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121.
There have been many studies of the retail industry in recent years, and of the impact that retailing has had on the spatial arrangement of urban areas and on consumer behaviour. Little attention has been paid, however, to employment in retailing, which is disturbing in view of its growing importance and its rapidly changing nature and composition. This paper examines the nature of the broad structural changes within the industry, and investigates their spatial consequences through a case study of employment generation within a system of suburban retail centres in Canberra, Australia. It is shown that the evolution of suburban centres, particularly those of a regional variety, has had an important and enriching impact on the suburban labour market. The regional centres are also seen to be the focus of the major structural employment changes currently affecting the retail industry. This has some important implications for urban planning. 相似文献
122.
A conspicuous graben extends for 800 kilometers through El Salvador and western Nicaragua to the Caribbean Sea in northeastern Costa Rica. Like the smaller but structurally similar Semangko and Toba Depressions of northern Sumatra, the trough is clearly related to voluminous volcanic eruptions during Late Tertiary time. In the region around Lakes Managua and Nicaragua, where the depression is best defined and reaches its greatest dimension, a thick series of Tertiary sediments and volcanic rocks provides a means of interpreting the Cenozoic history of the region. Following a long period of intermittent volcanic activity and sedimentation, extensive sheets of andesitic and dacitic ignimbrites were erupted during Late Miocene time from fissure sources which appear to have been located near the now-subsided central portion of the graben. Near the coast, ignimbrites flowed across a flat lagunal shore overwhelming and burying the tropical vegetation and finally coming to rest in shallow water. Unusual textures and chaotic mixtures of pumice with sediments and silicified wood characterize the bases of many of the water-laid ignimbrites. Subsidence of the graben does not appear to have occurred concurrently with the ignimbrite eruptions but followed them closely near the end of the Miocene or the beginning of Pliocene time. Subsequent activity has been confined to relatively smaller eruptions from central vents near the boundary faults of the graben. 相似文献
123.
124.
Alexander Roglinov Ludmil Christoskov Reviewer J. Vaněk 《Studia Geophysica et Geodaetica》1977,21(1):11-18
Summary Aki's spectral 2 model[1] is used to estimate the amplitude field at epicentral distances up to 1000 km in the case of an absorption coefficient of seismic waves which varies with distance. Velocity spectra, the periods of the maximum of these spectra and the maximum velocity amplitudes are obtained. The results are compared with[2] and it is shown that the divergence of the amplitude field decreases if a variable absorption coefficient is used. The theoretical results, obtained in this case, approach the results seen in practice. The possibility of determining the limits of epicentral distances, at which the amplitude field may be considered as linear, is given. 相似文献
125.
126.
Graphical Interpretation of Water-Quality Data 总被引:12,自引:0,他引:12
Alexander Zaporozec 《Ground water》1972,10(2):32-43
127.
David Alexander 《Astrophysics and Space Science》2007,307(1-3):197-202
The solar atmosphere displays a wide variety of dynamic phenomena driven by the interaction of magnetic fields and plasma.
In particular, plasma jets in the solar chromosphere and corona, coronal heating, solar flares and coronal mass ejections
all point to the presence of magnetic phenomena such as reconnection, flux cancellation, the formation of magnetic islands,
and plasmoids. While we can observe the signatures and gross features of such phenomena we cannot probe the essential physics
driving them, given the spatial resolution of current instrumentation. Flexible and well-controlled laboratory experiments,
scaled to solar parameters, open unique opportunities to reproduce the relevant unsteady phenomena under various simulated
solar conditions. The ability to carefully control these parameters in the laboratory allows one to diagnose the dynamical
processes which occur and to apply the knowledge gained to the understanding of similar processes on the Sun, in addition
directing future solar observations and models. This talk introduces the solar phenomena and reviews the contributions made
by laboratory experimentation. 相似文献
128.
We present a direct comparison between two different techniques: time-distance helioseismology and a local correlation tracking
method for measuring mass flows in the solar photosphere and in a near-surface layer. We applied both methods to the same
dataset (MDI high-cadence Dopplergrams covering almost the entire Carrington rotation 1974) and compared the results. We found
that, after necessary corrections, the vector flow fields obtained by these techniques are very similar. The median difference
between directions of corresponding vectors is 24°, and the correlation coefficients of the results for mean zonal and meridional
flows are 0.98 and 0.88, respectively. The largest discrepancies are found in areas of small velocities where the inaccuracies
of the computed vectors play a significant role. The good agreement of these two methods increases confidence in the reliability
of large-scale synoptic maps obtained by them. 相似文献
129.
130.
We investigate the possibility of explaining the observed ripples in the X-ray gas in the Perseus and Virgo clusters through
natural oscillations of a perturbed radio cocoon. Such a perturbation would result from an expanding overpressured cocoon
of radio plasma overshooting its pressure equilibrium point with the cluster gas. The oscillations are heavily acoustically
damped, and energy injection rates required to sustain them are consistent with observed AGN powers. Viscous dissipation of
sound waves generated by these oscillations heats the cluster gas. By comparing our model with observations in Perseus and
Virgo, we reproduce the observed ripple separations and amplitudes. Spitzer viscosity is largely sufficient in explaining
the gas density profile, suggesting that thermal conductivity is likely to be heavily suppressed. In the central regions,
viscous heating can suppress cooling flows on timescales exceeding the radio source lifetime. 相似文献