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981.
982.
983.
L. K. Erastova 《Astrophysics》2011,54(1):143-145
Plates from the Second Byurakan Survey reveal two large increases in the brightness of this star in 1972 and 1975. Spectra
of this variable have been obtained for the first time. It is not visible in plate H2133 from the Hamburg survey, which has
a limiting brightness of ~18m. Our data confirm that the star is an eruptive variable, most likely of the U Gem type. 相似文献
984.
Mohamed F. YASSIN 《大气科学进展》2009,26(6):1241-1252
To assist validation of the experimental data of urban pollution dispersion, the effect of
an isolated building on the flow and gaseous diffusion in the wake region have been investigated
numerically in the neutrally stratified rough-walled turbulent boundary layer. Numerical studies were
carried out using Computational Fluid Dynamics (CFD) models. The CFD models used for the simulation
were based on the steady-state Reynolds-Average Navier-Stoke equations (RANS) with κ-ε
turbulence models; standard κ-ε and RNG κ-ε models. Inlet conditions
and boundary conditions were specified numerically to the best information available for each fluid modeling
simulation. A gas pollutant was emitted from a point source within the recirculation cavity behind the
building model. The accuracy of these simulations was examined by comparing the predicted results with wind
tunnel experimental data. It was confirmed that simulation using the model accurately reproduces the velocity
and concentration diffusion fields with a fine-mish resolution in the near wake region. Results indicated that
there is a good agreement between the numerical simulation and the wind tunnel experiment for both wind flow
and concentration diffusion. The results of this work can help to improve the understanding of mechanisms of
and simulation of pollutant transport in an urban environment. 相似文献
985.
Chung-Lin SHIE Long S. CHIU Robert ADLER Eric NELKIN I-I LIN Pingping XIE Feng-Chin WANG R. CHOKNGAMWONG William OLSON D. Allen CHU 《大气科学进展》2009,26(6):1071-1080
Accurate sea surface flux measurements are crucial for
understanding the global water and energy cycles. The oceanic
evaporation, which is a major component of the global oceanic fresh
water flux, is useful for predicting oceanic circulation and
transport. The global Goddard Satellite-based Surface Turbulent
Fluxes Version-2 (GSSTF2; July 1987--December 2000) dateset that was
officially released in 2001 has been widely used by scientific
community for global energy and water cycle research, and regional
and short period data analyses. We have recently been funded by NASA
to resume processing the GSSTF dataset with an objective of
continually producing a uniform dataset of sea surface turbulent
fluxes, derived from remote sensing data. The dataset is to be
reprocessed and brought up-to-date (GSSTF2b) using improved input
datasets such as a recently upgraded NCEP/DOE sea surface
temperature reanalysis, and an upgraded surface wind and microwave
brightness temperature V6 dataset (Version 6) from the Special
Sensor Microwave Imager (SSM/I) produced by Remote Sensing Systems
(RSS). A second new product (GSSTF3) is further proposed with a
finer temporal (12-h) and spatial (0.25ox0.25o)
resolution. GSSTF2b (July 1987--December 2008) and GSSTF3 (July
1999--December 2009) will be released for the research community to
use by late 2009 and early 2011, respectively. 相似文献
986.
987.
Irregularly shaped (IRS) particles widely exist in many engineering and industrial fields. The macro physical and mechanical properties of the particle system are governed by the interaction between the particles in the system. The interaction between IRS particles is more complicated because of their complex geometric shape with extremely irregular and co‐existed concave and convex surfaces. These particles may interlock each other, making the sliding and friction of IRS particles more complex than that of particles with regular shape. In order to study the interaction of IRS particles more efficiently, a refined method of constructing discrete element model based on computed tomography scanning of IRS particles is proposed. Three parameters were introduced to control the accuracy and the number of packing spheres. Subsequently, the inertia tensor of the IRS particle model was optimized. Finally, laboratory and numerical open bottom cylinder tests were carried out to verify the refined modeling method. The influence of particle shape, particle position, and mesoscopic friction coefficient on the interaction of particles was also simulated. It is noteworthy that with the increase of mesoscopic friction coefficient, the fluidity of IRS particle assembly decreases, and intermittent limit equilibrium state may appear. Copyright © 2014 John Wiley & Sons, Ltd. 相似文献
988.
989.
By using the results of processing of the instrumental data with high space resolution obtained in September 2008, we analyze
the structure of the Rim Current in the upper 100-m layer near the coast of Crimea. We determine the statistical characteristics
of the mesoscale fluctuations of currents according to the data of 1165 vertical probes. It is shown that the kinetic energy
of intense mesoscale perturbations observed in the vicinity of the Rim Current is of the same order of magnitude as the kinetic
energy of the mean current. 相似文献
990.