Climatology of Northern Hemisphere blocking in the ECHAM model     

S. Tibaldi  F. D’Andrea  E. Tosi  E. Roeckner 《Climate Dynamics》1997,13(9):649-666

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Acceleration of multiply charged ions of the anomalous cosmic-ray component at the heliosphere boundary     

V. M. Ostryakov  M. F. Stovpyuk  V. P. Shevel’ko 《Astronomy Reports》2004,48(4):342-351

The formation of the energy spectra of heavy ions at the front of a parallel shock is considered taking into account ionization and recombination during the acceleration. An analytic solution for ions with three possible charge states is obtained and applied to the acceleration of the anomalous cosmic-ray component at the boundary of the heliosphere. In addition, a more general numerical model for such acceleration at a spherical shock front is developed and used to obtain the energy dependence of the mean charges for C, N, O, Ne, Si, S, Ar, and Fe ions. The model implies that highly excited ions begin to dominate over ions with low charges at energies above 1 MeV/nucleon, in agreement with observational data.  相似文献   

Variations in Stable Carbon Isotopic Composition of n-Alkanes from Ordovician and Triassic-Derived Oils in Lunnan Oilfield, Tarim Basin, NW China： Global Paleoenvironmental Constraints     

卢鸿孙永革  彭平安 《中国地球化学学报》2004,23(3):207-219

Molecular stable carbon isotope technique was employed to study well-sourced crude oils collected from a single drilling well and from the entire Lunnan oilfield, Tarim Basin, NW China. The stable carbon isotopic composition of n-alkanes from crude oils showed that Ordovi-clan-derived oils are enriched in ^13C and Triassic-derived oils are depleted in ^13C. This is consistent with the distribution and evolution trend of stable carbon isotope ratios in crude oils/organic matter from all over the world in geological history (Stahl, 1977; Andrusevich et al. ,1998). An extensive survey of literature indicates that, except for thermal maturity, organic matter input and depositional environment, paleoenvironmental background is another key factor that affects the stable carbon isotopic composition of Ordovician- and Triassic-derived crude oils. The results showed that gas chromatographic-isotope ratio mass spectrometry ( GC-C-IRMS), combining with biogeoehemical evolution of organic matter in geological history, may be a powerful tool in refining oil/oil, oil/source correlations in multi-age, multi-source petroliferous basins like Tarim.  相似文献   

Masses of protostars with methanol protoplanetary disks     

I. E. Val’tts  S. Yu. Lyubchenko 《Astronomy Reports》2004,48(3):210-218

The masses of 12 protostars assumed to be the central bodies in circumstellar protoplanetary disks are estimated based on analysis of their methanol maser spectra and fine spatial structure. The calculations are based on the hypothesis that the class II methanol maser lines are formed in an edge-on Keplerian disk, while the thermal methanol emission and CS lines are formed in a cocoon around the protostar. This provides information about the velocities of the protostar and the methanol maser condensations relative to the center. In most of the star-forming regions studied, the derived masses are within limits admissible for disks around massive OB stars. The masses are in good agreement with the calculations of other authors based on models of the velocity gradients of the maser features. It is suggested that the methanol spectra display a triplet structure in which the two lateral features are class II methanol lines and the central component is a class I methanol maser line or thermal methanol line. This is consistent with the fact that the correlation of regions of maser emission with regions of emission of dense molecular gas in the CS line is about twice as strong(about 100%) as the correlation with ultracompact HII regions (about 50%). This should be taken into account when modeling protoplanetary disks and star-forming regions.  相似文献   

The earthquake of 6 September 2002 and the seismic history of Palermo (Northern Sicily,Italy): Implications for the seismic hazard assessment of the city     

R. Azzaro  M. S. Barbano  R. Camassi  S. D’Amico  A. Mostaccio  G. Piangiamore  L. Scarfì 《Journal of Seismology》2004,8(4):525-543

On September 6, 2002, a M_L = 5.6 earthquake, occurring some tens of kilometres offshore from the Northern Sicilian coast (Southern Tyrrhenian Sea), slightly damaged the city of Palermo and surroundings (degree 6 in the European Macroseismic Scale 1998). The macroseismic investigation of the shock and a detailed study of effects of the main earthquakes which affected Palermo in the past have been performed in order to evaluate the seismic response of the city. Moreover, the comparison of the recent event, which is instrumentally constrained, with historical earthquakes allows us to infer new insights on the seismogenic sources of the area, that seem located offshore in the Tyrrhenian sea.In the last 500 years, Palermo has never been completely destroyed but has suffered effects estimated between intensities 6 and 8 EMS-98 many times (1693, 1726, 1751, 1823, 1940, 1968, 2002). The damage scenarios of the analysed events have shown that damage distribution is strongly conditioned by soil response in the different parts of the city and by a high building vulnerability, mainly in the historical centre and in the south-eastern zone of the modern city. As a matter of fact, Palermo has always suffered greater effects than those reported for other nearby localities. The hazard assessment obtained using observed site intensities has shown that the probability of occurrence for intensity 8 (the strongest intensity observed in Palermo) exceeds 99% for 550 years, while the estimated mean return period is 152 ± 40 years. These results, in connection with building vulnerability due to the urban expansion before the introduction of seismic code, suggest that the city is exposed to a relatively high seismic risk.This paper has not been submitted elsewhere in identical or similar form, nor will it be during the first 3 months after its submission to Journal of Seismology.  相似文献   

Radio and optical spectral studies of radio sources     

V. L. Afanas’ev  S. N. Dodonov  A. V. Moiseev  A. G. Gorshkov  V. K. Konnikova  M. G. Mingaliev 《Astronomy Reports》2003,47(6):458-466

Optical identifications and an analysis of the radio spectra of eight radio sources from a flux-density-complete sample at declinations 4°–6° (B 1950) are presented. The observations were carried out at 4000–9000 Å on the 6-m telescope of the Special Astrophysical Observatory and at 0.97–21.7 GHz on the RATAN-600 telescope. Five of the eight sources are quasars and three are emission-line radio galaxies.  相似文献   

Observations of stellar objects at a shell boundary in the star-forming complex in the galaxy IC 1613     

T. A. Lozinskaya  V. P. Arkhipova  A. V. Moiseev  V. L. Afanas’ev 《Astronomy Reports》2002,46(1):16-26

The single region of ongoing star formation in the galaxy IC 1613 has been observed in order to reveal the nature of compact emission-line objects at the edges of two shells in the complex, identified earlier in Hα line images. The continuum images show these compact objects to be stars. Detailed spectroscopic observations of these stars and the surrounding nebulae were carried out with an MPFS spectrograph mounted on the 6-m telescope of the Special Astrophysical Observatory. The resulting stellar spectra were used to determine the spectral types and luminosity classes of the objects. Of star we identified the only object of this spectral type in IC 1613. The results of optical observations of the multishell complex are compared to 21-cm radio observations. The shells harboring the stars at their boundaries constitute the most active part of the star-forming region. There is evidence that shocks have played an important role in the formation of the shells.  相似文献   

Thermal emission of methanol and other molecules at millimeter wavelengths     

S. V. Kalenskii  V. I. Slysh  I. E. Val’tts 《Astronomy Reports》2002,46(2):96-109

The paper reports the results of a survey of Galactic star-forming regions in the methanol lines 8_?1–7₀ E at 229.8 GHz, 3_?2–4_?1 E at 230.0 GHz, 0₀–1_?1 E at 108.9 GHz, and a series of J ₁–J ₀ E lines near 165 GHz. In addition to the methanol lines, lines of methyl cyanide (CH₃CN), cyanoacetylene (HC₃N), methyl formate (HCOOCH₃), and sulphur dioxide (SO₂) were detected. Analysis of the data indicates that the methanol emission arises in warm (30–50 K) gas.  相似文献   

Macromolecules in the galaxy and the cosmic microwave background     

Yu. N. Pariiskii  N. N. Bursov  A. B. Berlin  N. A. Nizhel’skii  A. V. Bogdantsov  P. A. Tsybulev 《Astronomy Reports》2002,46(7):525-530

A deep search for the predicted Galactic microwave dipole emission of spinning interstellar fullerene-type molecules has been conducted using the RATAN-600 radio telescope. This effect is of interest both in its own right and as a new form of Galactic screen between the cosmic microwave background (CMB) and the observer. The power of this noise component on angular scales of about 0.1° (l=1000) is estimated. These scales are of primary interest for the “Cosmological Gene of the Universe” (RATAN-600), PLANCK Surveyor Mission, and other projects. At the frequencies of the expected emission peak of this dust component, the small-scale noise is a factor of 20 weaker than the predicted noise. It is shown that the role of this dust component is negligible, at least at the main PLANCK frequencies. The first estimates of the contribution from Galactic polarization noise are given for λ=3.9 cm, where the theory predicts a maximum in the CMB polarization (l～1000). At wavelengths of ～1 cm and shorter, macromolecules contribute less than 1 µK, and should not hinder CMB polarization studies. Galactic synchrotron polarization, likewise, should not prevent CMB polarization experiments at the main PLANCK frequencies.  相似文献   

Identification and alleviation pathways of multidimensional poverty and relative poverty in counties of China   总被引：1，自引：1，他引：0  

XU Lidan  DENG Xiangzheng  JIANG Qun'ou  MA Fengkui 《地理学报(英文版)》2021,31(12):1715-1736

To realize efficient and sustainable poverty alleviation,this study firstly investigated the identification of multidimensional poverty and relative poverty,and then explored relevant poverty alleviation pathways.Poverty levels in 31 provinces including the autonomous re-gions and municipalities of China were identified at the county level using the average nighttime light index (ANLI),county multidimensional development index (CMDI),and a method combining multidimensional poverty index and relative poverty standards.Poverty alleviation pathways for poverty-stricken counties were explored from the aspects of industry,education,tourism and agriculture.The results revealed that nearly 60％ of counties in China were primarily under relative poverty,most of which were corresponded to light relative pov-erty.In terms of ANLI and CMDI,63％ and 79％ of the national poverty-stricken counties,as of 2018,could be identified,suggesting that CMDI had a higher performance for identifying poverty at the county level.In terms of poverty alleviation pathways,414,172,442,and 298 poverty-stricken counties were receptive to industry poverty alleviation,education poverty alleviation,tourism poverty alleviation,and agriculture poverty alleviation,and 61％ of coun-ties had more poverty-causing factors,implying that multidimensional poverty alleviation is suitable in most of the counties.  相似文献