Measurements of the direction of the solar wind using interplanetary scintillation     

P. J. Moran  A. R. Breen  C. A. Varley  P. J. S. Williams  W. P. Wilkinson  J. Markkanen 《Annales Geophysicae》1998,16(10):1259-1264

EISCAT observations of the interplanetary scintillation of a single source were made over an extended period of time, during which the orientation of the baselines between the two observing sites changed significantly. Assuming that maximum correlation between the scintillations observed at the two sites occurs when the projected baseline is parallel to the direction of plasma flow, this technique can be used to make a unique determination of the direction of the solar wind. In the past it has usually been assumed that the plasma flow is radial, but measurements of eleven sources using this technique have indicated conclusively that in at least six cases observed at mid or high heliocentric latitude there is a significant non-radial component directed in four cases towards the heliocentric equator and in two cases towards the pole.  相似文献   

Velocity of auroral arcs drifting equatorward from the polar cap     

P. J. S. Williams  C. F. del Pozo  I. Hiscock  R. Fallows 《Annales Geophysicae》1998,16(10):1322-1331

The drift velocity of an auroral arc is compared with the component of F-region plasma velocity in the same direction for ten cases where the arc is seen to move steadily equatorward for several minutes without any major change in appearance or orientation. In most cases the two velocities are close, but on two occasions the drift velocity of the arc is much higher than the plasma velocity. From the cases studied it appears that during the growth and recovery phase of the substorm cycle the arc moves with a velocity close to the convection velocity, but during the expansion phase this is not the case.  相似文献   

Signatures of interplanetary transients behind shocks and their associated near-surface solar activity     

S. Bravo  X. Blanco-Cano 《Annales Geophysicae》1998,16(4):359-369

Interplanetary transients with particular signatures different from the normal solar wind have been observed behind interplanetary shocks and also without shocks. In this paper we have selected four well-known transient interplanetary signatures, namely: magnetic clouds, helium enhancements and bidirectional electron and ion fluxes, found in the solar wind behind shocks, and undertaken a correlative study between them and the corresponding solar observations. We found that although commonly different signatures appear in a single interplanetary transient event, they are not necessarily simultaneous, that is, they may belong to different plasma regions within the ejecta, which suggests that they may be generated by complex processes involving the ejection of plasma from different solar regions. We also found that more than 90% of these signatures correspond to cases when an H flare and the eruption of a filament occurred near solar central meridian between 1 and 4 days before the observation of the disturbance at 1 AU, the highest association being with flares taking place between 2 and 3 days before. The majority of the H flares were also accompanied by soft X-ray events. We also studied the longitudinal distribution of the associated solar events and found that between 80% and 90% of the interplanetary ejecta were associated with solar events within a longitudinal band of ±30° from the solar central meridian. An east-west asymmetry in the associated solar events seems to exist for some of the signatures. We also look for coronal holes adjacent to the site of the explosive event and find that they were present almost in every case.  相似文献   

含硬包体试样在破裂孕育过程中波速场的变化   总被引：2，自引：2，他引：0  

王彬  胡毅力 《地震研究》1998,21(3):256-260

含硬包体混凝土试样在底面支撑侧面双轴加压至主破裂的情况下波速场的变化图象为：加压初期,试样上的纵波平均速度在４１７５～４６１５ｍ／ｓ之间变化,随着压力升高,出现小于４１７５ｍ／ｓ的低速区,但范围甚小,位置在两个包体之间。随后出现大于４６１５ｍ／ｓ的高速区,范围大致与包体位置一致。随着σ１的增加,低速区在逐渐变大,高速区逐步减小后又重新变大,高速区与低速区在平面上相互重叠,在空间上看,高速区被低速区包围着。临近主破裂时,低速区变小并逐步形成条带,高速区也变小,主要集中在靠近未来出现破裂的一个包体位置上。最终的破裂面出现在此高速区与低速条带交界附近,包体也局部破裂了。  相似文献   

钢管高强混凝土叠合柱的抗震性能研究   总被引：11，自引：1，他引：10  

李惠  吴波  林立岩 《地震工程与工程振动》1998,18(1):45-53

通过周期性往复试验,研究了钢管高混凝土叠合柱柱的破坏形态,耗能能力、延性、承载力以及各种组成部分共同工作等内容,并与钢管高强混凝土核心柱进行了对比;随后通过计算,讨论了叠合柱中有关参数对其极限承载力和影响;最后给出了叠合柱正截面极限承载力的简化计算方法。  相似文献   

Non-equilibrium alcohol flooding model for immiscible phase remediation: 1. Equation development     

Stanley Reitsma  Bernard H. Kueper 《Advances in water resources》1998,21(8):1

The equations for a compositional model for simulation of a two-phase, three-component system with inter-phase mass transfer are developed. Emphasis is placed on development of inter-phase mass transfer equations for incorporation of rate-limited inter-phase mass transfer. Due to the nature of the three-component systems considered, a single-film model may be inadequate and a two-film model must be utilized. A two-film model accounts for the simultaneous transfer of components in both directions across phase interfaces. The effect of interaction between components on diffusion is considered using a general form of Fick's Law. A Hand Plot representation of ternary phase behavior is chosen since it allows for straightforward calculation of miscibility of bulk phases under conditions of local non-equilibrium. The developed set of equations form the basis for a numerical model to simulate the enhanced removal of non-aqueous phase liquids (NAPLs) from porous media using single-component alcohol floods.  相似文献   

Geological factors influencing the concentration of trace elements in the Philippi peatland, eastern Macedonia, Greece     

K. Christanis  A. Georgakopoulos  J. L. Fernndez-Turiel  A. Bouzinos 《International Journal of Coal Geology》1998,36(3-4)

Six peat samples obtained from the Holocene and the Weichselian of the Philippi peat deposit, eastern Macedonia, Greece, were analyzed for 48 trace elements by Inductively Coupled Plasma–Mass Spectrometry (ICP–MS). The ash contents of these samples were also determined. Most of the trace elements are associated with the minerals in the peat, while Ge, Mo, Pb, Se, Ta, Tl, U, and W display a greater affinity with the organic matter. Compared with crustal averages (Clarke concentrations), the Philippi peat is enriched in some elements (Ag, As, Au, Cd, Mo, Se, Te, U, and W) because of the respective mineralizations in the area. The Philippi peat is also enriched in Cr, Cu, Mo, Pb, Sc, Sn, T, V, Y, and Zn in comparison with typical fen peats, as well as in As, Cr, Mo, Se, and U in comparison with typical coals. Climatic and hydrogeological conditions strongly influenced the peat-forming environment resulting in a differentiation between Holocene and Weichselian peat. Generally, the Holocene peat contains lower concentrations of trace elements in the northern and southern part of the fen, than the Weichselian one. The opposite trend is observed in the fen area close to the western basin margins.  相似文献   

华北地台中寒武统张夏组上部高频层序研究   总被引：8，自引：1，他引：7  

陈建强  史晓颖 《地层学杂志》1998,22(2):109-115

根据华北地台东部寒武系露头层序地层研究,将张夏组划分为两个正层序,其中上部正层序（５３０－５２５ＭａＢ．Ｐ．,三叶虫带Ａｍｐｈｏｔｏｎ－Ｔａｉｔｚｕｉａ带至Ｄａｍｅｓｅｌａ带）由４个亚层序和１７－２３个小层序组成,其中正层序和亚层序具有高分辨率区域地层对比意义。每一级层序均表现为向上变浅和变粗进积型序列,底部常以间断－加深面或洪泛面为界。该时期的海平面变化具有高频振荡特点,构成一个三级复合海平面变化旋回。由不同级别层序所反映的海平面变化旋回可以分别与天文周期的奥特周期（２—５Ｍａ）、米兰科维奇长周期（０．１—０．４Ｍａ）和米兰科维奇短周期（０．０２—０．０４Ｍａ）相对比。据层序地层和相序及相模式的研究,识别出６种类型的小层序,陆棚盆地至上缓坡显示出由Ａ—Ｆ类型的规律性变化。  相似文献   

TFe/TiO_2比值在攀枝花层状辉长岩体钒钛磁铁矿矿床勘探中的应用     

邱仁轩  谢世敏 《四川地质学报》1998,(1)

攀枝花钒钛磁铁矿床是我国特大型晚期岩浆分凝型矿床。本文首次用ＴＦｅ／ＴｉＯ２比值对矿带、矿层、火成堆积旋回进行了详细划分,同时对断层位置、性质及矿床成因进行了判定,并提出在层状辉长岩体中,当ＴＦｅ／ＴｉＯ２比值小于２∶１的部位是寻找独立钛铁矿矿床最佳地段  相似文献   

江苏丰、沛、铜地区高氟地下水成因探讨   总被引：4，自引：0，他引：4  

张景荣  朱法华  陈汝秀  缪晓图  姚素平 《高校地质学报》1998,(2)

通过该区太古界一新生界氟的地层地球化学剖面及岩浆岩和土壤中氟的丰度的研究,论证了该区为一高氟的地球化学区。根据重矿物对比研究和地貌分析,阐明了泰沂隆起区太古界和元古界的高氟古老岩系为该区土壤沉积物源,黄河多次泛滥堆积（粘土矿物对氟的吸附）对土壤氟起了叠加富集的作用。研究揭示该区土壤水溶氟较高,经降水淋滤和浸取作用氟转入地下水,并在凹陷区或河间洼地中聚集,水体停泄、蒸发浓缩形成高氟地下水区。  相似文献