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31.
矿体的形成,尤其是矿体的赋存和保存与地质构造密切相关.目标勘查矿点构造控矿特征明显,为摸清勘查区内构造特征,圈定不同地质体及可能矿化体,我们使用DDS-3型甚低频电磁仪,结合高精度GPS开展地球物理勘查工作、圈定出一明显甚低频低阻异常,异常宽30-50m,断续分布,控制长200m.实践表明,使用甚低频磁倾角(D)测量法可以有效地揭示出勘查区内矿体及断裂构造的分布特征,为下一步研究及探矿工作提供初步依据.  相似文献   
32.
Extremely low frequency (ELF)/Very low frequency (VLF) hiss is whistler mode wave that interacts with energetic electrons in the magnetosphere. The characteristics features of ELF/VLF hiss observed at low latitude ground station Jammu (Geomag. lat. 22°16′ N, L=1.17) are reported. It is observed that most of hiss events first propagate in ducted mode along higher L-values (L = 4–5), after reaching lower edge of ionosphere excite the Earth-ionosphere waveguide and propagate towards equator to be received at low-latitude station Jammu. To understand the generation mechanism of ELF/VLF hiss, incoherent Cerenkov radiated power from the low-latitude and mid-latitude plasmasphere are evaluated. Considering this estimated power as an input for wave amplification through wave–particle interaction, the growth rate and amplification factor is evaluated which is too small to explain the observed wave intensity. It is suggested that some non-linear mechanism is responsible for the generation of ELF/VLF hiss.  相似文献   
33.
作者在辽东地区把甚低频(VLF)法应用于金矿、硼镁铁矿、铜矿、钼矿和煤矿的普查勘探工作中。通过6个矿区,9条VLF剖面的测量,发现VLF法在固体矿产普查中异常显著,并与已知矿体吻合,找矿效果较好。应用VLF法不公可以发现良导体矿,而且可以确定矿体的产状、规模和矿体叠加状态。VLF法应用于普查表层矿产,其效果更为显著。  相似文献   
34.
本文利用搭载在DEMETER卫星上的感应式磁力仪(Instrument Magnetometer Search-Coil,IMSC)探测数据分析了磁场甚低频(Very Low Frequency,VLF)波功率谱的空间分布.在排除地磁扰动影响(Dst≤-30 nT,Kp≥3,AE≥200 nT)的前提下,我们给出200...  相似文献   
35.
电离层人工调制激发的下行ELF/VLF波辐射   总被引:2,自引:2,他引:0       下载免费PDF全文
常珊珊  赵正予  汪枫 《地球物理学报》2011,54(10):2458-2467
通过大功率ELF/VLF调幅高频波对电离层进行加热,形成电离层虚拟天线,可以作为发射ELF/VLF波的一种有效手段.本文使用汪枫(2009)的调制加热模型,计算高频加热电离层产生的低频辐射源强度,采用全波解算法分析辐射的低频波向下传播过程中的衰减和反射问题,并采用HAARP实验参数,模拟出在海面上接收到的低频信号强度为...  相似文献   
36.
以内蒙古敖汉旗小四家萤石矿的勘查为例,在地质研究的基础上,对小四家隐伏萤石矿体进行甚低频和EH-4测量,结果表明甚低频和EH-4的组合使用在隐伏萤石矿体的勘查中效果明显,甚低频测量能够快速确定构造低阻带平面延伸规律,EH4测量能够清晰显示构造低阻带深部展布形态,两者组合使用可以达到优势互补的目的,为下一步勘探提供科学依据。  相似文献   
37.
玉树地震前电离层VLF信号信噪比变化   总被引:1,自引:0,他引:1       下载免费PDF全文
2010年4月13日23点49分38秒(世界时),青海省玉树县发生了Ms7.1地震.根据法国DEMETER卫星电场探测仪(ICE)实验数据,研究震区上空半径500 km范围内电离层10-20 kHz甚低频(VLF)电场频谱信噪比发现,玉树地震前3个不同频率的地面VLF发射站信号对应的信噪比均出现相同的变化特征,即震前DEMETER卫星1个重访周期内的平均信噪比明显减弱,而2009年相同时段和区域的平均信噪比并未出现相似变化趋势.分析认为,玉树地震孕震期信噪比衰减现象很可能是由地震-电离层耦合所致.  相似文献   
38.
In order to estimate the dynamic structure of the VLF ionospheric exit point, we conducted multipoint ground-based observation of the natural VLF emissions at three unmanned sites: West Ongul (69°01′ S, 39°30′ E), Skallen (69°40′ S, 39°24′ E), and H100 (69°18′ S, 41°19′ E) around Japanese Syowa station, Antarctica, during a whole year of 2006. In this observation, we developed three sets of unmanned autonomous observation systems for natural VLF emissions. Each observation system consists of two crossed vertical loop antennas to pick-up North–South (NS) and East–West (EW) magnetic components, a multi-channel analyzer, and a data logger. The intensity and polarization of NS and EW magnetic components are obtained in 4 spaced frequency (0.5, 1.0, 2.0, and 6.0 kHz) channels by the multi-channel analyzer.The VLF emissions observed at the three sites exhibit an interesting difference in the wave intensity as well as the polarization that allows important information about the locations of their ionospheric exit point to be determined. Firstly, to find the distinct exit point, we have theoretically calculated the spatial distributions of the wave intensity and the polarization on the Earth for VLF whistler mode waves coming down from the magnetized ionosphere, by using the full-wave analysis. Then, we have compared the calculated results with the observed data, to evaluate the possible locations of the ionospheric exit point for the auroral hiss events.As an example, the direction of the estimated ionospheric exit point for the auroral hiss event at 31 March 2006 was found to be consistent with a bright aurora region. However, in this case, the estimated ionospheric exit point was located a few hundred kilometers equatorward of the associated aurora. This would suggest that the ray paths for the auroral hiss could be different from the directions of the geomagnetic field lines for auroral precipitation.  相似文献   
39.
利用2005—2010年DEMETER卫星记录NWC发射站的19.8kHz电场功率谱数据,采用统计和线性拟合等方法,研究了NWC站发射的电磁波在顶部电离层及磁共轭区激发的电场效应及其在不同方位的衰减特性。结果发现:(1)在NWC发射站上空,卫星记录电场呈椭圆状扩散分布,电场最强中心点位置相对地面人工源位置有一定偏移;(2)研究区上空电场北部衰减梯度最小,东部衰减梯度最大;(3)在其磁共轭区,南部电场衰减梯度最小,北部衰减梯度最大。综合分析认为人工源(NWC)发射的VLF电磁波传播到电离层高度后,受地磁场影响,电磁波主要沿磁力线方向传播,空间电场最强中心点位置相对发射站的位置发生偏移,向磁赤道方向倾斜,而且偏于磁赤道方向的电场衰减梯度最小。  相似文献   
40.
《Geofísica Internacional》2014,53(2):135-151
There are about 175 abandoned mining sites in Portugal, of which about 60 are old uranium workings. The Castelejo mine is an old uranium located about 2 km W of Vila Cortês da Serra, in Guarda district, on the River Mondego basin. In geologic terms, the mine is located in medium-grained two-mica monzonitic granite, with porphyroidal tendency. Exploitation started with two open cast mines between 1979 and 1990 which produced about 132 tonnes U3O8. From 1992, production started to be carried out through the in situ H2SO4 leaching of the mine’s low-grade materials. The superficial and groundwater circulation are structurally conditioned by the intense fracturing in the area. Two exploratory geophysical field campaigns were conducted in order to characterize the fracturing. The first was a VLF survey that allowed us to identify major fault systems that may provide paths for groundwater flow. From the second campaign, which was an RMT survey conducted at a fault gauge which records the mine natural gradient flow, we obtained the resistivities and thicknesses of the weathered granite material. The profiles obtained show that resistivity declines with increasing depth. This fact may arise from natural causes – the material which fills the fault gauge is more weathered at depth than on the surface – or it may indicate contamination at depth, due to acid mine drainage.  相似文献   
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