湘黔桂新元古代拉伸纪晚期地层年代格架对比及关键地质事件初探     

张嘉玮  陈建书  吴滔  叶太平  陈明华  代雅然  邓小杰  牟军 《地学前缘》2020,27(4):1-16

湘黔桂地区发育一套完整的新元古代拉伸纪晚期地层(下江群及其相当地层),是研究扬子克拉通与华夏板块碰撞拼接后华南大陆裂谷盆地演化的重要载体。本文报道了贵州省铜仁市万山区清水江组上部、平略组底部及中部变质凝灰岩和沉凝灰岩的年龄,分别为(763.8±5.5) Ma(N=24,MSWD=0.29)、(760.2±4.1) Ma(N=25,MSWD=0.39)、(759.1±3.9) Ma(N=26,MSWD=0.38)。通过对湘黔桂地区下江群及其相当地层中已有火山岩、火山碎屑沉积岩、含凝灰质岩石年龄的系统梳理与分析研究,进一步确定下江群其及相当地层的沉积时限在822~715 Ma,桂北丹洲群三门街组玄武岩是在武陵造山后伸展背景下湘黔桂地区裂谷最大裂陷时期的产物,清水江组与平略组内大量的火山物质可能来源于江南造山带东段800~760 Ma的中酸性喷出岩。结合地层、岩性、年代特征,本文恢复了湘黔桂盆地新元古代拉伸纪晚期的演化历史,并认为该套地层符合建立下江系条件。  相似文献   

Classification of Harmonic Functions in the Exterior of a Unit Sphere and Its Application to the Description of the External Magnetic Field of the Earth     

Akhmet’ev  P. M.  Petrov  A. V. 《Geomagnetism and Aeronomy》2019,59(6):752-760

Geomagnetism and Aeronomy - The magnetic fields of a subterranean source observed on the Earth’s surface or from the orbit of a satellite are studied. We analyze the space of all harmonic...  相似文献   

The Oldest Vendian (Ediacaran) Fossils of Eurasia: U–Pb Isotope Age of the Basa Formation (Asha Group,Southern Urals)     

Razumovskiy  A. A.  Novikov  I. A.  Ryazantsev  A. V.  Rud’ko  S. V.  Kuznetsov  N. B.  Yashunskiy  Yu. V. 《Doklady Earth Sciences》2020,495(2):867-871

Doklady Earth Sciences - U–Th–Pb (SHRIMP II) isotopic dating of accessory zircons from Vendian (Ediacaran) ash tuffs of the Basa formation section (Asha Group, Southern Ural) was...  相似文献   

Ionosphere Disturbances Preceding Earthquakes according to the Data of Ground Based Station of the Vertical Ionospheric Sounding Wakkanai   总被引：1，自引：0，他引：1  

S. A. Pulinets  A. D. Legen’ka  V. V. Hegai  V. P. Kim  L. P. Korsunova 《Geomagnetism and Aeronomy》2018,58(5):686-692

The paper analyzes the data of manual ionograms processing of hourly measurements of the critical frequency foF2 of the F2 ionospheric layer at the Wakkanai ionospheric vertical sounding station (Japan) in a geomagnetically quiet environment before a series of earthquakes with magnitude M > 6.0, for which the station entered the earthquake preparation zone, in order to detect possible Ionospheric Disturbances Preceding Earthquakes (IDPE), and to determine their quantitative characteristics. Detected IDPE, in the opinion of the authors, can be related to the processes of preparation of the corresponding earthquakes, i.e., to be Ionospheric Precursors of Earthquakes (IPE).  相似文献   

Motion of Ionospheric Plasma: Results of Observations above Kharkiv in Solar Cycle 24     

L.?Ya.?Emel’yanovEmail author  M.?V.?Lyashenko  L.?F.?Chernogor  I.?F.?Domnin 《Geomagnetism and Aeronomy》2018,58(4):533-547

The equipment and methodical characteristics of determining the vertical component of the ionospheric plasma motion velocity V_z based on an incoherent scatter radar of Institute of Ionosphere, National Academy of Sciences and Ministry of Education and Science of Ukraine (Kharkiv), which is the only radar of such type in Central Europe, are described. Based on the radar data, the patterns of altitude and diurnal variations in V_z near the maximum of solar cycle 24 for the typical geophysical conditions (around the summer and winter solstices, the spring and fall equinoxes) at low geomagnetic activity and the specifics of these changes during ionospheric storms are presented. The results of modeling of the dynamic processes in ionospheric plasma under the conditions of the undisturbed ionosphere, including the determination of altitudetime variations in the thermospheric wind velocity, are presented. It has been established that this velocity can significantly differ from the thermospheric wind velocity calculated by the known empirical global models. This difference is likely related to the regional features of thermospheric wind that are not shown in the global models.  相似文献   

Reconstruction of Centennial Series of Solar Activity     

Tlatova  K. A.  Vasil’eva  V. V.  Skorbezh  N. N.  Illarionov  E. A.  Tlatov  A. G. 《Geomagnetism and Aeronomy》2018,58(8):1021-1028

Geomagnetism and Aeronomy - The results of the digitalization of the centennial series of solar activity are considered. The data contain information on sunspots since 1918, sunspot umbra since...  相似文献   

Dispersion features of transmitted channel waves and inversion of coal seam thickness     

Ze’an Hu  Pingsong Zhang  Guangquan Xu 《Acta Geophysica》2018,66(5):1001-1009

In-seam seismic survey currently is a hot geophysical exploration technology used for the prediction of coal seam thickness in China. Many studies have investigated the relationship between the group velocity of channel wave at certain frequency and the actual thickness of exposed coal beds. But these results are based on statistics and not universally applicable to predict the thickness of coal seams. In this study, we first theoretically analyzed the relationship between the depth and energy distribution of multi-order Love-type channel waves and found that when the channel wave wavelength is smaller than the thickness of the coal seam, the energy is more concentrated, while when the wavelength is greater than the thickness, the energy reduces linearly. We then utilized the numerical simulation technology to obtain the signal of the simulated Love-type channel wave, analyzed its frequency dispersion, and calculated the theoretical dispersion curves. The results showed that the dispersion characteristics of the channel wave are closely related to the thickness of coal seam, and the shear wave velocity of the coal seam and its surrounding rocks. In addition, we for the first time realized the joint inversion of multi-order Love-type channel waves based on the genetic algorithm and inversely calculated the velocities of shear wave in both coal seam and its surrounding rocks and the thickness of the coal seam. In addition, we found the group velocity dispersion curve of the single-channel transmitted channel wave using the time–frequency analysis and obtained the phase velocity dispersion curve based on the mathematical relationship between the group and phase velocities. Moreover, we employed the phase velocity dispersion curve to complete the inversion of the above method and obtain the predicted coal seam thickness. By comparing the geological sketch of the coal mining face, we found that the predicted coal seam thickness is in good agreement with the actual thickness. Overall, adopting the channel wave inversion method that creatively uses the complete dispersion curve can obtain the shear wave velocities of the coal and its surrounding rocks, and analyzing the depth of the abruptly changed shear wave velocity can accurately obtain the thickness of the coal seam. Therefore, our study proved that this inversion method is feasible to be used in both simulation experiments and actual detection.  相似文献   

Study of Lateral Sedimentation in the Western Atlantic on Cruise 53 of the R/V Akademik Ioffe     

Ivanova  E. V.  Murdmaa  I. O.  Borisov  D. G.  Ovsepyan  E. A.  Simagin  N. V.  Mutovkin  A. D.  Nemchenko  N. V.  Kornilova  M. O.  Sud’in  V. V.  Novikov  Yu. V. 《Oceanology》2018,58(6):932-934

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On Increasing the Accuracy of Star Trackers to Subsecond Levels     

A. I. Zacharov  N. L. Krusanova  I. V. Moskatiniev  M. E. Prohorov  O. Y. Stekol’shchikov  V. K. Sysoev  M. S. Tuchin  A. D. Yudin 《Solar System Research》2018,52(7):636-643

Modern star trackers are based on photodetector arrays such as CCD or CMOS arrays. The accuracy of commercially available devices is ~1–3 arcseconds. However, the development of the space industry calls for higher orientation accuracies, which are needed in laser space communications, monitoring of near-Earth space and space debris, high-precision global mapping, and remote sensing of the Earth. The problems associated with enhancing the accuracy of modern star trackers are discussed.  相似文献   

Determination of Non-gravitational Effects in the Motion of Near-Sun Objects 321P, 322P, 323P,and 342P     

V.?V.?Emel’yanenkoEmail author  S.?A.?Naroenkov 《Solar System Research》2018,52(1):64-68

At the beginning of this century, the SOHO space observatory discovered near-Sun comets with perihelion distances q ≈ 0.05 AU, which remained observable over several close encounters with the Sun. This became one of the surprises in studying the small bodies of the Solar System. Currently, there are objects that have already been observed in four (342P) and five (321P, 322P, and 323P) apparitions. In the present work, the estimates of nongravitational effects are obtained for these objects based on the pair-wise linkage of the apparitions. The calculations show that the observations of these objects are poorly represented if solely the gravitational forces are considered. The magnitude of nongravitational effects in the semimajor axis noticeably changes with time. The motion of all comets is significantly affected by the components of nongravitational forces that are perpendicular to the orbital plane.  相似文献