川滇地震科学实验场地震目录最小完整性震级分析          下载免费PDF全文

史翔宇  王晓青  邱玉荣  袁小祥 《地球物理学报》1954,63(10):3683-3697

地震目录是地震监测预报、地震活动性等研究的重要资料.川滇地震科学实验场地区近几十年来积累了大量的地震记录,为实验场的地震科学研究提供了宝贵的数据.地震台网密度和仪器观测精度是逐步提高的,不同时期地震目录的完整性存在差异,因此进行现代仪器观测记录的地震目录最小完整性震级（M_C,Magnitude of Completeness）分析,对正确研究和认识该地区地震活动规律及其影响因素等具有重要意义.本文采用震级—序号方法、最大曲率法（MAXC,Maximum Curvature）和拟合度检测法（GFT,Goodness-of-Fit Test）分析了川滇地震科学实验场地区1970—2018年地震目录的最小完整性震级M_C值,得到了实验场地区及其内部各地震区（带）M_C值的时间演化特征和空间分布特征.结果表明,实验场地区及其内部各地震区（带）M_C值变化趋势大致为1970—1986年M_L2.0~2.6,1987—1999年M_L2.5~2.6,2000—2008年后M_L1.4~2.1,2009—2018年M_L1.2~1.9;实验场地区M_C值的空间分布大致呈现东北部和西南部较低、西北部和东南部较高的特征,其中云南最南端的澜沧—耿马区和思普区、四川西北部的理塘—木里区以及川藏交界处的金沙江带M_C值普遍较高,云南北部和四川南部的松潘—龙门山带、安宁河带、元谋区、楚雄—建水带和大理—丽江—盐源区M_C值普遍较低;强震会使M_C值出现突然升高、之后逐渐恢复的现象,其中M_C值升高程度与震级有一定相关性,并且强震导致的M_C值升高是M_C值空间和时间分布不均匀的原因之一.  相似文献   

Modelling of diffusion boundary-layers in subtidal macroalgal canopies: The response to waves and currents     

Craig L. Stevens  Catriona L. Hurd  Pål E. Isachsen 《Aquatic Sciences - Research Across Boundaries》2003,65(1):81-91

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The hydrogen emission spectrum of a shock wave in a stellar atmosphere     

Yu. A. Fadeyev 《Astronomy Letters》2003,29(11):775-782

Based on a self-consistent solution of the equations of gas dynamics, kinetics of hydrogen atomic level populations, and radiative transfer, we analyze the structure of a shock wave that propagates in a partially ionized hydrogen gas. We consider the radiative transfer at the frequencies of spectral lines by taking into account the effects of a moving medium in the observer's frame of reference. The flux in Balmer lines is shown to be formed behind the shock discontinuity at the initial hydrogen recombination stage. The Doppler shift of the emission-line profile is approximately one and a half times smaller than the gas flow velocity in the Balmer emission region, because the radiation field of the shock wave is anisotropic. At Mach numbers M₁?10 and unperturbed gas densities σ₁=10^?10 g cm^?3, the Doppler shift is approximately one third of the shock velocity U₁. The FWHM of the emission-line profile δ _? is related to the shock velocity by δ _? ≈ k _? U₁, where k _? = 1, 0.6, and 0.65 for the Hα, Hβ, and Hγ lines, respectively.  相似文献   

Pore scale modeling of immiscible and miscible fluid flows using smoothed particle hydrodynamics     

Alexandre M. Tartakovsky  Paul Meakin 《Advances in water resources》2006

A numerical model based on smoothed particle hydrodynamics (SPH) was developed and used to simulate immiscible and miscible fluid flows in porous media and to study effects of pore scale heterogeneity and anisotropy on such flows.  相似文献   

Ecosystem engineering: the impact of bioturbation on biogeochemical processes in marine and freshwater benthic habitats   总被引：1，自引：0，他引：1  

Florian Mermillod-Blondin  Rutger Rosenberg 《Aquatic Sciences - Research Across Boundaries》2006,68(4):434-442

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人工合成烃类包裹体的实验研究   总被引：6，自引：3，他引：6  

倪培  王一刚 《岩石学报》2007,23(9):2033-2038

运用 Sterner 和 Bodnar(1984)提出的愈合裂隙的实验技术,在石英中成功地合成了烃类包裹体,并对合成的包裹体进行了岩相学观察、显微温度测定及激光拉曼光谱分析等。实验揭示出除合成压力之外,合成温度、反应时间和油水比例是烃类包裹体合成时几个需要重点考虑的因素。此外,合成时加入的初始溶液盐度和酸碱度也值得进一步考虑。人工合成烃类包裹体为研究天然烃类包裹体的形成机制及测定分析奠定了基础。  相似文献   

Experimental study on the effects of artificial bed roughness on turbidity currents over abrupt bed slope change     

《国际泥沙研究》2020,35(3):256-268

A series of experimental observations are presented in the current study to discuss the effects of artificial bed roughness on the turbidity current flowing in a rectangular channel with an abrupt change in bed slope.For this purpose,two different types of elements,sinusoidal and trapezoidal,with various heights and arrangements are considered as artificial bed roughness.A Vectrino velocity meter was used to measure the velocity and sediment concentration profiles.The effects of inlet sediment concentration on front velocity,body velocity,unit discharge,sediment concentration,and suspended load transport rate also were investigated.Accurate equations were developed for estimation of the velocity of a turbidity current over smooth and rough beds.The unexpected experimental results showed that unlike the effect of roughness height,a change in the roughness arrangement has no significant influence on the velocity of a turbidity current.Also,the effect of bed roughness on the front velocity of a denser current is more significant.  相似文献   

Stream overflow and dwarf nova eruptions     

M. R. Schreiber  & F. V. Hessman 《Monthly notices of the Royal Astronomical Society》1998,301(3):626-630

We consider the effects of accretion stream overflow on the viscous dynamics of accretion discs in dwarf novae. If the stream from the secondary star is geometrically thick enough, some fraction of its material can flow over and under the disc. The mass and specific angular momentum of the stream are then deposited not only at the point of collision with the outer disc, but also at those radii in the inner disc with geometric heights that are large enough to intercept the residual stream, or near the radius where the disc has the same specific angular momentum as the stream. The overflowing stream can alter the behaviour of heating fronts and cooling fronts in the disc. If the mass fraction of the overflowing stream is of order tens of per cent, the deposition of mass in the inner parts of the disc is sufficient to change the character of the eruption light curves significantly.  相似文献   

Numerical simulations of protostellar encounters — II. Coplanar disc–disc encounters     

S. J. Watkins  A. S. Bhattal  H. M. J. Boffin  N. Francis  & A. P. Whitworth 《Monthly notices of the Royal Astronomical Society》1998,300(4):1205-1213

It is expected that an average protostar will undergo at least one impulsive interaction with a neighbouring protostar whilst a large fraction of its mass is still in a massive, extended disc. Such interactions must have a significant impact upon the evolution of the protostars and their discs.   We have carried out a series of simulations of coplanar encounters between two stars, each possessing a massive circumstellar disc, using an SPH code that models gravitational, hydrodynamic and viscous forces. We find that during a coplanar encounter, disc material is swept up into a shock layer between the two interacting stars, and the layer then fragments to produce new protostellar condensations. The truncated remains of the discs may subsequently fragment; and the outer regions of the discs may be thrown off to form circumbinary disc-like structures around the stars. Thus coplanar disc–disc encounters lead efficiently to the formation of multiple star systems and small- N clusters, including substellar objects.  相似文献   

Magma fragmentation dynamics: experiments with analogue porous low-strength material     

Mikhail Alidibirov  Vsevolod Panov 《Bulletin of Volcanology》1998,59(7):481-489

 Experiments were conducted on the fragmentation of analogue low-strength porous material (plastiprin) by rapid decompression in a shock-tube-type apparatus. The porous samples (length=365 mm, cross-section dimensions 40×40 mm) pressurized by air to pressures up to 0.9 MPa, were rapidly decompressed to 0.1 MPa. Rapid decompression of samples caused fragmentation and ejection of the fragmentation products into a large volume tank. The process of analogue material fragmentation was documented using high-speed cinematography and dynamic pressure measurements. The duration of the fragmentation event is significantly shorter than that of the ejection event. The fragmentation of material precedes the acceleration of fragments. As a result of fragmentation, sub-parallel fractures are generated. The characteristic fragment size decreases as the initial pressure differential increases. The ejected fragments obtain velocities of 60 m/s. The mechanisms of material fragmentation during unloading and fragmentation wave propagation are discussed. The experimental results provide insight into the fragmentation dynamics of highly viscous magmas in which brittle failure at high strain rate is possible. Received: 23 July 1997 / Accepted: 23 November 1997  相似文献