文化旅游吸引物表征符号理论体系的探讨   总被引：1，自引：0，他引：1  

丁雨莲  赵媛 《云南地理环境研究》2011,23(5):13-17

通过文献总结法,理论探讨文化旅游吸引物表征符号系统。根据文化结构的三层次说,建立文化旅游吸引物表征符号结构与表征符号内容:历史文化表征符号、现代文化表征符号、民俗文化表征符号、伦理道德文化表征符号。认为制度文化表征系统与精神文化表征系统可视为"舞台"的"帷幕",引导游客由"前台"向"后台"探索,从而避免对目的地文化认识的肤浅化和片面化。对符号意义和价值的编码存在着一种社会选择机制,需根据主流价值观进行社会建构,以符合社会心理取向和游客兴趣。  相似文献   

黑龙江省“九五”与“十五”测震台网理论最小监测能力的对比   总被引：1，自引：1，他引：0  

吴宝峰  闫峰 《地震地磁观测与研究》2008,29(3):51-53

对黑龙江省地震局“九五”和“十五”地震台网的理论最小监测能力进行计算和对比,为地震台网的布局提出了一些合理化的建议,为以后的地震台网建设提供了很好的参考。  相似文献   

A fragmentation criterion for highly viscous bubbly magmas estimated from shock tube experiments     

Takehiro Koyaguchi  Bettina Scheu  Noriko K. Mitani  Oleg Melnik 《Journal of Volcanology and Geothermal Research》2008

When a highly viscous bubbly magma is sufficiently decompressed, layer-by-layer fracturing propagates through the magma at a certain speed (fragmentation speed). On the basis of a recent shock tube theory by Koyaguchi and Mitani [Koyaguchi, T., Mitani, N. K., 2005. A theoretical model for fragmentation of viscous bubbly magmas in shock tubes. Journal of Geophysical Research 110 (B10), B10202. doi:10.1029/2004JB003513.], gas overpressures at the fragmentation surface are estimated from experimental data on fragmentation speed in shock tube experiments for natural volcanic rocks with various porosities. The results show that gas overpressure at the fragmentation surface increases as initial sample pressure increases and sample porosity decreases. We propose a new fragmentation criterion to explain the relationship between the gas overpressure at the fragmentation surface, the initial pressure and the porosity. Our criterion is based on the idea that total fragmentation of highly viscous bubbly magmas occurs when the tensile stress at the midpoint between bubbles exceeds a critical value. We obtain satisfactory agreement between our simulation and experiment when we assume that the critical value is inversely proportional to the square root of bubble wall thickness. This fragmentation criterion suggests that long micro-cracks or equivalent flaws (e.g., irregular-shaped bubbles) that reach the midpoints between bubbles are a dominant factor to determine the bulk strength of the bubbly magma.  相似文献   

双层散体材料桩复合地基固结理论   总被引：1，自引：0，他引：1  

孙举  谢新宇  谢康和 《岩土力学》2008,29(2):321-326

研究了考虑涂抹效应和应力集中效应的双层散体材料桩复合地基固结解析解及其工程应用,分不同情况讨论了特征根的可能变化规律,也讨论了解析解转化为双层竖井地基以及双层天然地基的普遍适用性。研究发现,固结速率随井径比的减小、水平向渗透系数比的增大和桩体刚度的增大而增加;底面排水条件对双层散体材料桩复合地基的固结影响,在井径比不是很大的情况下影响不大;是否考虑应力集中效应对计算结果影响较大。  相似文献   

广义Drucker-Prager强度准则   总被引：8，自引：0，他引：8  

周凤玺  李世荣 《岩土力学》2008,29(3):747-751

基于摩擦性材料的试验研究,在已有研究成果的基础上,提出了具有Drucker-Prager准则表达形式的广义非线性强度理论,即广义Drucker-Prager强度理论。该强度理论在偏平面上的强度函数是介于Drucker-Prager准则和Mohr-Coulomb准则外包线的光滑外凸曲线,在子午面上的强度函数为线性函数。该强度理论用一个表达式来统一描述材料的强度特性,包含或逼近了现有主要的非线性单一强度理论,并且在应力空间中偏应力和静水压力分离,容易与具体的应力应变模型相结合。  相似文献   

含圆柱形弹性夹杂地基沉降量的解析解     

王明斌  李术才  李树忱  王兆清 《岩土力学》2008,29(6):1575-1579

研究各向同性地基中含一个圆柱形弹性夹杂的地基沉陷问题。考虑全场的应力、变形特征,运用复变函数的罗朗级数展开技术,构造合适的应力函数,结合夹杂的边界条件和无穷远的性态,获得了全场复势的解析表达。数值结果显示：由于两相材料剪切模量之比的不同,在某个范围内沉陷量大于基底中点沉陷;在这个范围之外,则小于基底中点沉陷。当夹杂埋深为夹杂半径的5倍以上时,就可以运用所得结果,而不致引起太大误差;含圆形隧洞和刚性夹杂的问题可作为特殊情况得到。  相似文献   

桩-土相互作用影响的模型试验研究   总被引：5，自引：2，他引：3  

王涛 《岩土力学》2008,29(6):1589-1592

通过将模型试验、现场实测的结果与弹性理论解进行对比,指出弹性理论解夸大了桩-桩、桩-土、土-土相互作用影响,造成沉降计算值偏大和过高估计桩顶反力的不均匀性（或筏底地基土反力的不均匀性）,并提出对弹性理论解进行修正的途径和方法。  相似文献   

溪洛渡水电站某危岩体稳定性及加固措施研究     

黄达  黄润秋  裴向军  刘卫华 《岩土力学》2008,29(5):1425-1429

在现场调查分析的基础上,提出了溪洛渡水电站某危岩体的两种可能失稳模式（剪切坠落或拉裂倾倒失稳）,进而建立了相应的稳定性计算极限平衡力学模型,而且对危岩体的变形和破坏特征进行了数值模拟分析,分析结果表明,危岩体抗拉裂倾倒稳定性较差,剪切坠落失稳的稳定性系数较高。在稳定性分析的基础上,计算出危岩体倾倒失稳时,安全系数为1.5时的锚固力,进而提出了危岩体加固方案：充填凹岩腔+填充裂隙+预应力锚索＋锚杆联合加固,数值模拟表明此加固方案效果良好。  相似文献   

基于分布式光纤传感技术的渗流监测理论研究   总被引：6，自引：1，他引：5  

肖衡林  鲍华  王翠英  蔡德所 《岩土力学》2008,29(10):2794-2798

从阐述多孔介质传热过程出发,逐一分析了在非渗流及渗流情况下,光纤与多孔介质之间的传热过程,详细分析了光纤与水流对流的传热过程,推导了多孔介质中渗流水和光纤之间的换热系数计算公式。在一定假设条件下,推导了导热系数（渗流流速）、加热功率和温升的非渗流情况与渗流情况监测理论方程,为分布式光纤传感技术监测渗流的应用提供了坚实的理论基础。  相似文献   

Gamma-ray emission from individual classical novae     

Jordi Gómez-Gomar  Margarita Hernanz  Jordi José  & Jordi Isern 《Monthly notices of the Royal Astronomical Society》1998,296(4):913-920

Classical novae are important producers of radioactive nuclei, such as ⁷Be, ¹³N, ¹⁸F, ²²Na and ²⁶Al. The disintegration of these nuclei produces positrons (except for ⁷Be) that through annihilation with electrons produce photons of energies 511 keV and below. Furthermore, ⁷Be and ²²Na decay producing photons with energies of 478 and 1275 keV, respectively, well in the γ-ray domain. Therefore, novae are potential sources of γ-ray emission. We have developed two codes in order to analyse carefully the γ-ray emission of individual classical novae: a hydrodynamical one, which follows both the accretion and the explosion stages, and a Monte Carlo one, able to treat both production and transfer of γ-ray photons. Both codes have been coupled in order to simulate realistic explosions. The properties of γ-ray spectra and γ-ray light curves (for the continuum and for the lines at 511, 478 and 1275 keV) have been analysed, with a special emphasis on the difference between carbon–oxygen and oxygen–neon novae. Predictions of detectability of individual novae by the future SPI spectrometer on board the INTEGRAL satellite are made. Concerning ²⁶Al, its decay produces photons of 1809 keV but this occurs on a time-scale much longer than the typical time interval between nova outbursts in the Galaxy, making it undetectable in individual novae. The accumulated emission of ²⁶Al from many Galactic novae has not been modelled in this paper.  相似文献