Pub Date : 2024-07-18DOI: 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.
{"title":"The Effect of Heavy Inclusions in the Upper Crust on Thermoconvective Instability of the Lithosphere","authors":"B. I. Birger","doi":"10.1134/S1069351324700411","DOIUrl":"10.1134/S1069351324700411","url":null,"abstract":"<p>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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"346 - 354"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743212","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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。
{"title":"On Constructing of Magnetic and Gravity Images of Mercury from Satellite Data","authors":"I. E. Stepanova, A. G. Yagola, D. V. Lukyanenko, I. I. Kolotov","doi":"10.1134/S1069351324700459","DOIUrl":"10.1134/S1069351324700459","url":null,"abstract":"<p><b>Abstract</b>—A new technique for simultaneous construction of the “gravity” and “magnetic” images of Mercury from satellite data based on the regional version of the <i>S</i> 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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"441 - 458"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743219","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Prediction Results for the Strongest Earthquakes of February 6, 2023 in Southern Turkey","authors":"A. I. Gorshkov, V. G. Kossobokov, O. V. Novikova","doi":"10.1134/S1069351324700423","DOIUrl":"10.1134/S1069351324700423","url":null,"abstract":"<p><b>Abstract</b>—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 <i>М</i> ≥ 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 <i>M</i>8 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 <i>М</i> ≥ 6.5, and both events occurred within the spatial and temporal coverage of the warning area diagnosed by the <i>M</i>8 algorithm in July 2021.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"339 - 345"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743211","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Seismic Pulses before the February 27, 2010 M = 8.8 Chile Earthquake","authors":"G. A. Sobolev, I. N. Migunov","doi":"10.1134/S1069351324700447","DOIUrl":"10.1134/S1069351324700447","url":null,"abstract":"<p><b>Abstract</b>—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 <i>M</i><sub>w</sub> 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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"333 - 338"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743210","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Technology of Mapping of Volcanic-Sedimentary Strata in a Complexly Dislocated Terrigenous Structure according to Seismic and Magnetic Exploration Data (Pechora Sea)","authors":"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","doi":"10.1134/S1069351324700496","DOIUrl":"10.1134/S1069351324700496","url":null,"abstract":"<p>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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"479 - 493"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743369","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Shear Trough Depth and Geometry Relation Determined from Satellite Radar Images from One or Two Orbits","authors":"I. P. Babayants, V. O. Mikhailov, E. P. Timoshkina, A. A. Baryakh","doi":"10.1134/S1069351324700514","DOIUrl":"10.1134/S1069351324700514","url":null,"abstract":"<p><b>Abstract</b>—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 <i>U</i><sub>subv</sub> 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 <i>U</i><sub>subv</sub> 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 <i>U</i><sub>subv</sub> 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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"508 - 517"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743112","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Investigation of the Lithospheric Plate Boundary Zone within the Sakhalin Island Based on Satellite Geodesy Data","authors":"M. S. Gridchina, G. M. Steblov, I. S. Vladimirova, A. V. Basmanov","doi":"10.1134/S1069351324700526","DOIUrl":"10.1134/S1069351324700526","url":null,"abstract":"<p>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 <i>TDEFNODE</i> 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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"518 - 527"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743221","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Meteorological Anomalies and Strong Earthquakes: A Case Study of the Petropavlovsk-Kamchatsky Region, Kamchatka Peninsula","authors":"G. N. Kopylova, Yu. K. Serafimova, A. A. Lyubushin","doi":"10.1134/S1069351324700502","DOIUrl":"10.1134/S1069351324700502","url":null,"abstract":"<p><b>Abstract</b>— 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 <i>I</i><sub>MSK<i>-</i>64</sub> ≥ 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 <i>En</i>, the logarithm of the curtosis coefficient logκ, and the autoregressive measure of nonstationarity <i>Q</i><sup>2</sup> 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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"494 - 507"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743218","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"What Does the Archaeomagnetic Record of Fired Ceramics Reflect?","authors":"O. V. Pilipenko, G. P. Markov, N. V. Salnaya, P. A. Minaev, N. A. Aphinogenova","doi":"10.1134/S1069351324700435","DOIUrl":"10.1134/S1069351324700435","url":null,"abstract":"<p><b>Abstract</b>—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-Fe<sub>2</sub>O<sub>3.</sub></p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"424 - 440"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743216","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2024-07-18DOI: 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.
{"title":"Chetdin Radon Anomaly (Komi Republic): Localization and Study","authors":"Yu. E. Ezimova, V. V. Udoratin, A. Sh. Magomedova","doi":"10.1134/S1069351324700484","DOIUrl":"10.1134/S1069351324700484","url":null,"abstract":"<p>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/m<sup>3</sup>. 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/m<sup>3</sup> on average, in rare cases up to 10 000–12 000 Bq/m<sup>3</sup>. 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.</p>","PeriodicalId":602,"journal":{"name":"Izvestiya, Physics of the Solid Earth","volume":"60 3","pages":"466 - 478"},"PeriodicalIF":0.9,"publicationDate":"2024-07-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"141743217","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}