Variability associated with α accretion disc theory for standard and advection-dominated discs     

Eric G. Blackman 《Monthly notices of the Royal Astronomical Society》1998,299(4):L48-L52

The α turbulent viscosity formalism for accretion discs must be interpreted as a mean field theory, modelling a steady state only on spatial or time-scales greater than those of the turbulence. The extent of the scale separation determines the relative precision error (RPE) of the predicted luminosity L _ν. Turbulence and the use of α implies that (1) field line stretching gives a magnetic pressure  α²/6 of the total pressure generally, and a one-to-one relation between α and the pressure ratio for thin discs, and (2) large turbulent scales in advection-dominated accretion flows (ADAFs) predict a lower L _ν precision than thin discs for a given observation duration and central mass. The allowed variability (or RPE) at frequency ν increases with the size of the contributing region. For X-ray binary ADAFs, the RPE ∼ 5 per cent at R  ≤ 1000 Schwarzchild radii ( R _s) for averages over  1000 s. However, current data for galaxies like NGC 4258 and M87 give RPEs in L _ν of 50–100 per cent even at R  ≤ 100  R _S. More data are required, but systematic deviations from ADAF predictions are more significant than random deviations, and may constrain properties of the turbulence, the accretion mode, the assumption of a steady state or the accretion rate.  相似文献   

Reviews     

Daniel F. Merriam  R. A. Reyment  John W. Harbaugh  Eric C. Dahlberg  Marie Morisawa 《Mathematical Geosciences》1975,7(5-6):485-492

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The geologic history of the Nicoya Ophiolite Complex, Costa Rica, and its geotectonic significance     

Eric P. Kuijpers 《Tectonophysics》1980,68(3-4)

Costa Rica forms part of an intra-oceanic arc between the Pacific and Caribbean oceans; the Nicoya Ophiolite Complex is located along its Pacific border. In this study, evidence is given that the Nicoya Complex is composed of ridge-formed oceanic crust that suffered a strong compressional stress during Late Santonian times. As a result of this, isoclinal folding and large-scale nappe emplacement occurred at a shallow crustal depth. The principal component of this compressional stress was E-W-directed. It is also demonstrated that, from this time, the complex was situated between a subducting plate and a volcanic arc. From that Campanian until the Middle Eocene the zone was undulated, and generally at a great depth below sea level. During the Eocene—Oligocene epoch a new tectonic stress affected the area. It produced open folding with upthrusting in the ophiolite complex and overthrust folding of the overlying rock series. As a result of crustal thickening during this tectonic phase, the area was uplifted. From Miocene times, the zone was shaped into a dome and a synform. These undulations are attributed to compression of the subducting Coco Plate, west of the area.The Upper Santonian tectonic phase demonstrates how compressional stress produced the break-up of the Caribo-Pacific plate west of the study area, as a result of which, a Caribbean plate without an associated oceanic ridge and a Pacific plate originated. The compressional stress in question was presumably generated by the opposed spreading directions of the new Mid-Atlantic Ridge and an older ridge to the west of the study area.Furthermore, it is argued that the Cretaceous obduction of the ophiolite belt along the Pacific coast of the American continents, was produced by the directional change of these continents during the birth of the Mid-Atlantic Ridge. This created intra-plate compressional stress and converted originally passive continental margins into active zones, where thrusting of oceanic crust on to a continental margin (obduction) could occur. When the Mid-Atlantic Ridge started spreading, the obduction phase ended due to subduction of the oceanic plate below the leading edge of the continent.  相似文献   

Upper Limit of Iodine Oxide in the Lower Stratosphere     

Irene Pundt  Jean-Pierre Pommereau  Celine Phillips  Eric Lateltin 《Journal of Atmospheric Chemistry》1998,30(1):173-185

It has been suggested that iodine oxides, IOx, could play a significant role in the ozone destruction in the lower stratosphere. To investigate this suggestion, spectra from nine SAOZ uv-visible spectrometer balloon flights were examined for the IO absorption signature between 405 and 450 nm. IO was not detected, either at mid- or high latitude, in the morning or the evening, in summer or winter. An upper limit of 0.2 parts per trillion by volume (pptv) at 20 km and 0.1 pptv at 15 km at the 95% confidence level (2), was derived from the best measurements at 90° SZA at sunset and sunrise. Since a photochemical model shows that 70% of inorganic iodine should be in the form IO at that time, it is concluded that unless iodine chemistry is different from that assumed at the moment, the role of iodine in stratospheric ozone depletion is small.  相似文献   

Uncertainty assessment and analysis of the calibrated parameter values of an urban storm water quality model   总被引：1，自引：0，他引：1  

Eric Gaume  Jean-Pierre Villeneuve  Michel Desbordes 《Journal of Hydrology》1998,210(1-4):38-50

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Phosphate in Angra dos Reis: Structure and composition of the Ca₃(PO₄)₂ minerals     

Eric Dowty 《Earth and Planetary Science Letters》1977,35(2):347-351

Extraterrestrial calcium phosphates (“whitlockites”) have the anhydrous β-Ca₃(PO₄)₂ structure, which is different from that of hydrous terrestrial whitlockite. This has been confirmed by X-ray refinement of the structure of a phosphate from the achondrite Angra dos Reis. In the β-Ca₃(PO₄)₂ structure, there is one crystallographic site, Ca(IIA), which is half-occupied by calcium, and which seems to have an energetically unfavorable configuration; natural phosphates with this configuration (including Angra dos Reis) have composition Ca₁₉(Mg,Fe)₂(PO₄)₁₄. Stability of the structure is probably increased by substitution of Na for Ca in Ca(IIA) giving composition Ca₁₈ (Mg,Fe)₂Na₂(PO₄)₁₄, which occurs in chondrites; by vacancy of Ca(IIA), with rare earths and yttrium substituting for calcium in other sites for charge balance, giving composition Ca₁₆(Y,RE)₂(Mg,Fe)₂(PO₄)₁₄, found in lunar rocks; or by replacing Ca with hydrogen, giving composition Ca₁₈(Mg,Fe)₂H₂(PO₄)₁₄, which is terrestrial whitlockite. Lack of the favorable substitutions of Na, (Y, RE) or H in Angra dos Reis phosphate implies that these elements were relatively scarce in its environment of formation.  相似文献   

The importance of adsorption in igneous partitioning of trace elements     

Eric Dowty 《Geochimica et cosmochimica acta》1977,41(11):1643-1646

For accurate mathematical modeling of trace-element partitioning during igneous fractionation, adsorption should be considered. Because of adsorption, the partitioning of elements between liquid and a surface layer of a crystal is often not the same as the partitioning between liquid and the solid crystal at true equilibrium. In some minerals e.g. high-calcium pyroxene, the effect of adsorption during crystal growth may be very important; this is suggested by the frequent occurrence of sector zoning in augite, and the wide range in measured partition coefficients for such elements as rare earths. The ions which are enriched by adsorption are usually those which are favored substituents according to Goldschmidt's rules. In other minerals, uptake of trace elements may be closer to equilibrium partitioning, rather than being determined by kinetic factors. For example, the relative partitioning of REE, U, Th and Pb into feldspars is qualitatively predicted by Pauling's rules for complex ionic crystals, rather than by Goldschmidt's rules.  相似文献   

Ferroan anorthosite: A widespread and distinctive lunar rock type     

Eric Dowty  Martin Prinz  Klaus Keil 《Earth and Planetary Science Letters》1974,24(1):15-25

Eight of eleven Apollo 16 rake-sample anorthosites are very similar to each other, to hand-specimen Apollo 16 anorthosites, and to Apollo 15 anorthosites. They have feldspar An_96.6, both high- and low-Ca pyroxene with a restricted range of (low-magnesium) composition, minor olivine (～ Fo₆₀), traces of ilmenite and chromite, and originally coarse-grained, but now cataclastic texture. Such ferroan anorthosite is evidently a coherent, distinctive and widespread lunar rock type of cumulate origin which may not necessarily be very closely related genetically to other highland rock types.  相似文献   

Dr Donald S. McLusky – An appreciation and thanks from ECSS     

Eric WolanskiIvan Valiela  Mike Elliott 《Estuarine, Coastal and Shelf Science》2010

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Numerical local analysis of relevant internal variables for constitutive modelling of granular materials     

Yuhanis Yunus  Eric Vincens  Bernard Cambou 《国际地质力学数值与分析法杂志》2010,34(11):1101-1123

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