Parameters of the intense X-ray and gamma-ray radiation from the solar flare of May 20, 2002, as observed from the Coronas-F spacecraft     

A. V. Bogomolov  A. P. Ignat’ev  K. Kudela  S. N. Kuznetsov  Yu. I. Logachev  O. V. Morozov  I. N. Myagkova  S. N. Oparin  A. A. Pertsov  S. I. Svertilov  B. Yu. Yushkov 《Astronomy Letters》2003,29(3):199-204

We consider temporal, spectral, and polarization parameters of the hard X-ray and gamma-ray radiation observed during the solar flare of May 20, 2002, in the course of experiments with the SONG and SPR-N instruments onboard the Coronas-F spacecraft. This flare is one of the most intense gamma-ray events among all of the bursts of solar hard electromagnetic radiation detected since the beginning of the Coronas-F operation (since July 31, 2001) and one of the few gamma-ray events observed during solar cycle 23. A simultaneous analysis of the Coronas-F and GOES data on solar thermal X-ray radiation suggests that, apart from heating due to currents of matter in the the flare region, impulsive heating due to the injection of energetic electrons took place during the near-limb flare S21E65 of May 20, 2002. These electrons produced intense hard X-ray and gamma-ray radiation. The spectrum of this radiation extends up to energies ≥7 MeV. Intense gamma-ray lines are virtually unobservable against the background of the nonthermal continuum. The polarization of the hard X-ray (20–100 keV) radiation was estimated to be ≤15–20%. No significant increase in the flux of energetic protons from the flare under consideration was found. At the same time, according to ACE data, the fluxes of energetic electrons in interplanetary space increased shortly (～25 min) after the flare.  相似文献   

The influence of cosmic rays on the stability and large-scale dynamics of the interstellar medium     

V. D. Kuznetsov 《Astrophysics and Space Science》1985,113(1):99-117

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The Expansion of the Hamiltonian of the Planetary Problem into the Poisson Series in All Keplerian Elements (Theory)     

Kholshevnikov  K. V.  Greb  A. V.  Kuznetsov  E. D. 《Solar System Research》2001,35(3):243-248

The study of the evolution of planetary systems, primarily of the Solar System, is one of the basic problems of celestial mechanics. The stability of motion of giant planets on cosmogonic time scales was established by numerical and analytical methods, but the question about the evolution of orbits of terrestrial planets and arbitrary solar-type planetary systems remained open. This work initiates a series of papers allowing one to advance in solving the problem of the evolution of the solar-type planetary systems on cosmogonic time scales by using powerful analytical tools. In the first paper of this series, we choose the optimum reference system and obtain the Poisson series expansion of the Hamiltonian of the problem in all Keplerian elements. We propose to use the integral representation of the corresponding coefficients or the Poisson processor means instead of conventionally addressing any possible special functions. This approach extremely simplifies the algorithm. The next paper of this series deals with the calculation of the expansion coefficients.  相似文献   

Pb-Pb age of sedimentary phosphorite reworking in Lower Riphean carbonate sediments,the Satka Formation of Southern Urals     

G. V. Ovchinnikova  A. B. Kuznetsov  I. M. Vasil’eva  I. M. Gorokhov  M. T. Krupenin  A. V. Maslov  T. L. Turchenko 《Stratigraphy and Geological Correlation》2008,16(2):138-142

The mineral composition and U-Pb and Rb-Sr systematics of phosphorites from the Satka Formation of Lower Riphean carbonates, the Burzyan Group of Southern Urals, are studied. Phosphorites occurring as small lenses between stromatolite layers are composed largely of fluorapatite with admixture of detrital quartz, feldspars, illite, and chlorite. Phosphorite samples have been subjected to stepwise dissolution in 1 N (fraction L-1) and 2 N (fraction L-2) HCl. As is established, the maximum apatite content is characteristic of fraction L-1, while fraction L-2 is enriched in products of dolomite and sulfide dissolution and in elements leached from siliciclastic components. The Sr content in the Satka apatites (280–560 ppm) is substantially lower as compared with that in unaltered marine apatite. The ⁸⁷Sr/⁸⁶Sr “initial ratio in the phosphorites studied (0.71705–0.72484) and host dolomites from the lower part of the Satka Formation is significantly higher than in the Early Riphean seawater that indicates a reset of the Rb-Sr original systems in sediments. The Pb-Pb age of 1340 ± 30 Ma (MSWD = 6.4) estimated based on 7 data points characterizing fractions L-1 and L-2 is younger than the formation time of overlying Burzyan sediments, being consistent, within the error range, with date of the Mashak rifting event recorded at the Early-Middle Riphean boundary. The comparative U-Pb characteristics of two soluble fractions (L-1 and L-2) and silicate residue of phosphorites show that epigenetic redistribution of Pb and U was characteristic of the phosphorite horizon only. The initial Pb isotope composition and μ (²³⁸U/²⁰⁴Pb) estimated according to model by Stacey and Kramers for the early diagenetic fluids in carbonate and phosphate sediments of the Satka Formation suggest that they were in isotopic equilibrium with erosion products of the Taratash crystalline complex.  相似文献   

Russian-Polish joint biohydrochemical studies in the gulf of Gdansk of the Baltic Sea (R/V Baltica, June 2005)     

M. Welgat  M. Zalewski  A. Amerik  A. Grelowski  L. L. Kuznetsov  N. M. Lapina  N. I. Torgunova  T. B. Semochkina 《Oceanology》2006,46(4):592-595

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New outcrop of buried Kazantsevo peat at lower reaches of the Irtysh River     

S. A. Laukhin  Kh. A. Arslanov  F. E. Maksimov  V. Yu. Kuznetsov  G. N. Shilova  F. Yu. Velichkevich  S. B. Chernov  Ya. A. Nikonorov 《Doklady Earth Sciences》2008,419(2):200-204

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Geochronology and landscape-climatic environments of the Early Zyryanian Interstadial in West Siberia     

S. A. Laukhin  F. E. Maksimov  Kh. A. Arslanov  V. Yu. Kuznetsov  S. B. Chernov  G. N. Shilova  F. Yu. Velichkevich 《Doklady Earth Sciences》2008,421(1):796-799

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The Cambrian pre-Uralide-Timanide orogen: Structural evidence for its collisional origin     

N. B. Kuznetsov 《Doklady Earth Sciences》2008,423(2):1383-1387

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Late Quaternary marine terraces in the Mediterranean coastal area of Syria: Geochronology and neotectonics     

A.E. Dodonov  V.G. Trifonov  T.P. Ivanova  V.Yu. Kuznetsov  F.E. Maksimov  D.M. Bachmanov  T.A. Sadchikova  A.N. Simakova  H. Minini  A.-M. Al-Kafri  O. Ali 《Quaternary International》2008,190(1):158

In order to provide new data on the neotectonics and geodynamic properties of western Syria, studies of marine terraces have been carried out. The most attention was paid to the lower terraces in the range of 3–5 to 30–35 m above sea level, because they have more complete distributions along the shore. The lower terraces were examined along the coastal area from Tartus to Latakia, and along the carbonate cliff on Arwad Island. Seven ²³⁰Th/U dates for these terraces are in the range of 85–130 ka, suggesting the age interval of the last interglacial (MIS 5). New dates on the lower terraces provide a basis for stratigraphical and geomorphological interpretation as well as neotectonic reconstruction. According to the geomorphological data and lithological composition of those terraces, two main uplifted blocks can be established. One coincides with the Latakia block, and another corresponds to the western margin of the Banias volcanic plateau. These blocks are divided by a subsided structure corresponding to the Nahr el Kebir graben. The amplitude of neotectonic uplifting in the Latakia and Banias blocks reaches 15–20 m for the Late Pleistocene.  相似文献   

Sedimentation rates in the sea of Azov inferred from <Superscript>137</Superscript>Cs and <Superscript>241</Superscript>Am specific activity     

Yu. A. Fedorov  A. N. Kuznetsov  M. E. Trofimov 《Doklady Earth Sciences》2008,423(1):1333-1334

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