Variable temperature and moisture conditions in Yungang Grottoes,China, and their impacts on ancient sculptures     

Xu-Sheng Wang  Li Wan  Jizhong Huang  Wenbing Cao  Fei Xu  Pei Dong 《Environmental Earth Sciences》2014,72(8):3079-3088

Deterioration of grottoes induced by the negative impacts of the variable temperature and moisture conditions has been an important issue in the conservation of heritage sites in China. In this case study, the spatial distributions and varying patterns of moisture and temperature in the caves of Yungang Grottoes, China, were investigated. The relative air humidity was approximately 100 % in the deep zone of the unsaturated surrounding rocks of the grottoes where the temperature remained almost steady at around 9.4 °C. However, the indoor air temperature, relative humidity, and rock surface temperature in the caves varied significantly because of the active exchange of the air with the outside atmosphere. The condensation water appeared on cave walls in the summer when the dew point in the air was higher than the rock surface temperature. Preliminary assessments with a special collection device indicated that the thickness of the transient condensation water could reach 0.03–0.10 mm on the back wall of a cave. The occurrence of this condensation water is expected to worsen salt deterioration of the sculptures in the grottoes. As revealed by long-term observations, a wooden building in front of a cave can weaken the indoor air temperature fluctuation and reduce the condensation water, and consequently, prevent the negative effects of the microclimate for the sculptures.  相似文献   

Stochastic Fracture Propagation Modelling for Enhanced Geothermal Systems     

Chaoshui Xu  Peter A. Dowd 《Mathematical Geosciences》2014,46(6):665-690

Fractures and fracture networks are the fundamental components of enhanced geothermal systems and determine their technical and economic viability. A realistic fracture model that can adequately describe a fracture-stimulated reservoir is critical for subsequent flow and heat transfer analyses of the system. Fractures in these systems are essentially the product of hydraulic stimulations of the reservoir that, together with ground conditions and the local stress regime, determine how fractures are formed and propagated. This paper describes three methods for generating realistic fracture models for enhanced geothermal systems; two of them incorporate the fracture propagation process in the modelling and hence provide a stochastic fracture propagation model. The methods are: a Bayesian framework in the form of Markov Chain Monte Carlo simulation, an extended Random Sampling Consensus model and a Point and Surface Association Consensus model. The conditioning data used in these methods are seismic events recorded during fracture stimulation. Geodynamics’ Habanero reservoir in the Cooper Basin of South Australia is used as a case study to test these methods.  相似文献   

Re-Identification of the ＇Enigmatic＇ X-ray Source 1RXS J114003.0＋124112     

Jiang-Hua Wu Tigran Movsessian Yang Chen Xiang-Tao He Xu Zhou Jun Ma 《中国天文和天体物理学报》2006,6(4):430-434

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A numerical model for Type II supernovae — The collapse stage     

Cong Xu  Zong-wei Li  Yun-zao Ge 《Chinese Astronomy and Astrophysics》1985,9(2):154-158

We use the following numerical model for the collapse stage of a Type II supernova of 15 M_⊙. Our electron capture rate includes the effects of the inverse reaction and the neutron-proton mass difference. This decreases the electron density at the collapse stage and led to rather large values of the maximum inward velocity and of the corresponding mass (Umax = 3.06 × 10⁹cm/s, Mmax=0.76 M_⊙). These larger values are more favourable for the propagation of shock after the rebounce and the triggering-off of a Type-II supernova explosion. For neutrino transport, we use a leakage model and an equilibrium diffusion model, respectively, for the thin and thick stages and a grey atmosphere model to assess the effect of neutrino precipitation on the collapse. We found this effect to be small, the energy precipitation to be not more than 10^?5 the neutrino energy loss and the momentum precipitation not more than 10^?6 the gravitational acceleration.  相似文献   

COSTAS环解调器设计及实践初探     

胡玉林  徐建军 《成都信息工程学院学报》1990,(1)

本文详细介绍自行设计的COSTAS环解调器的工作原理,环路参数选择以及实际工作效果。  相似文献   

利用自回归模型检测地球极移重力效应     

杨学峰  孙和平  徐建桥 《大地测量与地球动力学》2004,24(2):110-114

同时采用4个台站的国际超导重力仪长期连续重力观测资料和国际地球自转服务中心提供的同步地球自转参数，研究了极移引起的地球重力场变化特征。利用自回归模型估计了各序列的功率谱密度和积谱密度，结果表明极移导致的重力效应的主要能量集中在Chandler摆动和周年项附近，叠积后实际重力观测与极移重力信号理论值之间的差异分别为0．4％和3．9％，说明超导重力仪可有效监测极移导致的重力变化。  相似文献   

Transition probabilities and lifetimes in singly ionized rhenium     

P. Palmeri  P. Quinet  É. Biémont  H. L. Xu  S. Svanberg 《Monthly notices of the Royal Astronomical Society》2005,362(4):1348-1352

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Multi-wavelength Diagnostics of Bombardment by Non-thermal Particles in Solar Flares     

Zhi Xu  Cheng Fang  Wei-Qun Can Astronomy Department of Nanjing University  Nanjing  Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing 《中国天文和天体物理学报》2005,5(5):519-530

Chromospheric lines, including Ha, Lyα, Lyβand CaⅡK, CaⅡ8542, are systemically and quantitatively investigated with respect to the non-thermal excitation and ionization due to particle beam bombardment for a series of solar semi-empirical atmospheric models. As a result we propose to use the contrast in the integrated intensity of hydrogen lines to estimate the total energy flux of the bombarding beam during the solar flare impulsive phase. Partial frequency redistribution is considered in the Lyαline calculation and a smaller intensity enhancement in the Ha line-centers is found than in the previous results of Fang et al.  相似文献   

Adjoint Assimilation in Marine and an Example of Application   总被引：1，自引：1，他引：0  

XU Qing  LIU Yuguang  and LU Xianqing Physical Oceanography Laboratory  Ocean University of China  Qingdao  P.R.China 《中国海洋大学学报(英文版)》2005,4(1):14-20

This paper aims at a review of the work carried out to date on the adjoint assimilation of data in marine ecosystem models since 1995. The structure and feature of the adjoint assimilation in marine ecosystem models are also introduced. To illustrate the application of the adjoint technique and its merits, a 4-variable ecosystem model coupled with a 3-D physical model is established for the Bohai Sea and the Yellow Sea. The chlorophyll concentration data derived from the SeaWiFS ocean colour data are assimilated in the model with the technique. Some results are briefly presented.  相似文献   

Can the inner gap sparking take place in millisecond pulsars？     

Hong-Guang Wang  Guo-Jun Qiao  Ren-Xin XuDepartment of Astronomy  Peking University  Beijing   《中国天文和天体物理学报》2003,3(5):443-452

The inner vacuum gap model has become the foundation stone of most theories on pulsar radio emission. The fundamental picture of this model is the sparking, which was conjectured to be induced by magnetic absorption of background gamma photons. However, a question is, can the sparking be triggered in the millisecond pulsars (MSPs) with magnetic fields (B) only about 108 G? We investigate this problem by including the pair production above the inner gap. Under the assumption that the magnetic field is dipolar, our results show the background gamma-ray emission can not be the key factor that triggers the sparking, at least not in MSPs with B - 108 G, if the temperature in the polar cap region is only so high as is observed (< 4 × 106 K). Some other mechanisms are required.  相似文献