五大连池近代火山老黑山火烧山火山喷发过程的考察研究   总被引：4，自引：0，他引：4  

任锦章  白志达 《东北地震研究》1998,14(1):76-83

作者在已有工作的基础上,以当代火山学的研究思路和观点,为恢复五大连池两个近代火山,老黑山火烧山的喷发历史过程进行了野外考察研究工作。老黑山火山锥是由三套不同的碎屑堆积物组成。在锥体的南侧、东侧和西侧以及北测和北西侧有５个熔岩溢出口,按它们形成先后关系,认为有早、中、晚三期熔岩流。本文还对老黑山火山锥上的寄生火山、结壳熔岩与渣状熔岩的分布、流动特点及形成的控制因素进行了分析讨论。最后得出结论：老黑山火山是经多期次喷发活动形成的。火烧山火山锥是一碎屑化泡沫化程度很低的浮岩块和熔岩碎块组成,同老黑山有明显区别。  相似文献   

The impact of cooling flows on the T_X–L_Bol relation for the most luminous clusters     

S. W. Allen  & A. C. Fabian 《Monthly notices of the Royal Astronomical Society》1998,297(3):L57-L62

We examine the effects of cooling flows on the T _X– L _Bol relation for a sample of the most X-ray luminous ( L _Bol > 10⁴⁵ erg s⁻¹) clusters of galaxies known. Using high-quality ASCA X-ray spectra and ROSAT images we explicitly account for the effects of cooling flows on the X-ray properties of the clusters and show that this reduces the previously noted dispersion in the T _X– L _Bol relationship. More importantly, the slope of the relationship is flattened from L _Bol ∝  T ³_X to approximately L _Bol ∝  T ²_X, in agreement with recent theoretical models which include the effects of shocks and pre-heating on the X-ray gas. We find no evidence for evolution in the T _X– L _Bol relation within z  ∼ 0.3. Our results demonstrate that the effects of cooling flows must be accounted for before cosmological parameters can be determined from X-ray observations of clusters. The results presented here should provide a reliable basis for modelling the T _X– L _Bol relation at high X-ray luminosities.  相似文献   

The relationship between cooling flows and metallicity measurements for X-ray-luminous clusters     

S. W. Allen  & A. C. Fabian 《Monthly notices of the Royal Astronomical Society》1998,297(3):L63-L68

We explore the relationship between the metallicity of the intracluster gas in clusters of galaxies, determined by X-ray spectroscopy, and the presence of cooling flows. Using ASCA spectra and ROSAT images, we demonstrate a clear segregation between the metallicities of clusters with and without cooling flows. On average, cooling-flow clusters have an emission-weighted metallicity a factor ∼ 1.8 times higher than that of non-cooling-flow systems. We suggest that this is caused by the presence of metallicity gradients in the cooling-flow clusters, coupled with the sharply peaked X-ray surface brightness profiles of these systems. Non-cooling-flow clusters have much flatter X-ray surface brightness distributions and are thought to have undergone recent merger events, which may have mixed the central high-metallicity gas with the surrounding less metal-rich material. We find no evidence for evolution in the emission-weighted metallicities of clusters within z  ∼ 0.3.  相似文献   

Role of barotropic,baroclinic and combined barotropic-baroclinic instability for the growth of monsoon depressions and mid-tropospheric cyclones     

B. N. Goswami  R. N. Keshavamurty  V. Satyan 《Journal of Earth System Science》1980,89(1):79-97

A detailed barotropic, baroclinic and combined barotropic-baroclinic stability analysis has been carried out with mean monsoon zonal currents over western India, eastern India and S.E. Asia. The lower and middle tropospheric zonal wind profiles over western India are barotropically unstable. The structure and growth rate of these modes agree well with the observed features of the midtropospheric cyclones. Similar profiles over eastern India and S.E. Asia, however, are barotropically stable. This is attributed to weak horizontal shear, inherent to these profiles. The upper tropospheric profiles, on the other hand, are barotropically unstable throughout the whole region. The features of these unstable modes agree with those of observed easterly waves. The baroclinic and combined barotropic-baroclinic stability analyses show that the baroclinic effects are not important in tropics. Though the barotropic instability of the mean zonal current seems to be res ponsible for the initial growth of the mid-tropospheric cyclones, neither barotropic nor baroclinic instability of the mean zonal current seem to explain the observed features of the monsoon depressions.  相似文献   

Lagrangian meshfree particles method (SPH) for large deformation and failure flows of geomaterial using elastic–plastic soil constitutive model     

Ha H. Bui  Ryoichi Fukagawa  Kazunari Sako  Shintaro Ohno 《国际地质力学数值与分析法杂志》2008,32(12):1537-1570

Simulation of large deformation and post‐failure of geomaterial in the framework of smoothed particle hydrodynamics (SPH) are presented in this study. The Drucker–Prager model with associated and non‐associated plastic flow rules is implemented into the SPH code to describe elastic–plastic soil behavior. In contrast to previous work on SPH for solids, where the hydrostatic pressure is often estimated from density by an equation of state, this study proposes to calculate the hydrostatic pressure of soil directly from constitutive models. Results obtained in this paper show that the original SPH method, which has been successfully applied to a vast range of problems, is unable to directly solve elastic–plastic flows of soil because of the so‐called SPH tensile instability. This numerical instability may result in unrealistic fracture and particles clustering in SPH simulation. For non‐cohesive soil, the instability is not serious and can be completely removed by using a tension cracking treatment from soil constitutive model and thereby give realistic soil behavior. However, the serious tensile instability that is found in SPH application for cohesive soil requires a special treatment to overcome this problem. In this paper, an artificial stress method is applied to remove the SPH numerical instability in cohesive soil. A number of numerical tests are carried out to check the capability of SPH in the current application. Numerical results are then compared with experimental and finite element method solutions. The good agreement obtained from these comparisons suggests that SPH can be extended to general geotechnical problems. Copyright © 2008 John Wiley & Sons, Ltd.  相似文献   

Two-dimensional,two-phase granular sediment transport model with applications to scouring downstream of an apron     

L.O. Amoudry  P.L.-F. Liu 《Coastal Engineering》2009

We present a two-dimensional, two-phase model for non-cohesive sediment transport. This model solves concentration-weighted averaged equations of motion for both fluid and sediment phases. The model accounts for the interphase momentum transfer by considering drag forces. A collisional theory is used to compute the sediment stresses, while a two-equation (k–ε) fluid turbulence closure is implemented. A benchmark sediment transport problem concerning the scouring downstream of an apron is carried out as an example and numerical results agree with existing experimental data.  相似文献   

基于多元要素流的珠三角城市群功能联系与空间格局分析   总被引：1，自引：0，他引：1  

林勋媛  胡月明  王广兴  樊舒迪 《世界地理研究》2020,29(3):536-548

以珠三角城市群9个地级市为研究对象，结合当前热点网络开放大数据，对珠三角城市群内各城市的经济流、交通流、人口流和信息流的联系强度和作用方向进行测算与评价。借助赋值法分别对四种要素流的总量进行打分，以各城市的综合得分作为空间层级划分依据，提出关于“点—线—面”的空间互动格局，进而探索珠三角城市群未来的发展规划。研究结果表明：①从各要素流的联系强度上看，城市间的等级划分具有较高的重合度，说明四种要素流彼此之间相互联系、相互作用。从各要素流的作用方向上看，广州和深圳多作为区域内其它城市的首位空间联系城市，说明各要素流通常指向经济发展水平较高、通达性较好的城市。②从整体来看，珠三角城市群内部功能互动表现极度不平衡，一是中心城市占据了要素流强度的绝大部分，其余城市仅占据极小部分流量，两极分化严重；二是东西两岸发展不平衡，东岸发展水平明显要强于西岸发展水平。③广州、深圳、东莞和佛山等城市虽然在区域内起到了一定的辐射和带动作用，但是针对江门、肇庆等周边城市的辐射和带动强度仍有待提升,说明还需进一步优化珠三角城市群功能分工与产业布局，推进区域经济一体化。  相似文献   

Stellar and HI Mass Functions Predicted by a Simple Preheating Galaxy Formation Model     

Zhi-Jian Luo Cheng-Gang Shu 《中国天文和天体物理学报》2007,7(4):590-594

According to the new preheating mechanism of galaxy formation suggested by Mo et al., we construct a simple model of formation of disk galaxies within the current paradigm of galaxy formation. It incorporates preheating, gas cooling, bulge formation and star for-mation. The predicted stellar and HI mass functions of galaxies are discussed and compared with the observations. It is found that our model can roughly match both the observed galaxy luminosity function and the observed HI-mass function.  相似文献   

Comparison of Large-Scale Flows on the Sun Measured by Time-Distance Helioseismology and Local Correlation Tracking     

Michal Švanda  Junwei Zhao  Alexander G. Kosovichev 《Solar physics》2007,241(1):27-37

We present a direct comparison between two different techniques: time-distance helioseismology and a local correlation tracking method for measuring mass flows in the solar photosphere and in a near-surface layer. We applied both methods to the same dataset (MDI high-cadence Dopplergrams covering almost the entire Carrington rotation 1974) and compared the results. We found that, after necessary corrections, the vector flow fields obtained by these techniques are very similar. The median difference between directions of corresponding vectors is 24°, and the correlation coefficients of the results for mean zonal and meridional flows are 0.98 and 0.88, respectively. The largest discrepancies are found in areas of small velocities where the inaccuracies of the computed vectors play a significant role. The good agreement of these two methods increases confidence in the reliability of large-scale synoptic maps obtained by them.  相似文献   

Ionized nebulae surrounding brightest cluster galaxies     

N. A. Hatch  C. S. Crawford  A. C. Fabian 《Monthly notices of the Royal Astronomical Society》2007,380(1):33-43

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