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The Effect of Heavy Inclusions in the Upper Crust on Thermoconvective Instability of the Lithosphere 上地壳重包裹体对岩石圈热凸不稳定性的影响
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700411
B. I. Birger

The method of linear theory for small perturbations is used to study the stability of heavy inclusions in the upper crust. The existence of such inclusions of increased density is associated with chemical heterogeneity or phase transitions. At small deformations considered in the linear stability theory, the material undergoes transient creep which is described by the Andrade rheological model. With this rheology, the convective instability of thickened segments of the lithosphere is oscillatory: the increment is a complex number with a real part close to zero (threshold instability). Heavy inclusions in the upper crust introduce a small complex correction to the increment that determines the convective instability of the lithosphere, slightly increasing the real and imaginary parts of the increment, enhancing the instability and increasing the oscillation frequency.

摘要 小扰动线性理论方法用于研究上地壳重包裹体的稳定性。这种密度增大的包裹体的存在与化学异质性或相变有关。在线性稳定性理论考虑的小变形情况下,材料会发生安德拉德流变模型描述的瞬态蠕变。根据这种流变学原理,岩石圈增厚段的对流不稳定性是振荡的:增量是一个实部接近于零的复数(阈值不稳定性)。上地壳中的重包裹体对决定岩石圈对流不稳定性的增量引入了一个小的复数修正,略微增加了增量的实部和虚部,增强了不稳定性并提高了振荡频率。
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引用次数: 0
On Constructing of Magnetic and Gravity Images of Mercury from Satellite Data 根据卫星数据构建水星的磁力和重力图像
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700459
I. E. Stepanova, A. G. Yagola, D. V. Lukyanenko, I. I. Kolotov

Abstract—A new technique for simultaneous construction of the “gravity” and “magnetic” images of Mercury from satellite data based on the regional version of the S approximation is proposed. The mathematical statement of the inverse problem of finding the images of a planet from the data on the potential fields recorded at different instants with different degrees of accuracy is reduced to solving ill-conditioned systems of linear algebraic equations (SLAE) with approximate right-hand sides. Based on the analytical approximations of the mercury magnetic and gravity fields determined from the solution of the ill-conditioned SLAE, the distributions of the equivalent sources on the spheres are determined. The results of the mathematical experiment on constructing the magnetic image of Mercury from the radial component of the magnetic induction vector continued analytically to the field sources are presented.

摘要 根据区域版 S 近似值,提出了从卫星数据同时构建水星 "重力 "和 "磁力 "图像的新技术。从不同时刻记录的不同精确度的势场数据中寻找行星图像的逆问题的数学表述被简化为求解具有近似右边的无条件线性代数方程组(SLAE)。根据由非条件线性代数方程求解确定的汞磁场和重力场的分析近似值,确定了等效源在球体上的分布。介绍了根据磁感应矢量的径向分量继续分析场源构建水星磁图像的数学实验结果。
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引用次数: 0
Prediction Results for the Strongest Earthquakes of February 6, 2023 in Southern Turkey 2023 年 2 月 6 日土耳其南部最强烈地震的预测结果
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700423
A. I. Gorshkov, V. G. Kossobokov, O. V. Novikova

Abstract—On February 6, 2023, two devastating earthquakes struck southern central Turkey, nine hours apart. The ground shaking from these earthquakes even swept over a significant part of northwestern Syria. In this paper, we consider the locations of the epicenters of these earthquakes against the prediction of the М ≥ 6.5 earthquake epicenters in Anatolia and adjacent regions, which was made in 1973 by I.M. Gelfand, V.I. Keilis-Borok and their colleagues using the Kora-3 pattern recognition algorithm based on morphostructural zoning data. We also present the results of early detection of the periods with an increased probability of the strongest earthquakes as determined by the medium-term prediction algorithm for the M8 earthquakes. It is found that the epicenters of the February 6, 2023 earthquakes occurred in a node identified in 1973 as potentially earthquake-prone for М ≥ 6.5, and both events occurred within the spatial and temporal coverage of the warning area diagnosed by the M8 algorithm in July 2021.

摘要--2023 年 2 月 6 日,土耳其中南部相隔 9 个小时发生了两次毁灭性地震。地震引起的地面震动甚至席卷了叙利亚西北部的大部分地区。1973 年,I.M. Gelfand、V.I. Keilis-Borok 及其同事使用基于形态结构区划数据的 Kora-3 模式识别算法,对安纳托利亚及邻近地区的 М≥ 6.5 级地震震中进行了预测。我们还介绍了根据 M8 地震中期预测算法确定的强震发生概率增加时期的早期检测结果。结果发现,2023 年 2 月 6 日地震的震中发生在 1973 年确定的可能发生 М≥ 6.5 地震的节点上,并且这两次地震都发生在 2021 年 7 月 M8 算法所诊断的预警区域的时空覆盖范围内。
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引用次数: 0
Seismic Pulses before the February 27, 2010 M = 8.8 Chile Earthquake 2010 年 2 月 27 日 M = 8.8 智利地震前的地震脉冲
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700447
G. A. Sobolev, I. N. Migunov

Abstract—We study the records of ground motion vertical velocity in the vicinity of broadband seismic stations on the west coast of South America and in the adjacent region of the Pacific Ocean, where the Mw 8.8 earthquake occurred on February 27, 2010. Starting from 2009, asymmetric seismic pulses lasting several hundred seconds have been detected in records of some stations. These pulses occurred under quiet weather conditions and low geomagnetic activity. It is believed that the earthquake was preceded by tectonic movements in the oceanic and continental lithosphere.

摘要--我们研究了 2010 年 2 月 27 日发生 8.8 级地震的南美洲西海岸和太平洋邻近地区宽带地震台站附近的地动垂直速度记录。从 2009 年开始,在一些台站的记录中发现了持续数百秒的不对称地震脉冲。这些脉冲发生在安静的天气条件和地磁活动较低的情况下。据信,地震发生前,海洋和大陆岩石圈发生了构造运动。
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引用次数: 0
Technology of Mapping of Volcanic-Sedimentary Strata in a Complexly Dislocated Terrigenous Structure according to Seismic and Magnetic Exploration Data (Pechora Sea) 根据地震和磁力勘探数据绘制复杂错位陆相结构中的火山沉积地层图的技术(佩乔拉海)
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700496
I. V. Lygin, T. B. Sokolova, L. N. Kleschina, K. M. Kuznetsov, V. A. Nikitina, T. P. Shirokova, K. V. Krivosheya, K. S. Chernikov, A. V. Mazekina

The geological efficiency of seismic exploration and, as a result, the reliability of structural constructions in areas of intense tectonic dislocations (normal, reverse and thrust faults) is significantly reduced. At the same time, it is in such areas, that the presence of lithostratigraphic complexes contrasting in density or magnetic properties in the section and the abundance of subvertical boundaries provide prerequisites for the successful use of potential field methods (gravity exploration, magnetic exploration) to verify and supplement the structural interpretation of seismic exploration data. The paper presents the technology of complex interpretation of magnetic and seismic exploration data, tested on one of the objects of the Pechora Sea. In the course of the research, the connection of local magnetic anomalies with the seismic structural plan was established, which made it possible to identify and trace a magnetically active complex in the sedimentary strata with parameters typical of volcanogenic sedimentary rocks, weakly contrasting in seismic records. As a result of 3D modeling, the morphology of the roof and the base of the magnetic layer were determined, and the three-dimensional distribution of magnetization was calculated. It is proved that the sources of local magnetic field anomalies, a priori considered as isolated intrusive massifs, are associated with the distribution of magnetization within a single stratified volcanogenic-sedimentary strata. The obtained result was used in the construction of an updated geological and geophysical model. The developed technology is recommended as one of the promising approaches for building seismomagnetic models in similar physical and geological situations.

摘要 在构造错动(正断层、逆断层和推断断层)强烈的地区,地震勘探的地质效率大大降低,因此,构造构建的可靠性也大大降低。同时,正是在这些地区,剖面上存在密度或磁性对比强烈的岩石地层复合体,以及丰富的地下边界,为成功使用潜在的野外方法(重力勘探、磁力勘探)验证和补充地震勘探数据的构造解释提供了先决条件。本文介绍了磁力和地震勘探数据复合解释技术,并在佩乔拉海的一个对象上进行了测试。在研究过程中,建立了局部磁异常与地震结构图之间的联系,从而可以确定并追踪沉积地层中的磁活动复合体,其参数为火山沉积岩的典型参数,在地震记录中对比较弱。通过三维建模,确定了磁层顶部和底部的形态,并计算了磁化的三维分布。结果证明,先验地认为是孤立的侵入地块的局部磁场异常源与单一层状火山成因沉积地层内的磁化分布有关。获得的结果被用于构建最新的地质和地球物理模型。建议将所开发的技术作为在类似物理和地质情况下建立地震地磁模型的可行方法之一。
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引用次数: 0
Shear Trough Depth and Geometry Relation Determined from Satellite Radar Images from One or Two Orbits 从一个或两个轨道的卫星雷达图像确定剪切槽深度和几何关系
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700514
I. P. Babayants, V. O. Mikhailov, E. P. Timoshkina, A. A. Baryakh

Abstract—The subsidence of the Earth’s surface, calculated from the theoretical model of a shear trough above a longwall developed by pillar and room caving are compared with displacements that can be estimated from trough monitoring using satellite images acquired from a single and two orbits. It is shown that the transverse and longitudinal axes of the trough do not shift when subsidence is calculated using data from descending and ascending orbits together. The maximum subsidence magnitude is determined almost without error. Errors in the reconstruction of the trough geometry appear where there is a significant northern displacement component, which, due to the characteristics of satellite radar imaging, is usually neglected. For the north‒south and west‒east trending troughs, these are their northern and southern boundaries; and for a trough trending from northwest to southeast, these are its northernmost and southernmost corners. In the maps of displacements in the direction towards the satellite (Line-of-Sight displacements, LOS), as well as in the subvertical displacement maps Usubv calculated using images from a single orbit, assuming that horizontal surface displacements are much smaller than vertical ones, the subsiding and uplifting areas are always shifted towards the satellite. Namely, in the displacement maps based on satellite images acquired from ascending and descending orbits these areas are always shifted to the west and east, respectively. The displacement magnitude is 50–60 m. The displacement direction of the longitudinal and transverse axes of the trough in the maps of subvertical displacements Usubv depends on their strike. The displacements of the trough axes relative to their real ground position should be taken into account when estimating the location of a shear trough from the maps Usubv of subvertical displacements derived from images from one orbit. In these maps, the maximum subsidence magnitude is approximately 10% larger than the displacements calculated from the trough model.

摘要 通过柱洞和房间洞室发育的长壁上方剪切槽理论模型计算出的地球表面下沉量,与利用单轨道和双轨道获取的卫星图像进行槽监测估算出的位移量进行了比较。结果表明,当同时使用下降轨道和上升轨道的数据计算沉降时,槽的横轴和纵轴不会移动。最大下沉幅度的确定几乎没有误差。由于卫星雷达成像的特点,通常会忽略显著的北部位移分量,因此在重建海槽几何形状时会出现误差。对于南北走向和西东走向的海槽来说,这是其北部和南部的边界;而对于西北至东南走向的海槽来说,这是其最北端和最南端的角落。在朝向卫星方向的位移图(视线位移图,LOS)中,以及在利用单一轨道图像计算的亚垂直位移图 Usubv 中,假定水平表面位移远小于垂直位移,下沉和隆起区域总是向卫星方向移动。也就是说,在根据从上升轨道和下降轨道获取的卫星图像绘制的位移图中,这些区域总是分别向西和向东移动。在亚倾覆位移图 Usubv 中,海槽纵轴和横轴的位移方向取决于其走向。在根据一个轨道上的图像绘制的俯冲位移图 Usubv 估算剪切槽位置时,应考虑到槽轴相对于其实际地面位置的位移。在这些地图中,最大下沉幅度比根据海槽模型计算出的位移大约大 10%。
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引用次数: 0
Investigation of the Lithospheric Plate Boundary Zone within the Sakhalin Island Based on Satellite Geodesy Data 基于卫星大地测量数据的萨哈林岛内岩石圈板块边界带调查
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700526
M. S. Gridchina, G. M. Steblov, I. S. Vladimirova, A. V. Basmanov

Modelling of the movements at the interface of the Amur and Okhotsk plates within the Sakhalin Island was performed using repeated satellite measurements on the Sakhalin Island and the nearest continental zone for the period of 2016–2021, as well as previously published data. When modelling fault-block kinematics, well-known relations were used to calculate reverse movements for buried rectangular dislocations in an elastic medium, which were implemented in the TDEFNODE software package. In the process of modelling the movements, the measured horizontal components of GNSS (Global Navigation Satellite System) velocities, the boundary and the mutual kinematics of the Amur and Okhotsk plates relative to the North American Plate according to the NNR-MORVEL56 model were used as the input data. This approach revealed persistent deviations in the direction of the simulated displacements of the Earth’s surface from the observed ones, which can be explained by the discrepancy between the a priori specified kinematics of the blocks and the observed movements. To eliminate the systematic discrepancy, it was necessary to allow the possibility of updating the mutual kinematics of the blocks. The repeated calculations, with the same input data but in a problem formulation that allowed refinement of block kinematics, led to suppression of systematic discrepancies between the model and measured displacements while retaining the random scatter. The movement parameters of the Amur and Okhotsk plates, which were refined during the modelling, show typical slight differences from the movement parameters of the corresponding large lithospheric plates (the Eurasian and North American plates), from which they are separated into independent blocks in modern constructions. The calculated locking coefficients in the Sakhalin segment of the interplate boundary reach maximal values at depths of 20–30 km. The obtained locking pattern at the plate interface is compared with the sources of the largest earthquakes in the last 30 years in the considered area, viz., Neftegorsk (May 27, 1995) and Uglegorsk (April 4, 2000) earthquakes, which are found to be associated with zones of maximal locking and a high locking gradient, both in the dip and strike directions.

摘要-利用 2016-2021 年期间对萨哈林岛和最近大陆区域的重复卫星测量数据以及之前公布的数据,对萨哈林岛内阿穆尔板块和鄂霍次克板块交界面的运动进行了建模。在建立断层块运动学模型时,使用了众所周知的关系来计算弹性介质中埋藏的矩形位错的反向运动,这些关系已在 TDEFNODE 软件包中实现。在建立运动模型的过程中,使用了根据 NNR-MORVEL56 模型测得的全球导航卫星系统(GNSS)速度水平分量、阿穆尔板块和鄂霍次克板块相对于北美板块的边界和相互运动学作为输入数据。这种方法揭示了地球表面模拟位移方向与观测到的位移方向之间的持续偏差,这可以用先验地指定的板块运动学与观测到的运动之间的差异来解释。为了消除系统性差异,有必要允许更新块体的相互运动学。使用相同的输入数据进行重复计算,但在问题表述中允许细化木块运动学,从而抑制了模型与测量位移之间的系统性差异,同时保留了随机散点。在建模过程中完善的阿穆尔板块和鄂霍次克板块的运动参数与相应的大型岩石圈板块(欧亚板块和北美板块)的运动参数有典型的细微差别,在现代构造中,它们被分成独立的区块。计算得出的板块间边界萨哈林段锁定系数在 20-30 千米深处达到最大值。所获得的板块交界处的锁定模式与该地区过去 30 年最大地震(即涅夫特戈尔斯克地震(1995 年 5 月 27 日)和乌格列戈尔斯克地震(2000 年 4 月 4 日))的震源进行了比较,发现这两个地震与最大锁定区以及在倾角和走向方向上的高锁定梯度有关。
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引用次数: 0
Meteorological Anomalies and Strong Earthquakes: A Case Study of the Petropavlovsk-Kamchatsky Region, Kamchatka Peninsula 气象异常与强烈地震:堪察加半岛彼得罗巴甫洛夫斯克-堪察加地区案例研究
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700502
G. N. Kopylova, Yu. K. Serafimova, A. A. Lyubushin

Abstract— Long-term (1962‒2020) observations of air temperature and atmospheric pressure at two weather stations in the region of Petropavlovsk-Kamchatsky, Kamchatka Krai, are analyzed to examine the hypotheses about a connection between increased and decreased meteorological parameter values and their contrasting changes with a final stage of preparation of local Kamchatka earthquakes with magnitudes 5.2‒8.3, which occurred at epicentral distances of 22–440 km and caused perceptible shaking with intensity IMSK-64 ≥ 4–5. To identify meteorological anomalies, we used an empirical method comparing daily mean air temperatures and atmospheric pressures with daily averages of their annual seasonal-mean functions and a formalized method estimating the minimum normalized entropy En, the logarithm of the curtosis coefficient logκ, and the autoregressive measure of nonstationarity Q2 of the time series of air temperature and atmospheric pressure in a moving time window with a length of 112 days shifted by one day. Various types of meteoanomalies before earthquakes were studied on time intervals of seven and 30 days. The correlation between the detected anomalies and subsequent earthquakes was evaluated from the ratio of reliability and validity of the conditional meteorological precursor. It is found that the manifestation of various types of meteorological anomalies before earthquakes is mainly of a random nature. The lack of a pronounced correlation between air temperature increases and subsequent earthquakes casts doubt on the reality of the mechanism of generation of thermal surface anomalies before earthquakes in the lithosphere‒atmosphere‒ionosphere‒magnetosphere coupling (LAIMC) model for the study region. The methods used for meteorological data analysis can be applied in seismic forecasting in the region of the Petropavlovsk-Yelizovo agglomeration, Kamchatka Krai, for diagnosing weather-dependent anomalies in the changes of the ground-based observation data.

摘要-- 对堪察加边疆区彼得罗巴甫洛夫斯克-堪察加地区两个气象站的气温和大气压力的长期(1962-2020 年)观测数据进行了分析,以研究气象参数值的增减与堪察加当地 5.2-8.3 级地震最后准备阶段的对比变化之间的联系。为了识别气象异常,我们使用了一种经验方法,将日平均气温和大气压力与它们的年季节平均函数的日平均值进行比较;还使用了一种正规化方法,在一个长度为 112 天的移动时间窗口中,估计气温和大气压力时间序列的最小归一化熵 En、熵系数 logκ 对数以及自回归非平稳性度量 Q2。在 7 天和 30 天的时间间隔内研究了地震前的各类气象异常。根据条件气象前兆的可靠性和有效性比率,评估了检测到的异常现象与随后发生的地震之间的相关性。研究发现,地震前各类气象异常的表现主要具有随机性。气温上升与随后的地震之间缺乏明显的相关性,这使人们对研究区域岩石圈-大气层-电离层-磁层耦合(LAIMC)模型中地震前地表热异常产生机制的真实性产生怀疑。用于气象数据分析的方法可用于堪察加边疆区彼得罗巴甫洛夫斯克-叶利佐沃聚集区的地震预报,以诊断地面观测数据变化中与天气有关的异常现象。
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引用次数: 0
What Does the Archaeomagnetic Record of Fired Ceramics Reflect? 烧制陶瓷的考古磁记录反映了什么?
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700435
O. V. Pilipenko, G. P. Markov, N. V. Salnaya, P. A. Minaev, N. A. Aphinogenova

Abstract—A complex of archaeomagnetic and rock magnetic studies is conducted to compare the archaeomagnetic intensity determined by the Thellier–Coe and Wilson methods with the known “true” value of the geomagnetic field during the firing of the ceramic samples manufactured on February 21, 2017 in the town of Myshkin (Yaroslavl oblast, Russia). The results obtained show two different values of archaeomagnetic intensity corresponding to two temperature intervals. The archaeomagnetic intensity estimated from the low-temperature interval (~150–350°C) are approximately 13 μT lower than the true value, while the values obtained in the interval of ~350–600°C are fairly close to the “true” ones. The cause of the phenomenon is likely due to the presence of small magnetic grains in the ceramic under study, which are close in size to superparamagnetic ones and can resume their growth upon heating and reaching a particle size in a single-domain state. The results of rock magnetic studies suggest that thermoremanent magnetization in the studied ceramics is carried by grains of oxidized magnetite, hematite, and possibly ε-Fe2O3.

摘要 开展了一项考古磁学和岩石磁学的综合研究,以比较 2017 年 2 月 21 日在 Myshkin 镇(俄罗斯雅罗斯拉夫尔州)烧制陶瓷样品期间用 Thellier-Coe 和 Wilson 方法确定的考古磁强度与已知的地磁场 "真实 "值。获得的结果显示了与两个温度区间相对应的两个不同的古地磁强度值。低温区间(约 150-350°C)估算出的考古磁强度比真实值低约 13 μT,而在约 350-600°C 区间获得的值则相当接近 "真实 "值。造成这种现象的原因可能是所研究的陶瓷中存在小磁粒,这些小磁粒的尺寸接近超顺磁性磁粒,在加热后可恢复生长,并达到单域状态的粒度。岩石磁性研究结果表明,所研究陶瓷中的热永磁是由氧化磁铁矿、赤铁矿和可能的 ε-Fe2O3 晶粒携带的。
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引用次数: 0
Chetdin Radon Anomaly (Komi Republic): Localization and Study 切丁氡异常点(科米共和国):定位与研究
IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS Pub Date : 2024-07-18 DOI: 10.1134/S1069351324700484
Yu. E. Ezimova, V. V. Udoratin, A. Sh. Magomedova

When studying the fault tectonics of the Vychegodskii trough, we detected an area of high concentrations of soil radon, confined to the zone of the Vychegda–Lokchim fault. To localize the radon anomaly, we carried measurements of the volumetric radon activity out over a network of observation points. Air sampling at each point was performed from the wellhead with a depth of 0.5 m and a diameter of 0.1 m. Based on the data obtained, an intense radon anomaly was contoured. At different times, the anomaly changed in the size, shape, and intensity, but its center always remained fixed. According to areal observations, in the central part of the 2 × 2-km anomaly, the radon concentration reached 3800–4800 Bq/m3. The results of continuous daily monitoring in the center of the anomaly showed that the of radon concentration is subject to daily dynamics, which directly depends on meteorological parameters, namely on temperature and humidity. At night, with a decrease in temperature and an increase in air humidity, the level of radon increased to 6000–8000 Bq/m3 on average, in rare cases up to 10 000–12 000 Bq/m3. In the daytime, with an increase in temperature, a decrease in the volumetric radon activity was noted. In addition to the daily dynamics, seasonal variability of the radon field was observed. In autumn, the radon concentration is lower than in summer, which is associated with short-term precipitation and, as a result, the filling of the pore space with water. The Archean–Early Proterozoic basement composed of gneisses, amphibolites, quartzites, and migmatites at a depth of 2 km is considered as the main source of radon. Due to the fact that the anomaly is located in the zone controlled by the Vychegda–Lokchim fault, the latter is considered the main pathway for fluid transport to the surface.

摘要--在研究 Vychegodskii 海槽的断层构造时,我们发现了一个土壤氡浓度较高的区域,该区域仅限于 Vychegda-Lokchim 断层区。为了确定氡异常点的位置,我们通过观测点网络对氡活动的体积进行了测量。每个观测点的空气采样都是从井口开始,深度为 0.5 米,直径为 0.1 米。在不同时期,异常点的大小、形状和强度都会发生变化,但其中心始终保持固定。根据区域观测,在 2 × 2 千米异常点的中心区域,氡浓度达到 3800-4800 Bq/m3 。对异常点中心的每日连续监测结果表明,氡浓度受每日动态变化的影响,这直接取决于气象参数,即温度和湿度。在夜间,随着温度的降低和空气湿度的增加,氡浓度平均上升到 6000-8000 Bq/m3,在极少数情况下上升到 10 000-12 000 Bq/m3。在白天,随着温度的升高,氡活度的体积有所减少。除了日常动态变化外,还观察到氡场的季节性变化。秋季的氡浓度低于夏季,这与短期降水有关,因此孔隙中充满了水。由片麻岩、闪长岩、石英岩和岩浆岩组成的、深度为 2 千米的奥长安-早新生代基底被认为是氡的主要来源。由于异常点位于 Vychegda-Lokchim 断层控制区,后者被认为是流体向地表输送的主要通道。
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引用次数: 0
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Izvestiya, Physics of the Solid Earth
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