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551.
P. Oliver M. Ralchenko C. Samson R. E. Ernst P. J. A. McCausland G. F. West 《Meteoritics & planetary science》2018,53(3):433-447
Ordinary chondrites have previously been nondestructively characterized using bulk magnetic susceptibility, broadly reflecting their Fe-Ni alloy content. We seek to expand the information that can be recovered from magnetic susceptibility by using the University of Toronto Electromagnetic Induction Spectrometer (UTEMIS) to measure the complex magnetic susceptibility tensor of 20 ordinary chondrites samples in addition to 16 Gao–Guenie (H5) chondrites at 35 frequencies from 90 Hz to 64 kHz, at variable low applied field strengths <10 A m−1. Following removal of the field-dependent component of susceptibility, frequency dependence, in- and out-of-phase components, and bulk magnetic susceptibility were interpreted. Most meteorites showed no frequency-dependent in-phase responses, but had a frequency-dependent out-of-phase response attributed to eddy currents induced in conductive minerals. Greater in- and out-of-phase frequency dependence correlated with lower fayalite content in olivine and was, in turn, inversely proportional to Fe-Ni alloy content. The uncertainty in the UTEMIS measurements ranges from approximately 0.05% for low-frequency in-phase measurements to a maximum of 3% for low-frequency out-of-phase measurements. This uncertainty level was far lower than the intra-meteorite variability for the Gao–Guenie suite suggesting inhomogeneity at scales of approximately 10 g. 相似文献
552.
Liebermannite,KAlSi3O8, a new shock-metamorphic,high-pressure mineral from the Zagami Martian meteorite 下载免费PDF全文
Chi Ma Oliver Tschauner John R. Beckett George R. Rossman Clemens Prescher Vitali B. Prakapenka Hans A. Bechtel Alastair MacDowell 《Meteoritics & planetary science》2018,53(1):50-61
In this paper, we discuss the occurrence of liebermannite (IMA 2013-128), KAlSi3O8, a new, shock-generated, high-pressure tetragonal hollandite-type structure silicate mineral, in the Zagami basaltic shergottite meteorite. Liebermannite crystallizes in space group I4/m with Z = 2, cell dimensions of a = 9.15 ± 0.14 (1σ) Å, c = 2.74 ± 0.13 Å, and a cell volume of 229 ± 19 Å3 (for the type material), as revealed by synchrotron diffraction. In Zagami, liebermannite likely formed via solid-state transformation of primary igneous K-feldspar during an impact event that achieved pressures of ~20 GPa or more. The mineral name is in honor of Robert C. Liebermann, a high-pressure mineral physicist at Stony Brook University, New York, USA. 相似文献
553.
Roshanravan Bijan Aghajani Hamid Yousefi Mahyar Kreuzer Oliver 《Natural Resources Research》2019,28(2):309-325
Natural Resources Research - Classification of spatial exploration data for exploration targeting using neuro-fuzzy models means that the many spatial values have to be simplified and assigned to a... 相似文献
554.
Roshanravan Bijan Aghajani Hamid Yousefi Mahyar Kreuzer Oliver 《Natural Resources Research》2019,28(3):1089-1105
Natural Resources Research - In this paper an improved prediction-area plot has been developed. This type of plot includes performance measures similar to other existing methods (receiver operating... 相似文献
555.
Krysia Mazik Will Musk Oliver Dawes Katya Solyanko Sue Brown Lucas Mander Mike Elliott 《Estuarine, Coastal and Shelf Science》2010
Intertidal mudflats are critical to the functional ecology of estuaries yet large areas are being lost as a result of land claim, erosion and coastal squeeze. This study examines whether managed realignment (at Paull Holme Strays, Humber estuary) can realistically achieve compensation for the loss of intertidal mudflat in the long term. Typical estuarine species quickly colonised the site with the total number of species recorded from the site as a whole being almost equal to that in the reference area within one year. Comparable biomass between the two areas was achieved after 2 years. However, organism abundance remains an order of magnitude lower within the realignment site compared to outside. Community structure within the realignment has changed from one characterised by terrestrial/freshwater organisms and early colonising species to one composed of typically estuarine species. However, the developing benthic communities only represent those typical of the estuary in areas of low elevation and high inundation frequency. Rapid accretion has favoured saltmarsh colonisation in much of the realignment site and this is expected to increase as accretion proceeds with invertebrate colonisation being inhibited by increasing elevation. Hence, realignment to restore intertidal mudflats can only be a short term solution in sites of high tidal elevation and in a dynamic and turbid estuary with high natural accretion rates, such as the Humber. 相似文献
556.
M. Plionis S. Basilakos M. Rowan-Robinson S. J. Maddox S. J. Oliver O. Keeble W. Saunders 《Monthly notices of the Royal Astronomical Society》2000,313(1):8-12
Comparing the gravitational acceleration induced on the Local Group of galaxies by different tracers of the underlying density field we estimate, within the linear gravitational instability theory and the linear biasing ansatz, their relative bias factors. Using optical SSRS2 galaxies, IRAS (PSC z ) galaxies and Abell/ACO clusters, we find b O,I ≈1.21±0.06 and b C,I ≈4.3±0.8, in agreement with other recent studies. Finally, there is an excellent one-to-one correspondence of the PSC z and Abell/ACO cluster dipole profiles, once the latter is rescaled by b C,I , out to at least ∼150 h −1 Mpc. 相似文献
557.
Stephen Serjeant Seb Oliver † Michael Rowan-Robinson Hans Crockett Vasilis Missoulis Tim Sumner Carlotta Gruppioni Robert G. Mann Nick Eaton David Elbaz David L. Clements Amanda Baker reas Efstathiou Catherine Cesarsky Luigi Danese Alberto Franceschini Reinhardt Genzel y Lawrence Dietrich Lemke Richard G. McMahon George Miley Jean-Loup Puget Brigitte Rocca-Volmerange 《Monthly notices of the Royal Astronomical Society》2000,316(4):768-778
558.
Abstract— Mössbauer spectra showed the CV3 oxidized subgroup meteorites Allende and Axtell to be similar in olivine content and in a surprising lack of pronounced magnetic components, but different in Fe3+ phases. One atypical Allende sample showed an 8% area under the curve for magnetite, which is still less than a reported value for a CV3 reduced subgroup member. Allende's unusual Fe3+ spectral region distinguishes it from most other stony meteorites and is difficult to fit to known mineral parameters. 相似文献
559.
560.
A Computer-Aided Learning (CAL) program has been developed as a support aid for students learning the principle of effective stress and its application. The program called ESP (Effective Stress Program) has evolved over a period of two years as a result of research into student learning. This paper discusses the development, use and evaluation of the latest version of the program ESP98. ESP98 is shown to be an effective support tool by outperforming the conventional methods of instruction. The key to the success of ESP98 is the high level of interaction which students experience. The nature of the interaction is centred on a mistake-induced dialogue where the student is provided with progressive and instant feedback and guided towards the final answer. ESP has been integrated into the curriculum at Heriot-Watt University for the past two years and is freely available for use by other teaching institutions by contacting the authors. 相似文献