50% of the carbonate and 50% of the siliceous matter collected in sediment traps.
Phytoplankton activity in this eutrophic, hard-water lake accounts for the rest of the carbonate and siliceous matter, the
latter being mostly diatom frustules. Sedimentation rates are thus highest during periods of maximum river flooding, maximum
phytoplankton activity and following the breakdown of the thermocline, at which time trapped particles settle out. Resuspension
of sediment is important in at least one basin. Resolution of carbonate appears to be minor. 相似文献
47.
Peter Suter-Weider Dr. Ulrich Zimmermann 《Aquatic Sciences - Research Across Boundaries》1976,38(2):159-170
The freshwater musselDreissena polymorpha Pallas was sighted for the first time in Lake Zürich about 1969. This meant a real problem for the water treatment of lake
water. By means of a pump and vertical net hauls it was tried to add more information to the scarce results on Lake Zürich.
Additional dates about temperature, depth of Secchi disk visibility and beam transmittance were collected. There was a first
appearance of the larvae ofD. polymorpha at the beginning of June. Following the mean temperature of the epilimnion the number of individuals/m2 reached max. 210,000. The greatest concentration measured in 1974 of larvae/m3 was 54,375 at a depth of 4 m. The last appearance ofD. polymorpha was observed at the end of October.
相似文献
48.
Donald C. Noble Edwin H. McKee Edward Farrar Ulrich Petersen 《Earth and Planetary Science Letters》1974,21(2):213-220
Radiometric and geologic information indicate a complex history of Cenozoic volcanism and tectonism in the central Andes. K-Ar ages on silicic pyroclastic rocks demonstrate major volcanic activity in central and southern Peru, northern Chile, and adjacent areas during the Early and Middle Miocene, and provide additional evidence for volcanism during the Late Eocene. A provisional outline of tectonic and volcanic events in the Peruvian Andes during the Cenozoic includes: one or more pulses of igneous activity and intense deformation during the Paleocene and Eocene; a period of quiescence, lasting most of Oligocene time; reinception of tectonism and volcanism at the beginning of the Miocene; and a major pulse of deformation in the Middle Miocene accompanied and followed through the Pliocene by intense volcanism and plutonism. Reinception of igneous activity and tectonism at about the Oligocene-Miocene boundary, a feature recognized in other circum-Pacific regions, may reflect an increase in the rate of rotation of the Pacific plate relative to fixed or quasifixed mantle coordinates. Middle Miocene tectonism and latest Tertiary volcanism correlates with and probably is genetically related to the beginning of very rapid spreading at the East Pacific Rise. 相似文献
49.
50.
Susanne P. Schwenzer Siegfried Herrmann Ratan K. Mohapatra Ulrich Ott 《Meteoritics & planetary science》2007,42(3):387-412
Abstract— This study provides a complete data set of all five noble gases for bulk samples and mineral separates from three Martian shergottites: Shergotty (bulk, pyroxene, maskelynite), Zagami (bulk, pyroxene, maskelynite), and Elephant Moraine (EET) A79001, lithology A (bulk, pyroxene). We also give a compilation of all noble gas and nitrogen studies performed on these meteorites. Our mean values for cosmic‐ray exposure ages from 3He, 21Ne, and 38Ar are 2.48 Myr for Shergotty, 2.73 Myr for Zagami, and 0.65 Myr for EETA79001 lith. A. Serious loss of radiogenic 4He due to shock is observed. Cosmogenic neon results for bulk samples from 13 Martian meteorites (new data and literature data) are used in addition to the mineral separates of this study in a new approach to explore evidence of solar cosmic‐ray effects. While a contribution of this low‐energy irradiation is strongly indicated for all of the shergottites, spallation Ne in Chassigny, Allan Hills (ALH) 84001, and the nakhlites is fully explained by galactic cosmic‐ray spallation. Implanted Martian atmospheric gases are present in all mineral separates and the thermal release indicates a near‐surface siting. We derive an estimate for the 40Ar/36Ar ratio of the Martian interior component by subtracting from measured Ar in the (K‐poor) pyroxenes the (small) radiogenic component as well as the implanted atmospheric component as indicated from 129Xe, * excesses. Unless compromised by the presence of additional components, a high ratio of ~2000 is indicated for Martian interior argon, similar to that in the Martian atmosphere. Since much lower ratios have been inferred for Chassigny and ALH 84001, the result may indicate spatial and/or temporal variations of 40Ar/36Ar in the Martian mantle. 相似文献