Coseismic and other short-term strain changes recorded with Sacks-Evertson strainmeters in a deep mine, South Africa   总被引：2，自引：0，他引：2  

A. McGarr  I. S. Sacks  A. T. Linde  S. M. Spottiswoode  R. W. E. Green 《Geophysical Journal International》1982,70(3):717-740

Summary. During 1977 March and April, three Sacks-Evertson borehole dilatometers were installed at the ends of boreholes drilled into the sidewall of an experimental tunnel at a depth of 3.1 km in the ERPM gold mine near Johannesburg. In the following year coseismic strain changes ranging from 5 ± 10⁻¹⁰ to values exceeding 5 ± 10⁻⁶ were recorded for hundreds of mine tremors in the magnitude range -1 to 3.7 and at hypocentral distances of 50 m to about 2 km. Hypocentral coordinates and magnitudes were determined from seismograms recorded from an underground array of geophones. Amplitudes and polarities of the coseismic strain steps are generally in excellent agreement with theoretical expectations based on point-source dislocation theory; specifically, the strain steps are proportional to the seismic moment divided by the cube of hypocentral distance. At a strain level of 5 ± 10⁻⁹ or greater the tremors do not appear to be preceded by any short-term indications of instability even for tremors producing coseismic steps greater than 5 ± 10⁻⁶ and for which the strainmeters were within a source radius of the hypocentre. Continuous strain changes observed at the times when the mine excavation, at a distance of about 100 m, is extended are in good agreement with calculated changes based on the theory of elasticity. A similar calculation is consistent with post-seismic strain changes observed to follow some of the closer tremors. These post-seismic strains show a logarithmic dependence on time following the tremor and appear to be due to the interaction of a tremor with the adjacent mine excavation rather than to deformation within the actual seismic source region.  相似文献   

The Magnetic Helicity Budget of a cme-Prolific Active Region     

Green  L.M.  López fuentes  M.C.  Mandrini  C.H.  Démoulin  P.  Van Driel-Gesztelyi  L.  Culhane  J.L. 《Solar physics》2002,208(1):43-68

Coronal mass ejections (CMEs) are thought to be the way by which the solar corona expels accumulated magnetic helicity which is injected into the corona via several methods. DeVore (2000) suggests that a significant quantity is injected by the action of differential rotation, however Démoulin et al. (2002b), based on the study of a simple bipolar active region, show that this may not be the case. This paper studies the magnetic helicity evolution in an active region (NOAA 8100) in which the main photospheric polarities rotate around each other during five Carrington rotations. As a result of this changing orientation of the bipole, the helicity injection by differential rotation is not a monotonic function of time. Instead, it experiences a maximum and even a change of sign. In this particular active region, both differential rotation and localized shearing motions are actually depleting the coronal helicity instead of building it. During this period of five solar rotations, a high number of CMEs (35 observed, 65 estimated) erupted from the active region and the helicity carried away has been calculated, assuming that each can be modeled by a twisted flux rope. It is found that the helicity injected by differential rotation (–7×10⁴² Mx²) into the active region cannot provide the amount of helicity ejected via CMEs, which is a factor 5 to 46 larger and of the opposite sign. Instead, it is proposed that the ejected helicity is provided by the twist in the sub-photospheric part of the magnetic flux tube forming the active region.  相似文献   

彩色印刷复制中色差公式加权系数的计算和可接受阈值的评价   总被引：1，自引：0，他引：1  

赵秀萍  Phil Green 《武汉大学学报(信息科学版)》2006,31(9):814-817

对印在有光泽的铜版纸上的9个颜色中心、共216种颜色色样进行了视觉评价和客观测量，得出了每种颜色中心的色差的可接受阈值；然后，应用视觉评价标准确定了可用于CIE94、CMC和CIE2000中的最佳l：c加权系数，并将△E94（l：c）、AEcmc（l：c）、DE2000（l：c）与△Eab进行了比较。  相似文献   

A 408-MHz variability study of two fields in the region 6^h30^m, +45°     

J. M. Riley  & D. A. Green 《Monthly notices of the Royal Astronomical Society》1998,301(1):203-209

Variability in 408-MHz flux density, over a 1-yr interval between 1995 and 1996, has been investigated using the DRAO Synthesis Telescope for a complete sample of 322 sources with S _408 MHz > 80 mJy at galactic latitude b  = 15°; four sources are found to show significant flux density variations. These results, taken with those from a similar study at b  = 58°, indicate that 408-MHz variability over a time-scale of 1 yr is more uncommon than has previously been thought; variations at a level >10 per cent could have been detected in a statistically complete sample of about 150 of these sources and none was found. Variability over a period of 18 yr has also been investigated by comparing the DRAO data with those from the B3 catalogue for 182 sources with S _408 MHz > 200 mJy; five variables are found. Large flux density variations over a period of 18 yr are much more common than over 1 yr, with roughly one source in 15 showing variations at the 15 per cent level or greater. The statistics are not good enough to show any conclusive evidence for a dependence of variability on galactic latitude. Roughly half of the variable sources have spectra that are steep at high frequencies and flatten at low frequencies; the other half have flat radio spectra over the entire frequency range. Simultaneous observations at 1420 MHz, also with the DRAO Synthesis Telescope, have been used to investigate variability at this frequency as well, and indicate that over a period of 1 yr roughly half of the flat-spectrum sources vary at the 5 per cent level or greater.  相似文献   

Improved ocean-geoid resolution from retracked ERS-1 satellite altimeter waveforms   总被引：6，自引：0，他引：6  

Stefan Maus  Chris M. Green  & J. Derek Fairhead 《Geophysical Journal International》1998,134(1):243-253

The ocean geoid can be inferred from the topography of the mean sea surface. Satellite altimeters transmit radar pulses and determine the return traveltime to measure sea-surface height. The ERS-1 altimeter stacks 51 consecutive radar reflections on board the satellite to a single waveform. Tracking the time shift of the waveform gives an estimate of the distance to the sea surface. We retrack the ERS-1 radar traveltimes using a model that is focused on the leading edge of the waveforms. While earlier methods regarded adjacent waveforms as independent statistical events, we invert a whole sequence of waveforms simultaneously for a spline geoid solution. Smoothness is controlled by spectral constraints on the spline coefficients. Our geoid solutions have an average spectral density equal to the expected power spectrum of the true geoid. The coherence of repeat track solutions indicates a spatial resolution of 31  km, as compared to 41  km resolution for the ERS-1 Ocean Product. While the resolution of the latter deteriorates to 47  km for wave heights above 2  m, our geoid solution maintains its resolution of 31  km for rough sea. Retracking altimeter waveform data and constraining the solution by a spectral model leads to a realistic geoid solution with significantly improved along-track resolution.  相似文献   

Sea level,climate change and coastal evolution in Morar,northwest Scotland     

Shennan  Ian  Tooley  Michael  Green  Frances  Innes  Jim  Kennington  Kevin  Lloyd  Jeremy  Rutherford  Mairead 《Geologie en Mijnbouw》1998,77(3-4):247-262

Analyses of geomorphologically contrasting sites in Morar, NW Scotland, describe the forcing mechanisms of coastal change. Isolation basins (i.e. basins behind rock sills and now isolated from the sea following isostatic uplift) accumulated continuous marine and freshwater sediments from c.12 to 2 ka BP. Raised dune, marsh and wetland sites register breaching, migration and stability of dunes from c. 9 to 2 ka BP. High-resolution methods designed to address issues of macroscale and microscale sea-level changes and patterns of storminess include 1-mm sampling for pollen, dinocyst and diatom analyses, infra-red photography, X-ray photography and thin-section analysis. The data enhance the record of relative sea-level change for the area. Major phases of landward migration of the coast occurred during the period of low sea-level rise in the mid-Holocene as the rate of rise decreased from c. 3 to < 1 mm/year. Relative sea-level change controls the broad pattern of coastal evolution at each site; local site-specific factors contribute to short-term process change. There is no record of extreme events such as tsunami. Within a system of dynamic metastable equilibrium, the Holocene records show that site-specific factors determine the exact timing of system breakdown, e.g. dune breaching, superimposed on regional sea-level rise. The global average sea-level rise of 3 to 6 mm/yr by AD 2050 predicted by IPCC would only partly be offset in the Morar area by isostatic uplift of about 1 mm/yr. A change from relative sea-level fall to sea-level rise, in areas where the regional rate of uplift no longer offsets global processes, is a critical factor in the management of coastal resources.  相似文献   

Possible formation scenarios for the giant H i envelope around the NGC 4490/4485 system     

M. S. Clemens  P. Alexander  & D. A. Green 《Monthly notices of the Royal Astronomical Society》1998,297(4):1015-1020

We present observations of H i in the nearby interacting galaxies NGC 4490 and 4485 made with the VLA in both C and D arrays. The galaxies are embedded in an extensive envelope of neutral hydrogen which is elongated in a direction approximately perpendicular to the plane of NGC 4490, with an extent of about 56 kpc. We argue that this distribution of neutral hydrogen can best be explained by a galactic-scale bipolar outflow of H  i driven by supernovae in NGC 4490. The flow from the disc appears to be reasonably well collimated and has probably persisted for approximately 6 × 10⁸ yr. The implications for galaxy evolution when such mass loss occurs are briefly discussed.  相似文献   

Experimental duplication of a high-pressure megacryst/cumulate assemblage in a near-saturated hawaiite     

Janice Knutson  Trevor H. Green 《Contributions to Mineralogy and Petrology》1975,52(2):121-132

The occurrence of corroded megacrysts and cumulates of olivine, clinopyroxene, orthopyroxene, plagioclase, ilmenite and apatite in near-saturated hawaiites from the mid-north coast of New South Wales point to the derivation of these hawaiites at elevated pressures. In an experimental study on one of these hawaiites under conditions ranging from 5–15 kb and 0–5% H₂O, orthopyroxene was identified in only one run with 2% H₂O at 1040° C and 6.5 kb. In this run it was associated with olivine, clinopyroxene and Fe-Ti oxide. The early appearance of plagioclase in the “dry” experimental runs and amphibole in runs with 5% H₂O, indicates that the water content in the natural hawaiite was intermediate to these values. The near-duplication of the natural megacryst-cumulate assemblage suggests that the hawaiite host precipitated these phases at a depth of approximately 20–24 km, prior to rapid eruption to higher crustal levels.  相似文献   

River channel changes | .K.J. Gregory, 1977. Wiley and Sons,Chichester, 448 pp., £ 19.00, U.S. $ 35.00     

C.P. Green 《Earth》1979,14(3):296-297

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A chart for designing modal analysis by point counting     

Dr. M. Solomon  Dr. R. Green 《International Journal of Earth Sciences》1966,55(3):844-848

Developing the work ofHasofer (1963) andSolomon (1963) concerning the factors controlling the precision of point counting, the authors have designed a chart to facilitate the choice of grid-spacing and sample area for individual minerals. After determining the grain radius, and making a rough estimate of the percentage of the mineral under investigation, suitable combinations of grid-spacing and number of counts can be rapidly determined from the chart.

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Zusammenfassung Diese Arbeit stellt eine Weiterentwicklung derjenigen vonHasofer (1963) undSolomon (1963) dar, die sich mit den Faktoren befaßten, welche die Genauigkeit der Punktezählung bestimmen. Die Autoren haben eine Tabelle entworfen, welche die Wahl der graphostatischen Abstände und des Mustergebietes für einzelne Mineralien erleichtert.

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Résumé Développant le travail deHasofer (1963) et deSolomon (1963) sur les facteurs qui déterminent la précision du compte par points, les auteurs ont élaboré un diagramme pour faciliter le choix du quadrillage et de la superficie d'essai pour des minéraux particuliers.

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