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771.
Fluvial styles recorded by the uppermost part of the Neoproterozoic ‘Rivieradal sandstones' succession of eastern North Greenland reflect variations in rate of generated accommodation space and possibly climatic changes. Three facies associations, arranged in two genetic sequences, are recognised within the succession. The lower sequence initially records little available accommodation space. A high degree of reworking results in sheet-like, high-energy, bed-load-dominated, braided river deposits lacking recurrent facies patterns. As accommodation space increases upwards through the sequence, reduction in reworking is recorded by the development of fining- and thickening-upward muddy fluvial cycles. Evidence of desiccation or prolonged periods of drought are absent within the deposits and climate was probably relatively humid. Channel deposits in the lower sequence reflect mixed-load, braided fluvial systems with stable channel banks and floodplains, and the gradient appears to have been low to moderate. These features are generally considered favourable for the establishment of meandering river systems, but channels, nevertheless, retained an overall braided character and their deposits show no evidence of meandering. Despite indications of a climatic setting without significant periods of drought sediments indicate that large fluctuations in discharge occurred within the mixed-load streams and this is suggested to be the main cause for the absence of meandering. The swift and rather dramatic response of the fluvial systems to changes in precipitation, probably resulted from rapid runoff rates caused by the absence of vegetation. The upper sequence shows an initial return to shallow, sandy braided river deposition recording little available accommodation space. A subsequent increase in the rate of generated accommodation space is indicated by the presence of alternating sheet sandstones and sand-streaked mudstones with abundant desiccation cracks. The sheet sandstones show evidence of high-energy, unconfined ephemeral fluvial flash-flood deposition, while the mudstones are interpreted to represent muddy floodplain deposits. The change in fluvial style, combined with the widespread evidence of desiccation, suggest an evolution towards a more semi-arid climate in the upper sequence. This climatic change could account for the reduced clastic input seen in the overlying marine succession which culminated in carbonate platform deposition. The present study suggests that even under conditions considered favourable for the formation of meandering streams, these will rarely occur in Proterozoic deposits due to the lacking influence of vegetation. Although meandering deposits cannot be ruled out as having formed in pre-vegetational times, the conditions for their formation appear to have been even more restricted than previously realised. 相似文献
772.
Dabrio Cristino J. Zazo Cari Lario Javier Goy José Luis Sierro Francisco J. Borja Francisco González José Ángel Flores José Abel 《Geologie en Mijnbouw》1998,77(3-4):263-281
This first sedimentary interpretation of two incised-valley fills in the Gulf of Cádiz (southern Spain), which accumulated during the last fourth-order eustatic cycle in response to fluvial incision, changes of sea level, and correlative deposition, relates the filling of the estuarine basins and their barriers with four regional progradation phases, H1 to H4. The cases studied are the wave-dominated Guadalete, and the mixed, tide and wave-dominated Odiel-Tinto estuaries. The sequence boundary is a type-1 surface produced during the lowstand of the Last Glacial period ca. 18 000 14C yr BP. No fluvial lowstand deposits were found in the area. Due to rapid transgression the valley fills consist of transgressive and highstand sediments. The maximum landward advance of the estuarine barriers occurred ca. 6500–6000 14C yr BP during the maximum of the Flandrian transgression, but there is no evidence of sea level rising appreciably above the present. A large part of the estuaries was filled during H1 (ca. 6500–4400 14C yr BP) but ravinement by shifting tidal inlets destroyed most of the coeval barriers. During the H2 phase (ca. 4200–2550 14C yr BP) sedimentation was favoured by arid conditions and concentrated in the axial estuarine zones and the barriers. Between H2 and H3 prevailing winds changed from W to WSW, increasing spit growth to the east and south-east. Progradation of bay-head deltas and flood-plains during H3 (ca. 2300–800 14C yr BP) and H4 (500 yr ago to the present) further reduced the accommodation space in the largely-filled valleys, and sediment by-passed the estuaries and accumulated in the estuarine barriers as fast-growing spits. Arid conditions and increasing human activity have caused rapid coastal modifications. 相似文献
773.
On the use of microtremor recordings in seismic microzonation 总被引:4,自引:0,他引:4
M. Bour D. Fouissac P. Dominique C. Martin 《Soil Dynamics and Earthquake Engineering》1998,17(7-8):465-474
Experimental methods involving microtremor recordings are useful for determining site effects in regions of moderate seismic activity where ground motion records are few, and in urban or industrial contexts where the noise level is high. The aim of this study is to establish a microzonation by using the Nogoshi–Nakamura method,[1, 2] a simple experimental technique based on microtremor recordings. Since the physical phenomena underlying the method are only partially understood, the spectral responses obtained cannot be used alone. We, therefore, complete our experimental results by comparing them with the solutions of a one-dimensional numerical simulation (SHAKE91).[3, 4] The experimental programme was carried out on a plain near the Rhone Delta (South of France). H/V spectral ratios were calculated at 137 noise measurement points. In addition, we were able to compute the numerical transfer functions from soil columns defined by geotechnical characteristics inside the studied region. A comparison of the results obtained by the experimental and numerical methods showed that the fundamental frequencies are in good agreement, but that the amplitudes obtained by the two techniques are sometimes different. The analysis of H/V spectral ratios enabled us to establish maps to characterize the region: a resonance frequency map and maps of amplification levels as a function of frequency range, leading to a seismic microzonation for the whole of the region. 相似文献
774.
Mihály Horányi 《Astrophysics and Space Science》1998,264(1-4):257-271
This is a review of recent in situ and remote sensing observations, and theoretical advances of our understanding dust plasma
interactions in Jupiter's magnetosphere. Dust grains exposed to plasmas and UV radiation collect electrostatic charges and
their dynamics can be altered due to electric and magnetic fields. Hence, magnetospheric effects can shape the size and spatial
distributions of micron sized and smaller dust grains. The ring/halo region, the dust streams and the captured ring at Jupiter
are recent examples where dust plasma interaction effects can best explain the observations.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
775.
776.
The Gran Telescopio CANARIAS (GTC) is a high performance 10-m class telescope whose construction has been promoted by the
IAC (Instituto de Astrofísica de Canarias). It will be installed at the Roque de los Muchachos Observatory (ORM), in the island
of La Palma. First light is planned for end-2002. The key science drivers for the project are image quality, operational efficiency
and reliability, as emphasized in the Conceptual Design Document which was finished in mid-97. The Preliminary Design is now
proceeding on all aspects of the project. The GTC Project is presently funded at the 70% level by Spain. The scientific drives
behind the GTC project are described here, as well as the current technical, managerial, and operational baseline.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
777.
Martin A. Lee 《Astrophysics and Space Science》1998,264(1-4):497-508
The interaction of interstellar pickup ions with the solar wind termination shock is reviewed and assessed. The pickup ions
mass and momentum load the wind and increase its pressure, effects which decrease the strength of the shock and its distance
from the Sun. The pickup hydrogen may contribute substantially to the "reflected" ion population, which should provide most
of the dissipation at the supercritical quasi-perpendicular shock. A fraction of the pickup ions impinging on the shock is
"injected" into the process of diffusive shock acceleration to form the anomalous cosmic ray component. An injection mechanism
which accounts for the apparent absence of solar wind ions in the anomalous component is "shock surfing", in which pickup
ions which approach the shock slowly may be trapped between the upstream Lorentz force and the shock potential and accelerated
in the motional electric field beyond the energy threshold for diffusive shock acceleration. However, the simplest interpretation
of shock surfing would favor less massive pickup ion species, in contradiction with Voyager observations of anomalous component
composition. A possible extension of the shock surfing mechanism is considered, as well as other injection mechanisms. Finally,
the pressure of the anomalous component may modify the structure of the termination shock, which in turn may influence injection
rates.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
778.
779.
Our main goal is to determine the dynamic equations of a certain complex system, as is the case of the mechanical system for
a small aperture telescope. Causes of this complexity are: the lack of documents about the operation of the elements belonging
to the system, and the variation of dynamics with respect to the time and the position of the telescope. To check that we
have obtained a valid set of dynamic equations, we will design a computer control system that will implement a self-guide
system for the telescope.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
780.
Simon J. Woodings rew J. Williams Ralph Martin Ronald R. Burman & David G. Blair 《Monthly notices of the Royal Astronomical Society》1998,301(1):L5-L9
Following the proposal by Damineli that the central object of Eta Carinae may be an early-type binary, we perform numerical simulations of the X-ray emission from colliding stellar winds. A synthetic light curve has been generated which qualitatively agrees with the recent X-ray variability, and provides further support for the binary model. In particular, the model predicts a rise in the observed X-ray emission towards periastron, followed by a sharp drop and subsequent recovery. This is indeed what is seen in the RXTE light curve, although some problems concerning the X-ray spectrum at periastron still need to be explained. The simulations suggest that the width of the periastron dip will provide strong constraints on the binary and stellar wind properties of the components of Eta Car. 相似文献