Non-axisymmetric relativistic Bondi–Hoyle accretion on to a Schwarzschild black hole

We present the results of an exhaustive numerical study of fully relativistic non-axisymmetric Bondi–Hoyle accretion on to a moving Schwarzschild black hole. We have solved the equations of general relativistic hydrodynamics with a high-resolution shock-capturing numerical scheme based on a linearized Riemann solver. The numerical code was previously used to study axisymmetric flow configurations past a Schwarzschild black hole. We have analysed and discussed the flow morphology for a sample of asymptotically high Mach number models. The results of this work reveal that initially asymptotic uniform flows always accrete on to the hole in a stationary way, which closely resembles the previous axisymmetric patterns. This is in contrast with some Newtonian numerical studies where violent flip-flop instabilities were found. As discussed in the text, the reason can be found in the initial conditions used in the relativistic regime, as they cannot exactly duplicate the previous Newtonian setups where the instability appeared. The dependence of the final solution on the inner boundary condition as well as on the grid resolution has also been studied. Finally, we have computed the accretion rates of mass and linear and angular momentum.     

Resonant tidal disruption in galactic nuclei

It has recently been shown by Rauch 38 Tremaine that the rate of angular momentum relaxation in nearly Keplerian star clusters is greatly increased by a process termed 'resonant relaxation'; it was also argued, via a series of scaling arguments, that tidal disruption of stars in galactic nuclei containing massive black holes could be noticeably enhanced by this process. We describe here the results of numerical simulations of resonant tidal disruption which quantitatively test the predictions made by Rauch 38 Tremaine. The simulation method is based on an N -body routine incorporating cloning of stars near the loss cone and a semirelativistic symplectic integration scheme. Normalized disruption rates for resonant and non-resonant nuclei are derived at orbital energies both above and below the critical energy, and the corresponding angular momentum distribution functions are found. The black hole mass above which resonant tidal disruption is quenched by relativistic precession is determined. We also briefly describe the discovery of chaos in the Wisdom–Holman symplectic integrator applied to highly eccentric orbits and propose a modified integration scheme that remains robust under these conditions. We find that resonant disruption rates exceed their non-resonant counterparts by an amount consistent with the predictions; in particular, we estimate the net tidal disruption rate for a fully resonant cluster to be about twice that of its non-resonant counterpart. No significant enhancement in rates is observed outside the critical radius. Relativistic quenching of the effect is found to occur for hole masses M  >  M _Q  = (8 ± 3) × 10⁷  M . The numerical results combined with the observed properties of galactic nuclei indicate that for most galaxies the resonant enhancement to tidal disruption rates will be very small.     

The numerical simulation on the PBL structure and its evolution over small-scale concave terrain

A high-resolution, nonhydrostatic, three-dimensional diagnostic PBL model over small-scale concave terrain was established in this paper. A two-dimensional prognostic model was developed based on the diagnostic model. The hydrostatic approximation was abandoned and the simple energy (E-ε) closure scheme was used in both mod-els. Using the two models, characteristics of PBL structure and its evolution were fully studied. The main characteris-tic of the PBL is the circulation, and it fairly affects the distribution of the pollutant in the pit.     

对流云团资料在局地暴雨数值模拟预报中的应用

使用ＰＳＵ／ＮＣＡＲ中尺度数值模式,对两次暴雨实例进行了数值模拟试验。结果表明：相对应用地面及高空常规资料作为初始场的控制试验而言,就用实时卫星对流云团资料增强局部湿度场的敏感性试验,可使暴雨及邻近地区对流层中低层气流辐合上升运动增强,     

绿洲与荒漠相互影响下大气边界层特征的模拟

用发展的二维中尺度土壤－植被－大气连续体数值模式模拟了绿洲与荒漠相互影响下的大气边界层特征。得到了绿洲和临近荒漠之间的边界层高度、风螺线、风速廓线、位温廓线和比湿廓线的差别,并给出了绿洲对其上游和下游荒漠大气的不同影响。基本再现了白天绿洲大气逆温和临近绿洲的荒漠大气逆湿。模拟实验研究不仅验证了外场观测结果,而且也使我们对复杂下垫面边界层结构有了一些新的认识。     

SIMULATION OF MONTHLY CLIMATIC MEAN FIELD IN JANUARY AND JULY IN QINGHAI-XIZANG PLATEAU AND NORTHWESTERN CHINA

In this paper,we simulate the regional climate in summer and winter in northwestern part ofChina and the Qinghai-Xizang Plateau with regional climate model(MM4)nested with GFDLdata,and compare the simulated results with observed data and GFDL data.The results show thatthe regional model reproduces the regional climate systems,such as the high pressure on theplateau and the low pressure in the north of the plateau in winter,the warm-low pressure over theplateau and pressure ridge in south and north of the Qinghai-Xizang Plateau in summer.Theseregional climate features could not be distinguished by the GCM.The simulations of precipitationdistribution are reasonable.But differences between the simulated and observed precipitationvalues in some places are obvious.The precipitation in south of the Qinghai-Xizang Plateau isunderestimated,and in north of the Qinghai-Xizang Plateau,the precipitation is overestimated.The simulation of height field is better than temperature field.     

NUMERICAL STUDY ON THE EFFECTS OF SEA SURFACE TEMPERATURE ON TROPICAL CYCLONE INTENSITY-PART I:NUMERICAL EXPERIMENT OF THE TROPICAL CYCLONE INTENSITY RELATED TO SST Duan Yihong;Qin Zenghao;Gu dianfeng;Li Yongping, Shanghai Typhoon Institute.Shangh

In the context of a model of tropical cyclone intensity based on an improved meso-scaleatmospheric model, numerical simulation is performed of the track and intensity variation oftropical cyclones (TC) arising from sea surface temperature (SST) variation over a specified searegion. Evidence suggests that the model is capable of modeling quite welt the track and intensityof TC: SST variation leads to an abrupt change in the cyclone intensity: the response of thecyclone to the abrupt SST change lasts 8—12 h.     

黄河三角洲短期暴雨预报系统

在天气学分析的基础上,利用１９９０～１９９５年日本数值预报产品与实时资料相结合,研制黄河三角洲短期暴雨预报系统,经１９９６年使用效果较好。     

NUMERICAL EXPERIMENT OF MEDIUM-RANGE CHANGE OF THE SUBTROPICAL HIGH Ⅰ. THE INFLUENCE OF THE HEATING SOURCE OVER TIBET PLATEAU

The medium-range change of the subtropical high of June 1979 and its influences of the heating sources over Tibet Plateau are studied by using a global circulation spectrum-model. The analyses of the simulation results show that the heating sources over Tibet Plateau play an important role in the process of frontogenesis. the intensity of frontal zone and the upper-tropospheric westerly jet associated with it. When there are heating sources over Tibet Plateau. both the frontal zone and westerly jet are stronger. There are very important mutual relations between the sensible heating and latent heating. After the sensible heating and latent heating are isolated.it departs much from reality that the significance of them are studied