边界层风廓线雷达相控阵天线子阵设计与应用

对比研究了国内外风廓线雷达产品天线系统和子阵的类型,设计了一款5波束有限相扫相控阵微带天线子阵。此天线系统由21个相同的正方形子阵组成,每个子阵包含16个阵元,4×4的正方形对称划分,每个阵元采用东西向、南北向2点同轴背馈馈电,子阵内双方向分别设计了等幅等相馈电网络,进而实现了东西向和南北向的水平极化。天线子阵各端口驻波小于1.2,提高了天线探测灵敏度,缩小了相控阵天线阵面面积,减轻了天线阵重量。结合子阵划分,优化了相控阵天线系统泰勒加权。天线具有两维步进电扫功能,在空域形成5个波束的探测。应用在TWP3型边界层风廓线雷达上,雷达探测高度大于5km。     

电子导体的极化暂态特性与差异激电法

电子导体的极化暂态特性与电子导体的性质有密切关系。差异激电法的观测参数─激电差△P能够反映这种特性。本文用极化暂态特性的理论对石墨板、铜板和铁板三种模型上激电差△P异常的基本形态各不相同的现象作了初步解释,说明根据激电差△P异常的基本形态可以把不发生阳极溶解、不可逆性较弱和不可逆性较强的矿石─围岩溶液体系区分开,并且可以剔除炭质干扰。文中还给出了野外试验结果和应用实例。极化暂态特性反映的信息量很丰富,进一步研究有利于激电异常的区分和场源性质的识别。     

微机井中激电仪的应用效果

简述DJJ-1型井中激电仪软件系统和几个应用实例。实例表明,在钻孔见矿的情况下,方位测量可用于查明矿体的空间形态和延展情况。     

嘎衣穷多金属矿床的激电勘查

白玉县嘎衣穷矿区经过三年的激发极化法测量工作,圈定了南北两个长达2200m的激电异常带,在异常带中进一步圈定了8个局部异常,其中Ⅱ_1号异常长440m,宽10—20m,经工程查证,圈定多金属矿体长360m,平均厚度9.11m;Ⅱ_2、Ⅲ_3号异常长约1300m,宽约20—60m,经工程查证,圈定多金属矿体长870m,地表最大厚度21.4m。通过激电工作同时发现了矿区南东部位的大规模异常,经少量地表、深部工程控制也已见到了多金属矿体。嘎衣穷矿床属火山岩型多金属矿床,地质、地球物理条件对开展激电工作都较有利,所以取得了较好的找矿效果。     

Shear wave splitting and polarization anomaly with deep seismic sounding data

In this paper we study the S wave basement velocity structure and S wave splitting and polarization anomalies using the three component records of deep seismic sounding in the Three Groges Dam area, and further discuss the methods to study the anisotropy of crustal medium, the direction of regional tectonic stress field, and the physical indicator of potential earthquake sources using shear wave splitting and polarization anomalies. It has been demonstrated by analyzing the DSS data in the Three Gorges Dam area that S wave splitting and polarization anomalies are reliable means for studying seismic anisotropy of crustal medium and the direction of regional tectonic stress field. At the same time, it has been shown that DSS data are very useful for widening S wave observing window and distinguishing anomalous body, because DSS data have the advantage that the source position is known prior and S wave ray path can be traced exactly. The Chinese version of this paper appeared in the Chinese edition ofActa Seismologica Sinica,15, 1–3, 1993.     

On the structure of ducts for mid-latitude whistlers and their ionospheric transmission as deduced from the ground-based direction finding

The ground-based direction finding carried out at Ceduna, Australia (L=1.93) has yielded the structure for mid-latitude whistlers and their duct ionospheric transmission mechanism. It is found that the ducts tend to take place (or be formed) at the same latitudes and that such sheet-shaped duct includes some inhomogeneities within it which act as field-aligned ducts.     

河南宜阳下三叠统刘家沟组微生物成因沉积构造演化及其对古环境变化的响应*

河南宜阳地区下三叠统刘家沟组红色砂岩中发育数十种微生物成因沉积构造(MISS),如皱饰构造、脱水裂痕、微生物席碎片等。按照其形态特征的演化可分为4个不同的组合,由下往上依次为皱饰构造组合、隆脊构造组合、小型脱水裂痕组合和大型脱水裂痕组合,其分别反映了不同的古环境与古气候: (1)皱饰构造组合反映了弱氧化的温暖、潮湿环境;(2)隆脊构造组合反映了富氧的温暖、潮湿环境;(3)小型脱水裂痕组合反映了弱氧化的温暖、半干旱环境;(4)大型脱水裂痕组合反映了富氧的炎热、半干旱—干旱环境。依据研究区的地球化学特征和岩石学特征,认为早三叠世宜阳地区的古环境由湿润、温暖、弱氧化向炎热、半干旱、富氧转变。两者比较表明,宜阳地区微生物成因沉积构造的发育与演化是对早三叠世陆相古环境细微变化的联动响应。     

直流激电测深多参数综合分析划分含水异常岩体

直流激电测深观测 (计算) 的参数多, 现已成为一种有效的找水方法。但由于不同的地区存在各种不同的干扰, 因此, 合理、准确地综合利用这些参数, 减少多解性, 避免解释错误显得尤为重要。本文在分析原始实测参数的基础上, 对部分参数进行了转化, 使其抗干扰能力更强, 资料解释更可靠, 并通过实例评价了部分参数的优越性和局限性。应用实例表明, 多参数综合解释方法具有推广意义。      

Giant radio sources

We present multifrequency Very Large Array (VLA) observations of two giant quasars, 0437−244 and 1025−229, from the Molonglo Complete Sample. These sources have well-defined FR II radio structure, possible one-sided jets, no significant depolarization between 1365 and 4935 MHz and low rotation measure (|RM|<20 rad m⁻²). The giant sources are defined to be those with overall projected size 1 Mpc. We have compiled a sample of about 50 known giant radio sources from the literature, and have compared some of their properties with a complete sample of 3CR radio sources of smaller sizes to investigate the evolution of giant sources, and test their consistency with the unified scheme for radio galaxies and quasars. We find an inverse correlation between the degree of core prominence and total radio luminosity, and show that the giant radio sources have similar core strengths to smaller sources of similar total luminosity. Hence their large sizes are unlikely to be caused by stronger nuclear activity. The degree of collinearity of the giant sources is also similar to that of the sample of smaller sources. The luminosity–size diagram shows that the giant sources are less luminous than our sample of smaller sized 3CR sources, consistent with evolutionary scenarios in which the giants have evolved from the smaller sources, losing energy as they expand to these large dimensions. For the smaller sources, radiative losses resulting from synchrotron radiation are more significant while for the giant sources the equipartition magnetic fields are smaller and inverse Compton loss owing to microwave background radiation is the dominant process. The radio properties of the giant radio galaxies and quasars are consistent with the unified scheme.