南水北调中线初期引汉工程经济效益初探

南水北调是补充华北地区新水源的有效途径之一。“中线”初期引汉工程是从长江支流汉江调水,渠线跨越汉江、淮河、黄河、海河四大水系,直达北京市。引汉水源是丹江口水库。该库集流面积95200平方公里,多年平均年径流量380亿立米,已建成初期规模。坝顶高程162米,正常蓄水位157米,总库容174.5亿立米。     

On the Line Formation in Stellar Magnetized Atmospheres

1 INTRODUCTIONIn the previous paper (on et al. 1999, hereafter Paper I), we investigated the wavelength-dependence of four colltribution functions (CFs) derived from dmerent formal solutions andreferring to different emergellt quantities in the unpolarized case. Because one cannot generallyassign a single formation region to the whole line band in a real stellar atmosphere, e.g., the solaratmosphere, instead, the line formation region can be defined as the layers deviating farthestfrom t…     

Paleoproterozoic Extensional Structure and Its Controlling on Mineralization in the East of Liaoning Province

IntroductionThe area of eastern Liaoning is an importantmetal and nonmetal metallogenetic district in China,and the Liaohe group is one of the most importantstrata that hosts Pb, Zn, Au, B and Mg etcstratabound deposits. Up to now many geo1ogistssuch as Z…     

抗差估计的初值选择

对L1 范估计的平差值和LS估计的平差值作为抗差估计的初值进行了比较 ,指出在 ρ函数是严凸函数时 ,二者无明显的区别。因为LS估计简单且易于计算 ,因此建议用LS估计的平差值作为抗差估计的初值。     

On the influence of magnetic fields on level populations

The influence of magnetic fields on the energy level populations of atoms is firstly studied by analysing the Stokes profiles of Fe  i 6302.5 forming in the solar magnetized atmosphere, with the aid of a departure factor defined to evaluate the deviation from the normal Boltzmann distribution without a magnetic field. This factor is directly related to the ratio of line-source function to the continuum one. The relationship between the departure and the magnetic field reveals an effect that the magnetic field induces an exponential increase in the level population of the lower level of Fe  i 6302.5 (Landé factor   g = 2.5  ) with the field strength. This indicates that the magnetic field can cause the redistribution of populations of those levels whose Landé factors are non-zero. Therefore, this effect should be included in the calculation of the statistical equilibrium. Secondly, an experiment utilizing the Hg5461 line in the laboratory on the Earth is carried out to reveal that the exponential relation is independent of variations in temperature, and the excitation is completely magneto-induced. Finally, the exponential relation is explained by taking account of the magnetic energy in the Boltzmann distribution.     

Direct generation of solar and stellar radio bursts by energetic electron maser

A fully relativistic electron maser is proposed for the explanation of certain non-thermal solar and stellar radio bursts. This mechanism (maser synchrotron) is based on a gyroresonant interaction between waves and electrons of high energies and uses the free energy contained in an electronic distribution function that peaks for energies around 1 MeV.By a calculation of the growth rates of the three electromagnetic modes, we show that the X-mode prevails for values of _p/ _cup to 2 or 3. This result is very different from the standard cyclotron maser case where such values of _p/ _clead to quench the X-mode growth. Hence, the synchrotron maser instability appears to be a direct and efficient amplification process for considerably larger physical conditions than the cyclotron maser. In addition, the radiation, emitted over the second gyroharmonic, freely propagates without a strong reabsorbtion at the 2 _clayer. All these points can constitute major advantages of this mechanism in an astrophysical context.Proceedings of the Second CESRA Workshop on Particle Acceleration and Trapping in Solar Flares, held at Aubigny-sur-Nère (France), 23–26 June, 1986.     

海上不同高度风速换算关系的研究

本文用海上石油平台上观测的风梯度资料,计算了在不同风况下海面摩擦速度和粗糙高度。结果表明,海面摩擦速度u_*与海上10m高度处风速u_(10)的关系为u_*=0.055u_(10)-0.058。在4—5级风时,海面平均摩擦速度为50cm/s,粗糙度为0.022m,它相当于陆上的平均粗糙高度。在风速为2—3级时,二者与海上通常采用的数据接近。文中最后给出了上述两种风况下海上不同高度的换算系数。     

渤海、黄海、东海海面热量平衡的平均状况——Ⅰ.资料处理和计算方法

渤、黄、东海海面热量平衡状况对该海域海洋水文和中国气候有着重要的影响。我们对该海域热量平衡各分量的年平均和年变化进行了计算,并分别就资料处理和计算方法、年平均状况、年变化特征等几个方面进行了分析。本文作为该项研究的第一部分,讨论了所用的资料和计算公式,提出了在稳定温度层结条件下的交换系数的校正方法。     

冬季中纬度海气相互作用与长江中下游汛期旱涝预测

中纬度海洋的热力状况对大气环流的维持和变化起着重要的作用,尤其在冬季。汛期的研究表明,冬季黑潮海域海表面水温(SST)与长江中下游和华北平原汛期降水有密切的关系(中国科学院大气物理研究所长期预报组,1978),夏季阿留申海域的SST异常与北太平洋上空大气环流场和后期秋季美国的气温和降水亦存在有意义的关系(Namias,1976)。赵永平(1986a;赵永平, McBean,1996)和Zhao and McBean(1989)曾用北太平洋海洋对大气加热场资料详细地分析了其时空分布特征,揭露了黑潮及邻近海域海洋异常加热对同期和后期半年至一年北半球大气环流的影响事实,并提出用海洋异常加热对同期和后期大气环流作用的反相性假说来进行解释。以上研究表明,冬季中纬度海洋异常加热与大气环流的异常和我国汛期旱涝之间存在一定的联系。 冬季黑潮和湾流海域是中纬度海洋的两个巨大热源,它们对同期和后期大气环流有重要影响。本文研究了冬季中纬度黑潮和湾流海域海洋异常加热对夏季副热带高压和中高纬度西风环流的影响,讨论了长江中下游汛期旱涝前期冬季和同期大气环流型。结果表明,冬季东亚和北美冷空气都强时,黑潮和湾流海域对大气异常多加热,夏季西太副热带高压、乌山和鄂海阻塞高压多趋减弱,中纬环流平直,形成长江中下游偏旱的环流形势；反之,西太副热带高压、乌山和鄂海阻塞高压多趋加强,中纬槽脊系统明显,形成长江中下游偏涝的环流场。本文还对可能的物理过程进行了讨论。     

副热带海域的海洋加热异常及其对副高的影响

海洋在天气、气候及大气环流变化过程中起着重要作用,海洋热源的异常分布是造成长期天气异常的重要原因。海洋对大气的作用主要是通过海气界面的热量交换来实现的，因此,直接运用海气热量交换来考虑海洋对大气的加热作用,分析海洋加热异常对长期天气、气候及大气环流的影响,具有更明确的物理意义。 西北太平洋副热带高压是造成我国旱、涝及天气变化的主要副热带天气系统,对我国夏季气温、雨带位置及强度影响很大。西北太平洋中、低纬副热带地区是海洋向大气提供热量和水汽较多的地区,也是海气相互作用最强烈的海域,这一地区的海洋加热对西北太平洋副热带高压的变化将有直接影响。本文分析了冬季西北太平洋副热带海域海洋加热主要场的分布特征,指出了海洋加热与西北太平洋副热带高压的关系。结果表明,冬季该海域海洋加热较常年偏多时,冬、春至初夏副高偏弱,位置偏东、南(6月副高脊线位置除外);反之,海洋加热较常年偏少时,副高偏强,位置偏西、北(6月副高脊线位置除外)。该海域海洋加热对副热带地区大气环流,尤其是副热带高压环流的变化有着重要作用。本结果对预测西北太平洋副热带高压的变化,研究中纬度海洋加热对西北太平洋副热带高压及其大气环流的影响有十分重要的意义。