Application of MELTS to kinetic evaporation models of FeO‐bearing silicate melts     

C. M. O'D. ALEXANDER 《Meteoritics & planetary science》2002,37(2):245-256

Abstract— Incorporation of the MELTS silicate melt solution model into models of evaporation successfully reproduces the evaporation behavior of alkali‐free, FeO‐bearing (≥2 mol%) chondritic melts at temperatures between 1700 and 2000 °C. In conjunction with the Berman CMAS melt solution model for FeO‐poor melts, evaporation of alkali‐free melts can now be modeled over a very wide range of conditions. MELTS‐based evaporation models can also quite successfully reproduce the evaporation behavior of K when Al/(Na + K) > 1. However, reproduction of Na evaporation experiments is much poorer.  相似文献   

RESISTIVITY ANALYSIS FOR MODELS OF A SPHERE IN A HALF-SPACE WITH BURIED CURRENT SOURCES*     

R. H. MERKEL  S. S. ALEXANDER 《Geophysical Prospecting》1971,19(4):640-651

Boundary-value problems in steady-state current flow were solved numerically in bispherical coordinates for a sphere of arbitrary conductivity in a half-space. Solutions for the potential on the surface of the half-space were examined for the cases where both current sources were on the surface, one source on the surface and the second between the surface and the sphere, and one source on the surface and the other in the sphere. Results show a great similarity with the layered case when the buried electrode is placed between the surface and the conducting region. Such a buried electrode configuration makes it possible to obtain an accurate measurement of the depth to the conductor in both cases. A model with the current electrode placed in a conductive sphere is compared with a three-layered model with the source in a conductive intermediate layer, and results indicate that the lateral extent of a finite anomalous zone can be estimated using these limiting curves. The validity of these theoretical calculations for buried spheres was confirmed experimentally by tests conducted on an analog model.  相似文献   

The Skaergaard Layered Series, Part VII: Sr and Nd Isotopes   总被引：2，自引：0，他引：2  

McBIRNEY  ALEXANDER R.; CREASER  ROBERT A. 《Journal of Petrology》2003,44(4):757-771

The initial isotopic ratios of strontium and neodymium in theSkaergaard Layered Series vary both vertically and laterally,on every scale from the intrusion as a whole down to coexistingminerals in a single rock. The magma that filled the Skaergaardchamber was contaminated to various degrees with the metamorphicrocks through which it rose and was never completely homogenizedafter being intruded. The contamination was most pronouncedin contact zones and aureoles around rare xenoliths. The greaterconcentrations of lithophile trace elements in the Upper BorderSeries was previously attributed to assimilation of buoyantfragments of gneiss that collected under the roof, but mostof the rocks of the Upper Border Series are isotopically indistinguishablefrom those of the Layered Series. It is doubtful, therefore,that this part of the intrusion assimilated much more of themetamorphic basement than did the rest of the magma. Similarly,the marked increase in the concentrations of excluded elementsin the upper part of the Layered Series is not matched by achange in the isotopic character of the rocks and cannot beattributed to a later influx of new magma. Analyses of mineralsseparated from rocks with exceptionally mafic or felsic modalcompositions revealed marked inhomogeneities in the isotopiccompositions of their constituent minerals. For example, coexistingplagioclase and pyroxene from closely associated anorthositesand pyroxenites have very different initial isotopic ratiosof both strontium and neodymium. The same is true of mafic andfelsic layers in modally graded gabbros. These differences areunrelated to the low-temperature alteration shown by oxygenisotopes. They must have been introduced when the original gabbrowas largely crystallized and underwent local metasomatic replacementby nearly mono-mineralic mafic and felsic assemblages. KEY WORDS: Nd isotopes; Skaergaard; Sr isotopes  相似文献   

Elemental redistribution in Tieschitz and the origin of white matrix     

ROBERT HUTCHISON  CONEL M.O'D. ALEXANDER  JOHN C. BRIDGES 《Meteoritics & planetary science》1998,33(5):1169-1179

Abstract— Two types of mesostasis coexist within some porphyritic chondrules in Tieschitz. One type is smooth. The other, confined to chondrule margins, is blocky on a 5–10 μm scale. Mesostases in one porphyritic olivine-pyroxene (POP) chondrule and one porphyritic olivine (PO) chondrule were analysed by scanning electron microscopy (SEM) and energy-dispersive x-ray spectrometry (EDS), as was white matrix nearby. Mesostases in the PO chondrule and in four others were analysed by ion probe. Pyroxene phenocrysts or dendrites extend across contacts between smooth and blocky mesostasis with no compositional change. Relative to smooth mesostasis, blocky mesostasis is enriched in Al, alkalis, Ba, F, and Cl but depleted in Si, Fe, and Ca. White matrix fills channels between the chondrules. It is physically and chemically similar to blocky mesostasis, but three ion probe analyses indicate that, unlike the mesostases, it is poor in Sc and has variable and fractionated rare earth elements (REEs). Smooth mesostasis is interpreted as solidified primary chondrule liquid; whereas blocky mesostasis is its alteration product or, less likely, a precipitate replacing smooth mesostasis leached out by aqueous fluid. White matrix may have formed by secondary alteration or replacement of mesostases that had been expelled from chondrules during accretion, or as a precipitate filling interchondrule voids. Iron may have been lost from the bulk meteorite, but most other elements merely underwent internal redistribution. Disturbed isotopic systems indicate that aqueous fluid may have been active on the Tieschitz parent body only 2 Ga ago. If correct, this would be the first evidence that an ordinary chondrite parent body underwent internal reprocessing significantly later than 4.5 Ga ago.  相似文献   

Large-scale structure of Calamus River deposits (Nebraska, USA) revealed using ground-penetrating radar   总被引：2，自引：0，他引：2  

JOHN BRIDGE  RICHARD COLLIER  & JAN ALEXANDER 《Sedimentology》1998,45(6):977-986

The large-scale (i.e. bar-scale) structure of channel deposits of the braided, low-sinuosity Calamus River, Nebraska, is described using ground-penetrating radar (GPR) profiles combined with vibracores. Basal erosion surfaces are generally overlain by medium-scale, trough-cross-stratified (sets 3–25 cm thick), very coarse to medium sands, that are associated with relatively high amplitude, discontinuous GPR reflectors. Overlying deposits are bioturbated, small-scale cross-stratified (sets <3 cm thick) and vegetation-rich, fine to very-fine sands, that are associated with low-amplitude discontinuous reflectors. Near-surface peat and turf have no associated GPR reflectors. In along-stream profiles through braid and point bars, most GPR reflectors dip downstream at up to 2° relative to the basal erosion surface, but some reflectors in the upstream parts of bars are parallel to the basal erosion surface or dip upstream. In cross-stream profiles through bars, GPR reflectors are either approximately parallel to bar surfaces or have low-angle inclinations (up to 6°) towards cut banks of adjacent curved channels. Basal erosion surfaces become deeper towards cut banks of curved channels. These structures can be explained by lateral and downstream growth of bars combined with vertical accretion. Convex upwards forms up to 0·5 m high, several metres across and tens of metres long represent episodic accretion of unit bars (scroll bars and bar heads). Stratal patterns in channel fills record a complicated history of erosion and deposition during filling, including migration of relatively small bars. A revised facies model for this type of sandy, braided river has been constructed based on this new information on large-scale bedding structure.  相似文献   

Tyatya Volcano, southwestern Kuril arc: Recent eruptive activity inferred from widespread tephra   总被引：2，自引：0，他引：2  

MITSUHIRO  NAKAGAWA  YOSHIHIRO  ISHIZUKA †  TAKASHI  KUDO  MITSUHIRO  YOSHIMOTO ‡  WATARU  HIROSE  YOSHIO  ISHIZAKI  NOBUO  GOUCHI  YOSHIO  KATSUI  ALEXANDER W.  SOLOVYOW  GENRIKH S.  STEINBERG  ARSLAN I.  ABDURAKHMANOV 《Island Arc》2002,11(4):236-254

Abstract Tyatya Volcano, situated in Kunashir Island at the southwestern end of Kuril Islands, is a large composite stratovolcano and one of the most active volcanoes in the Kuril arc. The volcanic edifice can be divided into the old and the young ones, which are composed of rocks of distinct magma types, low‐ and medium‐K series, respectively. The young volcano has a summit caldera with a central cone. Recent eruptions have occurred at the central cone and at the flank vents of the young volcano. We found several distal ash layers at the volcano and identified their ages and sources, that is, tephras of ad 1856, ad 1739, ad 1694 and ca 1 Ka derived from three volcanoes of Hokkaido, Japan, and caad 969 from Baitoushan Volcano of China/North Korea. These could provide good time markers to reveal the eruptive history of the central cone, which had continued intermittently with Strombolian eruptions and lava flow effusions since before 1 Ka. Relatively explosive eruptions have occurred three times at the cone during the past 1000 years. We revealed that, topographically, the youngest lava flows from the cone are covered not by the tephra of ad 1739 but by that of ad 1856. This evidence, together with a report of dense smoke rising from the summit in ad 1812, suggests that the latest major eruption with lava effusion from the central cone occurred in this year. In 1973, after a long period of dormancy, short‐lived phreatomagmatic eruptions began to occur from fissure vents at the northern flank of the young volcano. This was followed by large eruptions of Strombolian to sub‐Plinian types occurring from several craters at the southern flank. The 1973 activity is evaluated as Volcanic Explosivity Index = 4 (approximately 0.2 km³), the largest eruption during the 20th century in the southwestern Kuril arc. The rocks of the central cone are strongly porphyritic basalt and basaltic andesite, whereas the 1973 scoria is aphyric basalt, suggesting that magma feeding systems are definitely different between the summit and flank eruptions.  相似文献   

Further Considerations of Double-Diffusive Stratification and Layering in the Skaergaard Intrusion     

MCBIRNEY  ALEXANDER R. 《Journal of Petrology》1985,26(4):993-1001

Depending on the orientation of thermal and compositional gradientsat the margins of a cooling intrusion, double-diffusive convectionmay take one of two principal forms. If the body is coolingat a steep wall, so that both gradients are horizontal, theresult can be boundary layer flow up or down the wall and segregationof the fractionated liquid under the roof or on the floor. Ifcooling is through the roof or floor of a broad sheet-like body,the gradients will be vertical and if the physical propertiesof the liquid are appropriate, they could lead to broad horizontallystratified convection. The first case has been analysed by Nilsonet al. (1985) and shown to be a physically plausible explanationfor certain types of zoned magmas, but the second case, in whichboth gradients are vertical, appears to be less likely, especiallyin slowly cooled intrusions in which temperatures are controlledby crystal-liquid equilibrium. Depending on whether the magma is losing heat through its roofor floor and on whether its density increases or decreases withcooling and differentiation, four possible conditions are possible.A linear stability analysis based on the experimental and theoreticalcriteria of Baines & Gill (1969) and Shirtcliffe (1969)indicates that neither calc-alkaline liquids that accumulateunder their roof nor tholeiitic liquids ponded on their floorare likely to convect in stratified layers. Even though thegradients and relative diffusivities of heat and compositionmay be in a direction that tends to destabilize the magma, themagnitude of the compositional effect on density is so greatthat the temperature gradient would have to diverge widely fromthe liquidus, and convection would be possible only with largeamounts of under-cooling or superheat. A similar mechanism, based on opposed gradients of two chemicalcomponents of differing diffusivities, may provide an alternativeexplanation for certain types of stratification, but field relationsin the Skaergaard Intrusion do not support any origin that isprimarily dependent on gravity.  相似文献   

Laboratory sustained turbidity currents form elongate ridges at channel mouths     

JAN ALEXANDER  STUART J. MCLELLAND†  THOMAS E. GRAY  CHRIS E. VINCENT  MIKE R. LEEDER  SUSANNA ELLETT 《Sedimentology》2008,55(4):845-868

The turbulent flow structure, suspended sediment dynamics and deposits of experimental sustained turbidity currents exiting a channel across a break in slope into a wide tank are documented. The data shed light on the flow evolution and deposit geometry of analogous natural channel‐fed submarine fans. Flows generated in a 0·3 m wide, sloping (0°, 6°, 9° or 20°) channel crossed an angular slope break and spread onto a horizontal tank floor. Flow development comprised: (i) channelized phase (unsteady channel flow developing into steady channel flow); (ii) initial lateral expansion phase (unsteady‐spreading wall jet phase); (iii) constant lateral expansion phase (steady‐spreading wall jet phase); and (iv) rapid waning phase. Phases (i) and (iv) are similar to laterally constrained turbidity currents, but phases (ii) and (iii) are considerably different from such two‐dimensional currents. Steeper channel slopes produced greater flow velocities and turbulence intensities, but these effects diminished markedly with distance from the channel mouth. Flow velocity vectors in the tank had similar patterns for all channel slopes, with a central core of faster velocity and narrow vector dispersion and slower flow with larger dispersion at the jet margins. Suspended sediment concentrations were higher within flow heads and dense basal layers in flow bodies. Time‐averaged acoustic backscatter data showed vertical concentration gradients, confirmed by siphon samples. The deposits comprised a thick central ridge, of similar order width to the channel mouth, with abrupt margins and a surrounding, very thin, fan‐like sheet. The ridge was coarser grained and better sorted than the original sediment, with grain‐size fining downstream, particularly over the fan‐like sheet. The formation of a central ridge suggests that, in the tank, vertical turbulent momentum exchange is more significant for sediment dynamics than spanwise momentum exchange due to lateral expansion. The streamwise elongate geometry of the ridge contrasts with conventional fan‐like geometry found with surge‐type turbidity flows, a result that has widespread stratigraphic and economic implications.  相似文献   

Presolar silicon carbide from the Indarch (EH4) meteorite: Comparison with silicon carbide populations from other meteorite classes     

SARA S. RUSSELL  ULRICH OTT  CONEL M. O'D. ALEXANDER  ERNST K. ZINNER  JOHN W. ARDEN  C. T. PILLINGER 《Meteoritics & planetary science》1997,32(5):719-732

Abstract— Presolar SiC from the Indarch (EH4) meteorite was studied by scanning electron microscopy (SEM), by ion probe analysis for C and Si isotopic compositions, and by static source mass spectrometry for noble gas and C isotopic compositions. The data obtained are compared to SiC data from other meteorites, especially from Murchison (CM2), for which there is the most information available. The isotopic compositions of the major elements in SiC from Indarch and Murchison are similar. Stepped combustion data suggest a mean δ¹³C for SiC from both meteorites of ～+1430%o. Silicon isotopes in Indarch and Murchison SiC also compare well. In some other important respects, however, SiC in the two meteorites are different. Morphologically, SiC from Indarch appears finer grained than SiC from Murchison and is entirely composed of submicron grains. The finer-grained nature of Indarch SiC is confirmed by its noble gas characteristics. The mean Ne-E/Xe-S ratio for bulk Indarch SiC is significantly lower than the same ratio in Murchison (625 ± 47 vs. ～3500) but is similar to that of the finest grain-size fractions (<1 μm) in Murchison. A comparison of noble gas data from SiC from several different meteorites suggests that it might be Murchison SiC, rather than Indarch SiC, that is unusual. The grain-size disparities in SiC between meteorites are difficult to explain by residue processing differences or differing parent body processing. Instead, we speculate that a grain-size sorting mechanism for SiC may have operated in the solar nebula.  相似文献   

Physiological adaptations in Coleoptera on Spitsbergen     

JOHN ALEXANDER STRøMME  THOMAS WANJOHI NGARI  KARL ERIK ZACHARIASSEN 《Polar research》1986,4(2):199-204

Metabolic rates and Q₁₀ values were determined for three species of Spitsbergen Coleoptera, Amara quenseli, Simplocaria metallica and Rhynchaenus flagellum . The beetles had metabolic rates which were elevated compared to values of Coleoptera from other regions. This is interpreted as an adaptation to the prevailing low temperatures and short activity period on Spitsbergen.
A. quenseli had rates of water loss comparable to values of beetles in temperate and tropical xeric habitats, indicating that the habitat of the beetles on Spitsbergen at least occasionally is xeric.
Determination of cold-hardiness parameters such as supercooling point and haemolymph melting point of A. quenseli beetles revealed that the beetles had values corresponding to those of active insects in the temperate and tropical region. They had no thermal hysteresis factors. Thus, during summer they show no physiological adaptations to cold.  相似文献