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71.
John Wilson Stewart Fotheringham Gary Hunter Jochen Albrecht 《Transactions in GIS》2006,10(2):153-153
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73.
Amy L Wolfe Ran Liu Brian W Stewart Rosemary C Capo David A Dzombak 《Geochemical transactions》2007,8(1):9
Background
Standardized sample preparation techniques allow comparison of pyrite dissolution experiments under diverse conditions. Our objective was to assess dry and wet sieving preparation methodologies, and to develop a reproducible technique that yields uniformly size-distributed material within a limited size range of interest. 相似文献74.
Tsunami deposits in the geological record 总被引:2,自引:0,他引:2
A review is presented here of tsunami deposits in the geological record. It begins with a discussion of the relationships between the processes of tsunami generation and propagation and the sedimentary responses. This is followed by a consideration of the sedimentary processes associated with the passage of tsunami waves across coastlines. Attention is also given to the sedimentary processes associated with tsunami-triggered gravity backwash flows and comparisons are made with turbidity current action. We observe that despite sedimentary evidence for recent tsunamiites, geological research on ancient tsunamis has not identified stratigraphic units associated with onshore tsunami sedimentation. Equally, it is noted that nearly all published studies of sedimentary processes associated with modern tsunamis have not considered patterns of sediment transport and deposition in the offshore zone. 相似文献
75.
The Sun's magnetic field extends far from the photosphere, into the corona, defining a magnetically dominated region before being drawn out radially by the solar wind flow. This region, where the internal sources of the solar field dominate the plasma structures and the energetic particle movement, can be properly considered the solar magnetosphere. The magnetic field in this region can be approximately described by models that extrapolate photospheric magnetic field observations under some simplifying assumptions. In this paper we use a potential field model which describes the solar field up to a source surface at 3.25 Rs, where the field is constrained to become radial. We present the variation of the magnitude and inclination of the various multipolar components throughout the solar magnetic cycle that characterise the changes in the structure of the solar magnetosphere over a period of 22 years. We also present some 3-D images of the coronal magnetic structure to show the global evolution of the solar magnetosphere throughout the solar cycle and discuss the importance of taking this structure into account in order to relate interplanetary and solar features. 相似文献
76.
A. Collier Cameron 《Astrophysics and Space Science》1998,261(1-4):71-80
I review recent progress in the field of stellar surface imaging, with particular reference to advanced methods for mapping
surface-brightness inhomogeneities and the surface vector magnetic field on magnetically active late-type stars. New signal
enhancement techniques, utilising profile information from hundreds or thousands of photospheric lines simultaneously, allow
images to be derived for stars several magnitudes fainter than was previously possible. For brighter stars, the same techniques
make it possible to map features as small as two or three degrees in extent on the stellar surface. This opens up whole new
areas of research, such as the ability to use starspot tracking to study surface differential rotation patterns on single
and binary stars, and to follow the secular evolution of the magnetic field itself.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
77.
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79.
A summary is given of the final results of measurements of cosmogenic Al26 activity in a total of 50 stone meteorites, mainly chondrites, carried out using coincidence gamma-spectrometry. 相似文献
80.
The finite-element method based on a Galerkin technique was used to formulate the problem of simulating the two-dimensional (cross-sectional) transient movement of water and solute in saturated or partially saturated nonuniform porous media. The numerical model utilizes linear triangular elements. Nonreactive, as well as reactive solutes whose behaviour can be described by a distribution coefficient or first-order reaction term were considered. The flow portion of the model was tested by comparison of the model results with experimental and finite-difference results for transient flow in an unsaturated sand column and the solute transport portion of the model was tested by comparison with analytical solution results. The model was applied to a hypothetical case involving movement of water and solutes in tile-drained soils. The simulation results showed the development of distinct solute leaching patterns in the soil as drainage proceeded. Although applied to a tile drainage problem in this study, the model should be equally useful in the study of a wide range of two-dimensional water and solute migration problems. 相似文献