Estimation of Aerosol Radiation Effects under Background and Smoke-haze Atmospheric Conditions over Siberia from Empirical Data     

M. V. Panchenko  T. B. Zhuravleva  V. S. Kozlov  I. M. Nasrtdinov  V. V. Pol’kin  S. A. Terpugova  D. G. Chernov 《Russian Meteorology and Hydrology》2016,41(2):104-111

The results of numerical simulation of downward solar radiation fluxes for background and smoke-contaminated atmospheric conditions are discussed. Vertical profiles of aerosol characteristics are obtained from the empirical model based on the data of aircraft sounding of profiles of angular scattering coefficients and content of absorbing particles in the lower troposphere. The background model was created using the results of measurements obtained under cloudless and mostly cloudless atmospheric conditions in 1999–2011. Optical parameters of smoke aerosol are determined from the data of aircraft measurements in the period of long-term wildfires in Siberia in the summer 2012. It is demonstrated that deficiency in diurnal values of total solar radiation at the surface level caused by the formation of the optically dense smoke layer as compared to background conditions, is more than 13 MJ/m².  相似文献   

The Answer to the Comments by Yu. D. Resnyanskii to the Papers by L. Kh. Ingel’ and A. A. Makosko     

. Kh. Ingel’  A. A. Makosko 《Russian Meteorology and Hydrology》2016,41(2):146-150

The critical comments to the publications by the authors ofthe present paper that were given in [10] (the publications deal with the possible effects of gravity field inhomogeneities in the atmosphere and ocean) are discussed. In the authors' opinion, some remarks are groundless. At the same time, the authors agree with one of the important remarks that the results of their paper concerning studies of the ocean disturbances are to be reconsidered.  相似文献   

Exploring the spatially varying innovation capacity of the US counties in the framework of Griliches’ knowledge production function: a mixed GWR approach   总被引：1，自引：0，他引：1  

Dongwoo Kang  Sandy Dall’erba 《Journal of Geographical Systems》2016,18(2):125-157

Griliches’ knowledge production function has been increasingly adopted at the regional level where location-specific conditions drive the spatial differences in knowledge creation dynamics. However, the large majority of such studies rely on a traditional regression approach that assumes spatially homogenous marginal effects of knowledge input factors. This paper extends the authors’ previous work (Kang and Dall’erba in Int Reg Sci Rev, 2015. doi: 10.1177/0160017615572888) to investigate the spatial heterogeneity in the marginal effects by using nonparametric local modeling approaches such as geographically weighted regression (GWR) and mixed GWR with two distinct samples of the US Metropolitan Statistical Area (MSA) and non-MSA counties. The results indicate a high degree of spatial heterogeneity in the marginal effects of the knowledge input variables, more specifically for the local and distant spillovers of private knowledge measured across MSA counties. On the other hand, local academic knowledge spillovers are found to display spatially homogenous elasticities in both MSA and non-MSA counties. Our results highlight the strengths and weaknesses of each county’s innovation capacity and suggest policy implications for regional innovation strategies.  相似文献   

刚果(金)地质特征与主要矿产资源概况   总被引：1，自引：0，他引：1  

张学良  姚锦其  邓贵安  徐文彦  黄学强  李明君 《矿产与地质》2016,(4):555-560

刚果(金)主要由刚果盆地和环盆地高原组成,盆地主要由中生代到新生代地层及近现代沉积物组成,沿着盆地内边缘分布有泛非时期的火山沉积物,环盆地高原主要为抬升的前寒武纪基底。刚果(金)优势金属矿产资源主要分布环盆地高原的加丹加新元古代铜-钴多金属成矿带、KIB-KAB中元古代锡-铌-钽-钨多金属成矿带、刚果东北太古代绿岩带型金-铁多金属成矿带上,而金刚石则主要分布开赛及东北部地区中新生代金刚石成矿区内。  相似文献   

Paleoproterozoic anorogenic granitoids of the Zheltav sialic massif (Southern Kazakhstan): Structural position and geochronology     

A. A. Tretyakov  K. E. Degtyarev  E. B. Sal’nikova  K. N. Shatagin  A. B. Kotov  A. V. Ryazantsev  A. V. Pilitsyna  S. Z. Yakovleva  E. V. Tolmacheva  Yu. V. Plotkina 《Doklady Earth Sciences》2016,466(1):14-19

The basement of the Zheltav sialic massif (Southern Kazakhstan) is composed of different metamorphic rocks united into the Anrakhai Complex. In the southeastern part of the massif, these rocks form a large antiform with the core represented by amphibole and clinopyroxene gneissic granite varieties. By their chemical composition, dominant amphibole (hastingsite) gneissic granites correspond to subalkaline granites, while their petroand geochemical properties make them close to A-type granites. The U–Pb geochronological study of accessory zircons yielded an age of 1841 ± 6 Ma, which corresponds to the crystallization age of melts parental for protoliths of amphibole gneissic granites of the Zheltav Massif. Thus, the structural–geological and geochronological data make it possible to define the Paleoproterozoic (Staterian) stage of anorogenic magmatism in the Precambrian history of the Zheltav Massif. The combined Sm–Nd isotopic—geochronological data and age estimates obtained for detrital zircons indicate the significant role of the Paleoproterozoic tectono-magmatic stage in the formation of the Precambrian continental crust of sialic massifs in Kazakhstan and northern Tien Shan.  相似文献   

Risk Assessment of Soil Compaction in the Walloon Region in Belgium   总被引：1，自引：0，他引：1  

Dimitri D’Or  Marie-France Destain 《Mathematical Geosciences》2016,48(1):89-103

  相似文献   

Russian studies of atmospheric electricity in 2011–2014     

E. A. Mareev  V. N. Stasenko  A. A. Bulatov  S. O. Dement’eva  A. A. Evtushenko  N. V. Il’in  F. A. Kuterin  N. N. Slyunyaev  M. V. Shatalina 《Izvestiya Atmospheric and Oceanic Physics》2016,52(2):154-164

This review contains the most significant results of Russian studies in the field of atmospheric electricity in 2011–2014. It is part of the Russian National Report on Meteorology and Atmospheric Sciences to the International Association of Meteorology and Atmospheric Sciences (IAMAS). The report was presented and approved at the XXVI General Assembly of the International Union of Geodesy and Geophysics (IUGG).¹ The review is followed by a list of the main published works on the studies of atmospheric electricity of Russian scientists in 2011–2014.  相似文献   

Russian investigations in the field of atmospheric radiation in 2011–2014     

Yu. M. Timofeev  E. M. Shul’gina 《Izvestiya Atmospheric and Oceanic Physics》2016,52(5):467-482

A short survey prepared by the Russian Commission on Atmospheric Radiation contains the most significant results of work in the field of atmospheric-radiation studies performed in 2011–2014. It is part of the Russian National Report on Meteorology and Atmospheric Sciences prepared for the International Association on Meteorology and Atmospheric Sciences (IAMAS)¹. During this period, the Russian Commission on Atmospheric Radiation, jointly with the concerned departments and organizations, organized two International Symposiums on Radiation and Dynamics (ISARD-2011 and ISARD-2013). At these conferences, the central problems in modern atmospheric physics were discussed: radiative transfer (RT) and atmospheric optics; greenhouse gases, clouds, and aerosols; remote methods of measurements; and new measurement data. This survey presents six directions covering the whole spectrum of investigations performed in the field of atmospheric radiation.  相似文献   

Fluorite as an Sm–Nd geochronometer of hydrothermal processes: Dating of mineralization hosted in the Strel’tsovka uranium ore field,eastern Baikal region     

I. V. Chernyshev  V. N. Golubev  A. P. Aleshin  Yu. O. Larionova  Yu. V. Gol’tsman 《Geology of Ore Deposits》2016,58(6):447-455

The possibility of using hydrothermal fluorite as an Sm–Nd geochronometer is based on the results of an REE pattern study of this mineral (Chernyshev et al., 1986). As a result of REE fractionation, in many cases, the Sm/Nd ratio achieves a multifold increase compared with its level in terrestrial rocks, and the radiogenic shift of the ¹⁴³Nd/¹⁴⁴Nd isotope ratio reaches 10–20 ε_Nd units over a short time interval (as soon as tens of Ma). This is a necessary prerequisite for Sm–Nd isochron dating of fluorite. Zonal polychrome fluorite from a vein referred to the final stage of large-scale uranium mineralization at the Sterl’tsovka deposit in the ore field of the same name located in the eastern Transbaikal region has been dated using the ¹⁴³Nd/¹⁴⁴Nd method. To optimize isochron construction, local probes with high and contrasting Sm/Nd ratios have been sampled from the polished surfaces of two samples, taking into account the REE pattern of zonal fluorite. Sm–Nd isochron dating has been carried out separately for each sample. The ¹⁴⁷Sm/¹⁴⁴Nd и ¹⁴³Nd/¹⁴⁴Nd ratios vary within the intervals 0.5359–2.037 and 0.512799–0.514105, respectively. Two isochrons, each based on six fluorite probes, have been obtained with the following parameters, which coincide within 2σ uncertainty limits: (1) t = 134.8 ± 1.3 Ma, (¹⁴³Nd/¹⁴⁴Nd)₀ = 0.512310 ± 13, MWSD = 0.43 and (2) t = 135.8 ± 1.6 Ma, (¹⁴³Nd/¹⁴⁴Nd)₀ = 0.512318 ± 10, MWSD = 1.5. The mean age of fluorite based on two isochron datings is 135.3 ± 1 Ma. Comparison of this value with the most precise dating of pitchblende related to the ore stage in the Strel’tsovka ore field (135.5 ± 1 Ma) shows that four mineralization stages, distinguished by geological and mineralogical data, that were completed with the formation of polychrome fluorite veins 135.3 ± 1 Ma ago, represent a single and indivisible hydrothermal process whose duration does not exceed 1 Ma.  相似文献   

Suprathermal ions in solar-wind outflows from coronal holes at 1 AU     

M. A. Zel’dovich  Yu. I. Logachev  G. M. Surova  K. Kecskemety  I. S. Veselovskii 《Astronomy Reports》2016,60(7):687-693

The energy spectra and relative abundances of ³He, ⁴He, C, O, and Fe ions with energies of ~0.04–2 MeV/nucleon are studied using data from the ULEIS instrument on board the ACE spacecraft obtained during quiescent periods in 2006–2012. During the unique, prolonged minimum between cycles 23 and 24, 35 quiescent periods were distnguished, during which solar-wind flows from near-equatorial coronal holes (CHs) were detected. It is shown that the C/O and Fe/O ratios for suprathermal ions correspond to the relative abundances of the corresponding thermal ions in the fast and slow (Maxwellian) solar wind (SWICS/ACE), while the ⁴He/O ratio exceeds the corresponding ratio in the solar wind by a factor of two. The intensities of the ³He, ⁴He, C, O, and Fe suprathermal ions in outflows from CHs grow with the speed of the solar wind. This indicates that, in periods ofminimumsolar activity, suprathermal ions from CHs represent a high-temperature “tail” of the solar wind. An additional flux of suprathermal helium ions may also be contributed by other external sources.  相似文献