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1.
I.?O.?Kitov I.?A.?Sanina S.?S.?Sergeev M.?A.?Nesterkina N.?L.?KonstantinovskayaEmail author 《Seismic Instruments》2018,54(2):158-174
The study of the stress-strain state of a medium in seismically quiet areas is difficult because of the absence of strong events. Under such circumstances, each earthquake, even relatively weak, is of high importance. In this case, all possible information on tectonic stresses and their dynamics, e.g., information on time, location, and magnitude of aftershocks, should be obtained from available seismic data. The earthquake near the town of Mariupol which occurred on August 7, 2016, had a body wave magnitude of 4.5–4.9 from the data of the different seismological centers. We detected 12 aftershocks that occurred within 5 days after the main shock using two seismic arrays (AKASG and BRTR) and one three-component station (KBZ) of the International Monitoring System, as well as two array stations of the Institute of Geosphere Dynamics, Russian Academy of Sciences. For six aftershocks, signals were found at three or more stations. The other aftershocks were detected from the data at two out of three nearest stations. Signal detection and association with aftershocks of the main shock, as well as estimation of magnitude and relative location of the found aftershocks, were carried out using the method of waveform cross-correlation (WFCC). The signals from the main shock that acted as the only master event (ME) for the WFCC method were used as waveform templates. To increase the signal-to-noise ratio and to determine the exact onset time of regular seismic waves from aftershocks, we used waveform templates of different length, from 10 to 180 s depending on the wave type and distance to the station, as well as band filtering in narrow frequency bands. The highest sensitivity of the detector and accuracy of the P-wave onset time estimates were reached when a waveform template included all regular waves from P to L g . Association of signals with aftershocks was based on back projection of signal arrival times to origin times using the travel time from a master event to the station, which was measured with a very low error, being equal to almost half of the digitization step length. To develop a seismic event hypothesis, the origin times at two or more stations should be spaced within a 2-s interval. 相似文献
2.
N. S. Bakhtigaraev P. A. Levkina L. V. Rykhlova A. V. Sergeev V. K. Taradiy N. V. Karpov V. V. Chazov 《Kinematics and Physics of Celestial Bodies》2016,32(5):237-240
Within the framework of the “Astronomy in the Elbrus Region” international program, investigations of space debris objects using optical measurements are carried out at the observation complex of the Zeiss-2000 telescope (developed by the International Center for Astronomical and Medico-Ecological Research, National Academy of Sciences, Ukraine) at Terskol Observatory. The objectives of this study are to detect, catalog, and determine the physical characteristics of small-sized space debris fragments, maintain orbit catalogs, and investigate the influence of nongravitational perturbations on the orbital motion and the evolution of orbits of these fragments. 相似文献
3.
M. A. Yudovskaya V. V. Distler N. V. Rodionov A. V. Mokhov A. V. Antonov S. A. Sergeev 《Geology of Ore Deposits》2011,53(1):27-57
The formation conditions and age of the Sukhoi Log gold deposit are considered on the basis of new isotopic-geochemical data.
The U-Pb isotopic study of zircon and monazite from high-grade ore and host black slates at the Sukhoi Log deposit was carried
out with SIMS technique using a SHRIMP II instrument. Two generations of monazite are distinguished on the basis of optical
and scanning electron microscopy, cathodoluminescence, and micro X-ray spectroscopy. Monazite I is characterized by black
opaque porphyroblasts with microinclusions of minerals pertaining to metamorphic slates and structural attributes of pre-
and synkinematic formation. Monazite II occurs only within the ore zone as transparent crystals practically free of inclusions
and as rims around monazite I. The REE contents are widely variable in both generations. Porphyroblastic monazite I differs
in low U and Th (0.01–0.7 wt % ThO2) contents, whereas transparent monazite II contains up to 4 wt % ThO2. The average weighted U-Pb isotopic age of monazite
I is 650 ± 8.1 Ma (MSWD = 1.6; n = 9) and marks the time of metamorphism or catagenesis. The U-Pb age estimates of synore monazite II cover the interval of
486 ± 18 to 439 ± 17 Ma. Zircons of several populations from 0.5 to 2.6 Ga in age are contained in the ore. Most detrital
zircon grains have porous outer rims composed of zircon and less frequent xenotime with numerous inclusions of minerals derived
from slates. The peaks of 206Pb/238U ages in the most abundant zircon populations fall on 570 and 630 Ma and correspond to the age of newly formed metamorphic
mineral phases. The discordant isotopic ages indicate that the U-ThPb isotopic system of ancient detrital zircons was disturbed
470–440 Ma ago in agreement with isotopic age of monazite II and the Rb-Sr whole -rock isochron age of black slates (447 ±
6 Ma). The new data confirm the superimposed character of the gold-quartz-sulfide mineralization at the deposit. Black shales
of the Khomolkho Formation of the Bodaibo Synclinorium were affected by metamorphism over a long period; the peaks of metamorphism
and catagenesis are dated at 570 and 650–630 Ma. The high-temperature ore formation was probably related to a hidden granitic
pluton emplaced 450–440 Ma ago, that is, 200 Ma later than the events of greenschist metamorphism. Hercynian granitoid magmatism
(320–270 Ma) did not exert a substantial effect on the U-Th-Pb isotopic system in accessory minerals from the ore and could
not have been a major source of ore-forming fluids. 相似文献
4.
A. M. Zubareva E. P. Pavlenko M. V. Andreev S. V. Antipin N. N. Samus’ A. V. Sergeev 《Astronomy Reports》2011,55(3):224-229
We have obtained data on various brightness states of the polar MT Dra over five years of observations, including the first
multicolor photometry for this close binary. We confirm the known orbital period, which has remained constant over 17 years,
which is unusual for cataclysmic binaries. Our observations in October 2006 demonstrated a transition of the polar to its
low brightness state within one day. 相似文献
5.
6.
N. N. Danchenko M. L. Kuleshova Z. P. Malashenko E. V. Petrova V. I. Sergeev 《Moscow University Geology Bulletin》2011,66(5):354-360
We study the filtering and sorption parameters of laboratory-produced composite materials, such as sand-gels, sand-gels with
an FeS activating additive, peat-gels, and commercial sorbents on the basis of cellulose coated with MnO2, which can be used for production of permeable geochemical barriers. The carry over and the efficiency of consumption of
the active component are estimated for materials with activating additives. It is shown that all the materials under study
can be used as fillers for a permeable geochemical barrier, but each of them has its own limitations. 相似文献
7.
Oceanology - During cruise 73 of the R/V Professor Gagarinskiy and cruise 53 of the R/V Akademik Oparin, oceanographic studies of the Sea of Japan and Sea of Okhotsk and the Northwest Pacific were... 相似文献
8.
Kapralova V. N. Chesnokova I. V. Makarycheva E. M. Sergeev D. O. 《Water Resources》2019,46(2):S81-S86
Water Resources - The dynamics of the talik zones, associated both with the internal cyclical nature of their development and with climate changes, leads to temporary differences in the volume of... 相似文献
9.
Doklady Earth Sciences - The results of isotope U–Pb dating of zircons from lherzolite and vein olivine orthopyroxenite composing the Roseta ultramafic massif are presented. The zircons... 相似文献