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991.
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994.
W. D. Hutchison N. Yazidjoglou D. J. Isbister D. H. Chaplin L. N. Shakhmuratova 《Hyperfine Interactions》1993,80(1-4):1173-1178
Results for an inhomogeneously broadened60CoFe NMRON sample have been obtained for gamma detected single pulse (nutation) and two pulse (free induction decay) experiments in the region of intermediate-to-lowR(=1/). Here 1 is the angular frequency measure of the strength of the ferromagnetically enhanced RF field at the nucleus and is the HWHM of the inhomogeneously broadened line. Comparisons of the oscillatory FID signals obtained are made with the theoretical predictions of the following paper [6]. 相似文献
995.
H. M. Ajvazyan 《International Journal of Infrared and Millimeter Waves》1993,14(11):2311-2338
Three hail-formation phases in a cloud may be detected, by means of MM and SubMM wave propagation analysis in Convective clouds. These phases are size increase of super-large(85 to 1500m in radius, and larger) droplets, their transition into supercooled state, and immediate droplets transition into ice or small hail, or their coating by ice Crust. Ice transparency window in absorption index, existing in SubMM wave band, is shown to serve as indicator of ice creation in a cloud. Radar reflection coefficient is shown to be increased by two orders of magnitude in the ice transparency window under super-large droplets transition into ice. 相似文献
996.
H. M. Ajvazyan H. H. Ajvazyan 《International Journal of Infrared and Millimeter Waves》1993,14(5):1155-1174
Two detection methods of hail embryons in a cloud are discussed in the paper: combined passive/active and purely active sensing of a convective cloud from board of air or space carrier. The first method makes it possible to determine the spectral dependence of absorption coefficient by oversized drops in convective cloud in the millimeter (MM) and submillimeter (SbMM) wavebands. With this purpose a highly sensitive 16-channel Dicke radiometer is used. In the second method a multiwave (12 wavelength) active radar is used to determine the spectral dependence of backscatter coefficient in the same wavebands. Variation of these spectral characteristics in time makes possible the detection of physical processes taking place in a cloud, such as drops drowth and evaporation, as well as transition of oversized drops into the overcooled state. The instant of water/ice phase transition in oversized drops is determined in both methods by means of active radar in SbMM waveband (in the transparency window of ice and atmosphere, 0.64 mm). Corresponding hardware, antennas, and wavelengths are considered for active/passive and purely active sensind of clouds. The effect of antenna beamwidth in SbMM on anomalous backscatter is discussed.Finally the authors would like to acknowledge the helpful discussions and assistance of Dr. K.E.Karapetyan in calculation of the antenna E characteristics. 相似文献
997.
We consider a class of vertex models describing directed lines on a lattice in arbitraryd dimensions, and solve the model exactly for the Cartesian lattice and in the case that each loop of lines carries a fugacity - 1. Our analysis, which can be carried out for arbitrary lattices, is based on an equivalence of the vertex model with a dimer problem. The dimer problem is, in turn, solved using the method of Pfaffians. It is found that the system is frozen below a critical temperatureT
cwith the critical exponent = (3 –d)/2. 相似文献
998.
Chemical and electronic properties of scrapecleaned YBa2Cu3O7–(YBCO) ceramics, which were also annealed in vacuum or exposed to H atoms or O2 molecules, were studied at room temperature by applying Auger electron (AES) and low-energy electron energy-loss spectroscopy (LEELS). Scanning electron micrographs showed such scraped surfaces to consist mainly of small, fractured YBCO crystallites, i.e. of clean YBCO surfaces. With only one exception, all low-energy AES lines were found to be shifted in energy compared to data recorded with surfaces of metallic Cu and Y. The analysis of the high-energy AES lines indicated the existence of non-stoichiometric material in grain boundaries. At least 25 different LEELS features were recorded. The 24.9-eV energy loss, which is due to the excitation of bulk valence-electron plasmons, indicates an enhanced oxygen deficit s 0.8 at scrape-cleaned YBCO surfaces. Annealing of scraped YBCO samples at approximately 700 K in vacuum and also their exposure to hydrogen atoms resulted in an additional oxygen depletion within a few atomic layers near to the surfaces. These oxygen deficiencies were found to increase the intensity ratios of low-and high-energy AES lines of Cu, Ba, and Y and to intensify the energy-loss peak at 4.4 eV which has been attributed to O–Cu–O dumbbells. 相似文献
999.
J. Wuttke M. Kiebel E. Bartsch F. Fujara W. Petry H. Sillescu 《Zeitschrift für Physik B Condensed Matter》1993,91(3):357-365
We present an extended set of incoherent neutron scattering measurements on the van der Waals liquido-terphenyl, obtained by time-of-flight and backscattering spectroscopy. In the supercooled liquid regime, data from three instruments are combined and analysed in terms of the selfcorrelationS(Q, t). In the time range 1...100 ps, the crossover from -to -relaxation is well described by the masterfunction of mode coupling theory, and fitted parameters are consistent with the previously established critical temperatureT
c
[Z. Phys. B83, 175 (1991)]. In the glassy regime, vibrations are harmonic and can be described by a density of states. Deviations at lowQ are quantitatively explained by a multiple scattering simulation. Throughout the article, experimental difficulties are discussed in some detail. 相似文献
1000.
S. E. Arnell D. Foltescu H. A. Roth Ö. Skeppstedt A. Nilsson S. Mitarai J. Nyberg 《Zeitschrift für Physik A Hadrons and Nuclei》1993,346(2):111-117
The level structure of92Ru has been studied by means of γ-ray spectroscopy. The nucleus was produced by the58Ni(40Ca, α2p)92Ru reaction at beam energies of 147 and 187 MeV. The NORDBALL detector system including particle selection was used. A large number of new levels with excitation energies up to 11.3 MeV and spin values up to 22 or 23 units of angular momentum have been established. The level scheme is compared with recent shell model calculations using100Sn as a core. Some systematics of the g 9 2/?2 configuration is discussed and a strong correlation between the levels in90Mo and92Ru is found. 相似文献