旅游供给与需求的空间关系研究   总被引：80，自引：4，他引：80  

牛亚菲 《地理学报》1996,51(1):80-87

本文研究旅游供给与旅游需求的地域分布规律和空间联系特征，提出了旅游供给与需求的空间模式以及二者之间的动态平衡关系。并根据我国旅游供需分布特点，以大城市为中心，分析了不同地域旅游供需关系。  相似文献   

植物在不同形态和不同状态下的荧光光谱特征研究     

吴荣  张崇静  朱永豪  刘南英  沈玉其  徐彬彬  石晓日  李德成  周斌 《遥感学报》1992,(Z1)

本文从光合作用的角度出发,讨论了植物叶片在不同形态、不同状态下的荧光光谱特征以及它们对荧光光谱的影响。文章涉及了以下几方面的内容:(1)植物在离体形态和活体形态下的荧光光谱特征;(2)叶片正面与反面的荧光光谱特征;(3)植物不同器官对荧光光谱的影响;(4)叶片放置时间对荧光光谱的影响;(5)叶片经不同处理时对荧光光谱的影响等。其目的是为激光荧光技术用于植被遥感的实施提供基础数据。  相似文献   

ISO Far-IR spectroscopy of IR-bright galaxies and ULIRGs     

J. Fischer  M.L. Luhman  S. Satyapal  M.A. Greenhouse  G.J. Stacey  C.M. Bradford  S.D. Lord  J.R. Brauher  S.J. Unger  P.E. Clegg  H.A. Smith  G. Melnick  J.W. Colbert  M.A. Malkan  L. Spinoglio  P. Cox  V. Harvey  J.-P Suter  V. Strelnitski 《Astrophysics and Space Science》1999,266(1-2):91-98

Based on far-infrared spectroscopy of a small sample of nearbyinfrared-bright and ultraluminous infrared galaxies (ULIRGs) with theISO Long Wavelength Spectrometer we find adramatic progression in ionic/atomic fine-structure emission line andmolecular/atomic absorption line characteristics in these galaxiesextending from strong [O III]52,88 m and [N III]57 m lineemission to detection of only faint [C II]158 m line emissionfrom gas in photodissociation regions in the ULIRGs. The molecularabsorption spectra show varying excitation as well, extending fromgalaxies in which the molecular population mainly occupies the groundstate to galaxies in which there is significant population in higherlevels. In the case of the prototypical ULIRG, the merger galaxy Arp220, the spectrum is dominated by absorption lines of OH, H₂O, CH,and [O I]. Low [O III]88 m line flux relative to the integratedfar-infrared flux correlates with low excitation and does not appear tobe due to far-infrared extinction or to density effects. A progressiontoward soft radiation fields or very dusty H II regions may explainthese effects.  相似文献   

既找矿又开矿搞活地勘单位：赴疆考察的认识和体会     

张攀华 《湖南地质》1993,12(2):70-74,79

“六五”和“七五”期间,新疆地矿局强化了地质找矿的科学管理,充分发挥了地质科技在找矿中的先导作用,争取到了一个好的外部环境,取得了地质找矿的重大突破。他们既找矿又开矿,以找矿促开发,走找矿与开矿结合的道路,实行探、采、工、贸一体化,创造了搞活地勘单位,振兴地方经济的成功经验。  相似文献   

土层结构对反应谱特征周期的影响   总被引：20，自引：3，他引：17  

薄景山  李秀领  刘德东  刘红帅 《地震工程与工程振动》2003,23(5):42-45

本文选取和构造了若干有工程意义的典型场地剖面,利用目前工程上广泛应用的场地地震反应分析的一维等效线性化波动方法,计算了在不同地震动输入下的不同场地剖面的地表加速度峰值和地表速度峰值。利用计算得到的地表加速度峰值和速度峰值计算了不同场地在不同地震动输入下的反应谱的特征周期。研究了不同土层结构对地表加速度反应谱特征周期的影响,获得了一些有意义的结果。  相似文献   

Multi‐variable relations for soil effects on seismic ground motion     

George D. Bouckovalas  Achilleas G. Papadimitriou 《地震工程与结构动力学》2003,32(12):1867-1896

Soil effects on peak ground acceleration, velocity and elastic response spectra (5% damping) are expressed by simple approximate relations in terms of five key parameters: (a) the fundamental vibration period of the non‐linear soil, T_S, (b) the period of a bedrock site of equal thickness, T_b, (c) the predominant excitation period, Te, (d) the peak seismic acceleration at outcropping bedrock, a, and (e) the number of significant excitation cycles, n. Furthermore, another relation is proposed for the estimation of T_S in terms of the soil thickness H, the average shear wave velocity of the soil V?_S,o and a. The aforementioned parameters were first identified through a simplified analytical simulation of the site excitation. The multivariable approximate relations were then formulated via a statistical analysis of relevant data from more than 700 one‐dimensional equivalent‐linear seismic ground response analyses, for actual seismic excitations and natural soil conditions. Use of these relations to back‐calculate the numerical results in the database gives an estimate of their error margin, which is found to be relatively small and unbiased. The proposed relations are also independently verified through a detailed comparison with strong motion recordings from seven well‐documented case studies: (a) two sites in the San Fernando valley during the Northridge earthquake, and (b) five different seismic events recorded at the SMART‐1 accelerometer array in Taiwan. It is deduced that the accuracy of the relations is comparable to that of the equivalent‐linear method. Hence, they can be readily used as a quick alternative for routine applications, as well as for spreadsheet computations (e.g. GIS‐aided seismic microzonation studies) where numerical methods are cumbersome to implement. Copyright © 2003 John Wiley & Sons, Ltd.  相似文献   

2001年世界黄金供需形势     

王淑玲 《黄金地质》2003,9(2):55-60

2001年受美国经济放缓,尤其是"9·11"事件的影响,世界黄金需求下降2 6%,金价低迷,以271 04美元 盎司的年均金价再次刷新了1978年以来的最低价位。持续恶劣的价格环境,促进了黄金矿业公司间的相互兼并,以此降低经营成本,提高国际竞争能力。受金价下跌的影响,金矿勘查费用再次下降。尽管如此,2001年黄金仍是全球固体矿产勘查投资最多的矿种,是全球勘查开发热点,黄金储量和储量基础仍保持增长态势,金资源保证程度增加。金产量并未因金价下跌而减少。  相似文献   

Peculiarities of the UV continuum energy distribution for T Tauri stars     

A. S. Kravtsova  S. A. Lamzin 《Astronomy Letters》2003,29(9):612-620

In the UV spectra of BP Tau, GW Ori, T Tau, and RY Tau obtained with the Hubble Space Telescope, we detected an inflection near 2000 Å in the F _λ ^c (λ) curve that describes the continuum energy distribution. The inflection probably stems from the fact that the UV continuum in these stars consists of two components: the emission from an optically thick gas with T<8000 K and the emission from a gas with a much higher temperature. The total luminosity of the hot component is much lower than that of the cool component, but the hot-gas radiation dominates at λ<1800 Å. Previously, other authors have drawn a similar conclusion for several young stars from low-resolution IUE spectra. However, we show that the short-wavelength continuum is determined from these spectra with large errors. We also show that, for three of the stars studied (BP Tau, GW Ori, and T Tau), the accretion-shock radiation cannot account for the observed dependence F _λ ^c (λ) in the ultraviolet. We argue that more than 90% of the emission continuum in BP Tau at λ>2000 Å originates not in the accretion shock but in the inner accretion disk. Previously, a similar conclusion was reached for six more classical T Tau stars. Therefore, we believe that the high-temperature continuum can be associated with the radiation from the disk chromosphere. However, it may well be that the stellar chromosphere is its source.  相似文献   

使用小波技术自动搜寻天体谱线     

罗阿理  赵永恒 《中国天文和天体物理学报》2000,20(4)

使用小波技术对包括恒星、近邻星系和ＡＧＮ等不同的天体光谱进行了自动处理．用小波滤波的方法将光谱中的连续谱与诸线分离;然后使用小波域隐含马尔可夫模型（ＨＭＭ）,对已去掉连续谱的光谱进行降噪,同时得到了噪声在每个光谱中的分布;在训练ＨＭＭ的过程中,使用改进的Ｔｙｉｎｇ方法增加训练数据以保证训练的可靠性;利用噪声分布确定出谱线信号的局部阈值,在已经降噪的光谱中找到吸收线和发射线;用高斯函数拟会出谱线的形状,标出线心的波长值,作为自动证认的基础．  相似文献   

南京市近地层湍流结构及输送特征研究   总被引：8，自引：2，他引：6  

陈铭夏  李宗恺 《气象科学》2000,20(2):111-119

本文利用"城市生物气溶胶研究”中的超声风温仪观测资料,对南京市近地层大气的湍流强度、相关系数、速度谱及通量输送等进行研究,得到南京市近地层湍流结构及输送特征的一些结论.  相似文献