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11.
Traditionally, most formulations of dynamic halfspace problems have represented the material as either an elastic or a viscoelastic solid. Herein the counterpart of Lamb's elastodynamic problem is reformulated and solved for a liquid-saturated poroelastic halfspace using Biot's theory of poroelasticity. The responses of the solid and fluid phases are evaluated due to steady-state harmonic concentrated loads applied to each phase at the surface. The solutions are presented over a broad range of permeabilities and are compared to solutions to Lamb's problem for equivalent drained and undrained solids. Methodology is then introduced by which these results are treated as Green functions for the solution of a mixed boundary-value problem. namely, the response of the poroelastic halfspace to steady-state harmonic vertical motion of a rigid. massless plate. It is observed that small differences exist among overall compliance functions for a drained solid, an undrained solid, and a liquid-saturated porous, halfspace. However, use of the poroelastic model permits the distribution between effective skeletal normal stresses and fluid stresses to be determined. 相似文献
12.
In the last four years we have carried out a number of studies on the radiative and collisional processes in theA
2
i
state of CN. Many of these of interest to those studying planetary atmospheres, comets and solar spectra are summarized in this paper. Data for CNA
2
i
fluorescence lifetimes and quenching rates, and collisional energy transfer between CNA
2
i
andX
2+ are reported. Detailed comparisons and a discussion of the results may be found in several already published papers. 相似文献
13.
14.
Leopold Müller-Salzburg 《Engineering Geology》1987,24(1-4):423-444
15.
We present the latest results from a multi-epoch timing and spectral study of the Transient Anomalous X-ray Pulsar XTE J1810–197.
We have acquired seven observations of this pulsar with the Newton X-ray Multi-mirror Mission (XMM-Newton) over the course
of two and a half years, to follow the spectral evolution as the source fades from outburst. The spectrum is arguably best
characterized by a two-temperature blackbody whose luminosities are decreasing exponentially with τ
1=870 d and τ
2=280 d, respectively. The temperatures of these components are currently cooling at a rate of 22% per year from a nearly constant
value recorded at earlier epochs of kT
1=0.25 keV and kT
2=0.67 keV, respectively. The new data show that the temperature T
1 and luminosity of that component have nearly returned to their historic quiescent levels and that its pulsed fraction, which
has steadily decreased with time, is now consistent with the previous lack of detected pulsations in quiescence. We also summarize
the detections of radio emission from XTE J1810–197, the first confirmed for any AXP. We consider possible models for the
emission geometry and mechanisms of XTE J1810–197.
XMM-Newton is an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This
research is supported by XMM-Newton grant NNG05GJ61G and NASA ADP grant ADP04-0059-0024. 相似文献
16.
Fine-grained lacustrine, riverine and ash-fall sediments of the Shooting Iron Formation, whose late Pliocene age is established by Blancan gastropods and vertebrates, yield a pollen flora that is essentially similar in composition to the modern pollen rain in the Jackson Hole area. The Pliocene assemblage suggests a climate like that of the Jackson valley and foothills today. These spectra also resemble a Pliocene pollen flora from Yellowstone Park dated at ∼ 2.02 Ma. However, the underlying Miocene Teewinot sediments differ by containing pollen of four exotic deciduous hardwoods (Tertiary relicts) that suggest a summer-moist climate, unlike that of today. The Shooting Iron sediments lie with an angular unconformity on and above the Miocene lake sediments of the Teewinot Formation. Both of these deposits probably preceded the main uplift of the Teton Range based on the absence of Precambrian clasts in the Tertiary valley deposits. Because the Pliocene floras were modern in aspect, a Plio-Pleistocene transition would be floristically imperceptible here. The sequence denotes a protracted period of relative stability of climate during Teewinot time, and a shift in vegetational state (summer-wet trees drop out) sometime between the latest Miocene and latest Pliocene. The Pliocene spectra suggest a dry, cooler climate toward the end of Shooting Iron time. 相似文献
17.
18.
Activity and stability phases as well as geomorphic processes within the Critical Zone are well known. Erosion and deposition of sediments represent activity; soils represent geomorphic stability phases. Data are presented from a 4 m deep sediment section that was dated by luminescence techniques. Upslope erosion and resulting sedimentation started in the late Pleistocene around 18 ka until 12 ka. Conditions at the study site then changed, which led to the formation of a well-developed soil. Radiocarbon dating of the organic matter yielded ages between 8552 and 8995 cal. BP. From roughly 6.2 to 5.4 ka another activity phase accompanied by according sediment deposition buried the soil and a new soil, a Cambisol, was formed at the surface. The buried soil is a strongly developed Luvisol. The black colors in the upper part of the buried soil are not the result of pedogenic accumulation of normal organic matter within an A-horizon. Nuclear magnetic resonance spectroscopy clearly documents the high amount of aromatic components (charcoal), which is responsible for the dark color. This indicates severe burning events at the site and the smaller charcoal dust (black carbon) was transported to deeper parts of the profile during the process of clay translocation. 相似文献
19.
20.
R. J. Ivison T. R. Greve J. S. Dunlop J. A. Peacock E. Egami Ian Smail E. Ibar E. van Kampen I. Aretxaga T. Babbedge A. D. Biggs A. W. Blain S. C. Chapman D. L. Clements K. Coppin D. Farrah M. Halpern D. H. Hughes M. J. Jarvis T. Jenness J. R. Jones A. M. J. Mortier S. Oliver C. Papovich P. G. Pérez-González A. Pope S. Rawlings G. H. Rieke M. Rowan-Robinson R. S. Savage D. Scott M. Seigar S. Serjeant C. Simpson J. A. Stevens M. Vaccari J. Wagg C. J. Willott 《Monthly notices of the Royal Astronomical Society》2007,380(1):199-228