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81.
Gunther Kletetschka Petr Schnabl Kristýna Šifnerová Zuzana Tasáryová Štěpán Manda Petr Pruner 《Studia Geophysica et Geodaetica》2013,57(1):103-117
Magnetic images have been produced at the distance of 0.1 mm from the polished basaltic thin sections of rocks from Prague Synform in Barrandian area. Three different magnetic textures were seen and when combined with optical imaging could be related to petrological features. The first magnetic texture revealed that most of the magnetic signature is localized within the amygdales formed later after the basalts became part of the sedimentary sequence. The second texture showed that the basaltic body contains large grain size distribution of magnetic carriers possibly with variable viscous magnetizations. The third texture suggested a presence of magnetic anisotropy of igneous origin. Such textural magnetic information along with the paleomagnetic characteristics of the basaltic rocks of Silurian age constrained the overall geological interpretation. 相似文献
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84.
P. A. Rosen B. H. Wilde R. J. R. Williams J. M. Foster P. A. Keiter R. F. Coker T. S. Perry M. J. Taylor A. M. Khokhlov R. P. Drake G. R. Bennett D. B. Sinars R. B. Campbell 《Astrophysics and Space Science》2005,298(1-2):121-128
In recent years, we have carried out experiments at the University of Rochester’s Omega laser in which supersonic, dense-plasma
jets are formed by the interaction of strong shocks in a complex target assembly (Foster et al., Phys. Plasmas 9 (2002) 2251). We describe recent, significant extensions to this work, in which we consider scaling of the experiment, the
transition to turbulence, and astrophysical analogues. In new work at the Omega laser, we are developing an experiment in
which a jet is formed by laser ablation of a titanium foil mounted over a titanium washer with a central, cylindrical hole.
Some of the resulting shocked titanium expands, cools, and accelerates through the vacuum region (the hole in the washer)
and then enters a cylinder of low-density foam as a jet. We discuss the design of this new experiment and present preliminary
experimental data and results of simulations using AWE hydrocodes. In each case, the high Reynolds number of the jet suggests
that turbulence should develop, although this behaviour cannot be reliably modelled by present, resolution-limited simulations
(because of their low-numerical Reynolds number). 相似文献
85.
86.
An equation of state for cold matter at neutron star densities, >1014 gm/cm3, is evaluated. The gas is considered to be a degenerate mixture of neutrons, protons, leptons, hyperons and massive baryons. We derive the equilibrium equations including the effects of nuclear interactions among all the hadrons. 相似文献
87.
O. M. Rosen A. V. Soloviev D. Z. Zhuravlev 《Izvestiya Physics of the Solid Earth》2009,45(10):914-931
Thermal evolution of the continental crust beneath the northeastern Siberian craton was studied based on the interpretation
of apatite fission-track ages. The samples selected for AFT dating were collected from depths between 2 and 3 km along a 1000-km-long
profile, from the crystalline basement of the Siberian platform. The AFT ages range from 185 to 222 Ma, indicating that in
the late Triassic-early Cretaceous, the top of the crystalline basement was cooled below ∼100°C. Once the apatite cooled below
this temperature, it began to accumulate and preserve tracks produced by spontaneous fissioning of 238U, and the number of tracks preserved is effective in determining the ages of events using the apatite fission-track method
(AFT).
The study showed that the apatite from Archean rocks was largely formed at 1.8–1.9 Ga as a result of a Paleoproterozoic metamorphic
overprinting during the terrane collision and the subsequent accretion of the Siberian craton. The last thermal event, the
self-heating of the collision prism, was terminated by cooling at ∼1.3 Ga. At that time, the Rb-Sr isotopic system became
closed and the upper crust passed the ~300°C isograd. The calculation results showed that on further cooling, the ∼100°C isograd
was passed at 1143 Ma. This age estimate could be obtained using AFT dating if the above event had been the last one in the
thermal history of the Siberian craton. The obtained track ages indicate the existence of a repeated, significantly younger,
heating of the crystalline crust due to some local reason. 相似文献
88.
刘顺生 GLASMACHER Ulrich 许志琴 WEBER Ursul WAGNER Günther JONCKHEERE Raymon 殷秀兰 《岩石学报》2009,25(7):1612-1618
本文包括中国大陆科学钻(CCSD)主孔(MH)0~5000m和先导孔(PP2)0~1000m的磷灰石裂变径迹分折结果,先导孔PP2的裂变径迹表观年龄变化范围为79.5±5.1~50.4±6.2Ma,主孔的裂变径迹表观年龄变化范围为98.6±17.0~2.9±2.0Ma,主孔在4200m以下,磷灰石样品中实际上已不存在自发裂变径迹,表明裂变径迹时钟已经“置零”。实验资料表明,裂变径迹表观年龄值随样品深度的增加而逐渐减少,直到一定深度,即达到磷灰石的裂变径迹封闭温度(~120℃)以后,年龄值为零。根据主孔0~2000m和先导孔0~1000m的裂变径迹年龄剖面,作为一级近似,计算出超高压变质岩体在90~30Ma期间,平均隆升速度为~35m/Ma。对主孔测定了9个样品的约束径迹(Confined track)长度,样品约束径迹平均长度的变化范围约为13.1~7.4μm,总的变化趋势是:约束径迹平均长度随样品深度的增加而逐渐减少。样品的约束径迹长度分布都具有双峰型特征。根据裂变径迹年龄和约束径迹长度的资料,应用计算机模拟得到了样品的时间-温度(t-T)轨迹。结果表明,岩体从早白垩世(~120Ma)快速冷却以后,在晚白垩世和始新世又经历了两次加热作用,始新世末岩体所达到的温度大约是80℃,随后岩体则一直上升和缓慢冷却到现今所处的位置。在最后~30Ma岩体的平均隆升速度为~53m/Ma。 相似文献
89.
Anthony Moraghan Michael D. Smith Alexander Rosen 《Monthly notices of the Royal Astronomical Society》2008,386(4):2091-2100
The properties of bipolar outflows depend on the structure in the environment as well as the nature of the jet. To help distinguish between the two, we investigate here the properties pertaining to the ambient medium. We execute axisymmetric hydrodynamic simulations, injecting continuous atomic jets into molecular media with density gradients (protostellar cores) and density discontinuities (thick swept-up sheets). We determine the distribution of outflowing mass with radial velocity (the mass spectrum) to quantify our approach and to compare to observationally determined values. We uncover a sequence from clump entrainment in the flanks to bow shock sweeping as the density profile steepens. We also find that the dense, highly supersonic outflows remain collimated but can become turbulent after passing through a shell. The mass spectra vary substantially in time, especially at radial speeds exceeding 15 km s−1 . The mass spectra also vary according to the conditions: both envelope-type density distributions and the passage through dense sheets generate considerably steeper mass spectra than a uniform medium. The simulations suggest that observed outflows penetrate highly non-uniform media. 相似文献
90.
Jonathan LEVINE Andrés ARAZI Thomas FAESTERMANN Jorge O. FERNáNDEZ NIELLO Gunther KORSCHINEK Ana María LA GAMMA Agustín NEGRI Georg RUGEL Peter STEIER Anton WALLNER 《Meteoritics & planetary science》2008,43(4):805-813
Abstract— We have measured a surprisingly long terrestrial age of 410,000 ±45,0020,000 yr (410 ±2045ka) for basaltic eucrite Río Cuarto 001 using accelerator mass spectrometry of 26Al, 36Cl, and 41Ca. Though many meteorites are known to have survived for tens or hundreds of ka in Antarctica or hot deserts, the mean annual precipitation of 815 mm in Río Cuarto, Cordoba Province, Argentina, makes the long survival of this meteorite remarkable. We propose two explanations for the exceptional preservation of Río Cuarto 001. First, the meteorite contains only trace amounts of metal, so the weathering and oxidation of metallic Fe, which commonly destroys chondrites, is ineffective in this case. Second, the meteorite was found in a relatively young deflation basin, and may have been exhumed only recently from beneath a protective layer of soil. Insofar as the survival on Earth of Río Cuarto 001 is due to environmental factors, there may be other meteorites with comparably long terrestrial ages still to be discovered in the vicinity. 相似文献