旅游中心城市在旅游业中的地位和功能研究   总被引：10，自引：0，他引：10  

董志文  盛红 《海岸工程》2002,21(1):57-62

从中国旅游业发展实际出发,深入分析了旅游中心城市在旅游业发展中的地位和作用.通过探讨旅游资源开发与旅游城市建设的关系,确立旅游中心城市的主导地位,阐述旅游中心城市的主要功能,分析区域旅游发展的时空演化规律,并对发展旅游中心城市提出3点建议.  相似文献   

地下浅部异质体对表面波场谱扰动分析     

柴华友  柯文汇  柴扬斐  朱红西  王贤达  刘欢 《岩土力学》2022,43(6):1683-1693

均匀半无限体中表面源激发近表面波场由瑞利波主导,当浅部存在异质体,前行瑞利波发生散射,异质体周围表面波场响应谱发生变化。当异质体长度相对波长较大时,由异质体上方表面质点响应谱提取绕射波频散曲线可分析异质体与周围介质刚度差异对绕射波传播特性的影响。与含软层或硬层半无限体中瑞利波特性比较,可以发现绕射波具有与瑞利波类似的传播特性。异质体上方谱变化特征与异质体和周围介质间刚度差异有关,本研究基于异质体绕射波与入射瑞利波位移结构差异解释谱变化现象。结果表明：异质体上方谱与周围谱明显不同,在偏移距−波长域,相对于前方波场,软质体上方谱密度整体呈减弱趋势,硬质体上方谱密度整体呈增强趋势。根据谱密度变化对应偏移距、波长及谱密度强弱,可以预估异质体在传播方向的位置、埋深,并识别异质体类型。  相似文献   

改进的等效半空间法及瑞雷波频散曲线反演   总被引：5，自引：4，他引：5       下载免费PDF全文

陈祥  孙进忠 《地球物理学报》2006,49(2):569-576

层状模型的理论频散曲线表明，层状模型表面瑞雷波同一频率对应的相速度具有多值特点，这就是所谓的瑞雷波多阶性. 面波的多阶性导致了实测频散曲线的复杂性，当地层中存在软弱夹层时这一问题尤为突出，从而给实测频散曲线的解释带来了困难. 本文从工程实用的角度出发，根据等效半空间理论，提出了一种计算理论频散曲线的新算法——改进的等效半空间法，避开了面波多阶性这一复杂问题. 由此方法计算得到的面波相速度并不同于某个具体阶数的面波，而是对多阶面波的综合反映. 按照改进的等效半空间法编制了拟合反演程序，并在工程中进行了运用，取得较好的效果.  相似文献   

电法在秦岭钼多金属矿区找盲应用     

张开盾  张锋军  张倩 《陕西地质》2012,30(1):48-54

本文以电法在秦岭某钼多金属矿区寻找深部盲矿的应用为例,介绍了电法勘查方法应用效果,说明物探资料在地球物理前提条件具备时,可以为矿区设计和开发生产过程提供重要的信息和依据,在相似地区深部找矿和寻找盲矿体具有一定借鉴意义。  相似文献   

大功率激电在黔西北探测铅锌矿中的应用     

董国成 《四川地质学报》2012,(4):475-476

采用大功率激电对贵州赫章联发村地区铅锌矿做地质探讨评价。通过对该地区地质背景和成矿规律的研究。总结出该地区铅锌矿电性突出,具有“低视电阻率,高视极化率”特征。  相似文献   

Vertical amplitude reduction of Rayleigh waves by a row of piles in a poroelastic half‐space     

Yuan‐Qiang Cai  Guang‐Ya Ding  Chang‐Jie Xu  Jun Wang 《国际地质力学数值与分析法杂志》2009,33(16):1799-1821

A row of rigid piles is addressed as the countermeasures for isolating Rayleigh waves in a poroelastic half‐space. The complex characteristic equations for Rayleigh waves are derived via Biot's theory and their existence conditions are given. The piles are modeled as Euler–Bernoulli beams with longitudinal displacements and the diffracted field by each pile is constructed only with Rayleigh waves. Six infinite linear systems of algebraic equations are obtained in terms of the equilibrium of forces and continuity of displacements at the pile–soil interfaces. The systems are subsequently solved in the complex least‐squares sense. The influence of certain pile and soil characteristics such as the permeability of poroelastic soil, spacing between the piles and length of the piles on the isolating performance of a pile barrier is investigated. Computed results show that the permeability of poroelastic soil displays a significant effect on the vertical amplitude reduction of Rayleigh waves. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

The statistical distribution of nearbed wave orbital velocity in intermediate coastal water depth     

Zai-Jin You 《Coastal Engineering》2009

The statistical distribution of wave orbital velocity in intermediate coastal water depth has been quantitatively determined from the comprehensive field velocity data collected near the seabed in this study. Two ocean ADV current meters, which were mounted at 0.5 m above the seabed on two separate stainless steel tripods sitting on the seabed, were used to measure instantaneous water particle velocities at a 2 Hz sampling rate for 17.07 min every hour in two coastal water depths of 11 m and 23 m in nine field deployments over a period of 2 years. The zero-crossing method is applied to analyse the field velocity data collected in each field deployment to obtain a large sample of wave orbital velocity amplitudes of individual waves. Based on the collected field velocity data, it is found that the histogram of instantaneous wave orbital velocities perfectly follows the Gaussian distribution as commonly assumed, while the histogram of wave orbital velocity amplitudes is less accurately described by the Rayleigh distribution than the modified Rayleigh and the Weibull distribution. It is also found that large orbital velocity amplitudes are generally overestimated by the Rayleigh distribution, but well predicted by the modified Rayleigh and the Weibull distribution. The expected value of maximum orbital velocity in a velocity record of finite size is also derived from the three distributions and found to agree well with the present field data.  相似文献   

Constraining the geometry of the neutron star RX J1856.5−3754     

Wynn C. G. Ho 《Monthly notices of the Royal Astronomical Society》2007,380(1):71-77

RX J1856.5−3754 is one of the brightest, nearby isolated neutron stars (NSs), and considerable observational resources have been devoted to its study. In previous work, we found that our latest models of a magnetic, hydrogen atmosphere match well the entire spectrum, from X-rays to optical (with best-fitting NS radius   R ≈ 14  km, gravitational redshift   z _g∼ 0.2  , and magnetic field   B ≈ 4 × 10¹²  G). A remaining puzzle is the non-detection of rotational modulation of the X-ray emission, despite extensive searches. The situation changed recently with XMM–Newton observations that uncovered 7-s pulsations at the     level. By comparing the predictions of our model (which includes simple dipolar-like surface distributions of magnetic field and temperature) with the observed brightness variations, we are able to constrain the geometry of RX J1856.5−3754, with one angle <6° and the other angle     , though the solutions are not definitive, given the observational and model uncertainties. These angles indicate a close alignment between the rotation and the magnetic axes or between the rotation axis and the observer. We discuss our results in the context of RX J1856.5−3754 being a normal radio pulsar and a candidate for observation by future X-ray polarization missions such as Constellation-X or XEUS .  相似文献   

γ-ray burst ultraviolet/optical afterglow polarimetry as a probe of quantum gravity     

Yi-Zhong Fan †  Da-Ming Wei  Dong Xu 《Monthly notices of the Royal Astronomical Society》2007,376(4):1857-1860

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高速Ia型超新星的蓝色超出: 星周介质的尘埃散射          下载免费PDF全文

胡茂凯  王力帆  王晓锋 《天文学报》2023,64(2):13-22

Ia型超新星起源于碳氧白矮星在质量接近钱德拉塞卡极限时的热核爆炸,并被广泛地用作宇宙学距离的标准烛光.然而, Ia型超新星的前身星系统和爆炸机制还存在很多不明确的地方.近几十年来, Ia型超新星的星周环境得到了越来越多的关注.星周介质的空间分布性质为探究Ia型超新星的物理起源提供了重要线索.同时星周尘埃的散射会在Ia型超新星晚期的光变曲线、光谱和偏振等方面产生可观测效应.光谱上正常的Ia型超新星可以分成两类:喷射物速度正常和高速Ia型超新星.对比两者的光变曲线可以发现高速Ia型超新星在光极大后几个月内有明显颜色偏蓝的超出.该蓝色超出可以通过星周介质中的尘埃散射拟合得到.同时, Ia型超新星晚期光谱的拟合可以限制星周尘埃的颗粒大小等性质,晚期的偏振信号可以有效地限制星周尘埃的空间分布.拟合结果表明针对Ia型超新星晚期的多次图像偏振观测是揭示其星周尘埃环境特征的重要手段.  相似文献