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61.
J. Nicholas van Driel 《Environmental Geology》1980,3(3):151-157
A computer program for overlaying maps has been tested and evaluated as a means for producing geologic derivative maps. Four
maps of the Sugar House Quadrangle, Utah, were combined, using the Multi-Scale Data Analysis and Mapping Program, in a single
composite map that shows the relative stability of the land surface during earthquakes. Computer-composite mapping can provide
geologists with a powerful analytical tool and a flexible graphic display technique. Digitized map units can be shown singly,
grouped with different units from the same map, or combined with units from other source maps to produce composite maps. The
mapping program permits the user to assign various values to the map units and to specify symbology for the final map. Because
of its flexible storage, easy manipulation, and capabilities of graphic output, the composite-mapping technique can readily
be applied to mapping projects in sedimentary and crystalline terranes, as well as to maps showing mineral resource potential. 相似文献
62.
A model is developed for estimating location of a volcano relative to sample points in an associated ashfall, cloud height during eruption, and mean wind velocity during ash deposition. The ash deposit must cover a large area and have an elongate axis. The model appears to be applicable both to recent and to unobserved ashfalls in the past, provided adequate and representative ash samples are available. The opportunity to test the diagnostic model on volcanic ashfalls is limited by sparsity of the necessary input data. From more than 20 ashfalls described in the literature, the 1947 Hekla (Iceland) eruption is the only one which includes suitable particle size analyses taken from samples related to a well-defined axis. The application of the model to the Hekla ashfall is discussed. 相似文献
63.
Surendra K. Saxena Alan Benimoff Nicholas E. Pingitore Jr. 《Contributions to Mineralogy and Petrology》1977,60(1):77-90
The chemical composition of 2188 terrestrial igneous rocks ranging from ultrabasic to granitic composition was analyzed statistically using the method of factor analysis (principal components). The resultant first and second factors were: $$\begin{gathered} {\text{ }}F_1 = 0.933{\text{ Na}}_{\text{2}} {\text{O + 0}}{\text{.143 SiO}}_{\text{2}} + 0.206{\text{ K}}_{\text{2}} {\text{O}} - 0.346{\text{ CaO}} - 0.263{\text{ MgO}} - \hfill \\ .203{\text{ FeO}} \pm \cdot \cdot \cdot \hfill \\ {\text{ }}F_2 = 0.979{\text{ Al}}_{\text{2}} {\text{O}}_{\text{3}} - 0.269{\text{ MgO}} - 0.151{\text{ SiO}}_{\text{2}} - 0.112{\text{ FeO}} \pm \cdot \cdot \cdot \hfill \\ \end{gathered} $$ where oxides are in weight percent. A plot of the first factor against the second results in a useful igneous variation diagram. When the compositions of the 2188 terrestrial rocks and 604 lunar rocks are plotted on this diagram, the two groups of rocks are clearly separated within an albite-anorthite-forsterite-fayalite-quartz polygon. None of the terrestrial differentiation trends are significant for lunar rocks. The major difference in the chemistry of lunar and terrestrial rocks lies in the former being albite poor. Removal of most of the albite from the compositions of terrestrial layered intrusives such as the Skaergaard results in an excellent match between the compositions of the two groups of rocks. Albite subtracted compositions of Skaergaard rocks in particular cover the entire range of chemical variation in the lunar rocks. The statistical results prompt us to speculate further on the similarity of the moon and Skaergaard. We note that the average composition of the moon (Wanke et al., 1974) is similar to the albite subtracted composition of the Skaergaard magma. The lunar crust and a significant part of the lunar interior may match the albite subtracted and somewhat Mg enriched Skaergaard magma. 相似文献
64.
65.
Nicholas R. Golledge Derek Fabel Jeremy D. Everest Stewart Freeman Steven Binnie 《第四纪科学杂志》2007,22(8):785-791
We use cosmogenic 10Be surface exposure age techniques at a locality close to Rannoch Moor, western Scottish Highlands, in order to establish the age and chronology of its most recent glaciation. Glacial erratics and an in situ bedrock quartz vein sampled from this site—the summit of Beinn Inverveigh—have yielded zero‐erosion exposure ages of 12.9 ± 1.5 ka to 11.6 ± 1.0 ka, implying complete ice cover of the mountain during the Younger Dryas, or Loch Lomond Stadial. These results fit closely with published 14C dates that bracket the maximum (lateral) extent of ice cap outlet glaciers, and are the first internally consistent ages to specifically address this period of glaciation in Scotland. Furthermore, the dates imply that previous palaeoglaciological reconstructions for this area may have underestimated both the thickness of the former ice cap and, by implication, its volume. © British Geological Survey/Natural Environment Research Council copyright 2007. Reproduced with the permission of BGS/NERC. Published by John Wiley & Sons, Ltd. 相似文献
66.
Alaa I. Ibrahim Hisham Anwer Mohamed H. Soliman Nicholas Mackie-Jones Kalvir S. Dhuga William C. Parke Jean H. Swank Tilan Ukwatta M. T. Hussein T. El-Sherbini 《Astrophysics and Space Science》2007,308(1-4):535-539
A 6.4 keV emission line was discovered in an unusual burst from the soft gamma repeater SGR 1900+14 with the Rossi X-ray Timing
Explorer (RXTE). The line was detected in part of a complex multipeak precursor that preceded the unusual burst of 1998 August
29, i.e. two days after the giant flare of August 27 from the source. The origin of the line was not firmly identified and
two possible interpretations were equally plausible including (a) Kα fluorescence from a small iron rich material that was ejected to the magnetosphere during the August 27 flare, and (b) proton
or α-particle cyclotron resonance. If the iron scenario was correct, we expect to find evidence for the line during the intervening
interval between the flare and the August 29 burst, i.e. on August 28. Here we present the results of the August 28 burst
observation, taken with RXTE. We detect a total of seven bursts whose individual and joint spectra do not show evidence for
spectral lines. We also investigated a sample of nine bursts before and after the August 29 burst (from 1998 June to December)
that do not reveal evidence for a spectral line near 6.4 keV or elsewhere. These results disfavor the iron scenario and make
the proton/α-particle cyclotron resonance interpretation more plausible. The appearance of the emission line in part of a complex burst
and its absence from the studied sample indicate that the line is likely due to a transient phenomenon that may depend on
the burst morphology, energetics and the properties of the emission region.
相似文献
67.
Russell Cannon Michael Drinkwater Alastair Edge Daniel Eisenstein Robert Nichol Phillip Outram Kevin Pimbblet Roberto De Propris Isaac Roseboom David Wake Paul Allen Joss Bland-Hawthorn Terry Bridges Daniel Carson Kuenley Chiu Matthew Colless Warrick Couch Scott Croom Simon Driver Stephen Fine Paul Hewett Jon Loveday Nicholas Ross Elaine M. Sadler Tom Shanks Robert Sharp J. Allyn Smith Chris Stoughton Peter Weilbacher Robert J. Brunner Avery Meiksin Donald P. Schneider 《Monthly notices of the Royal Astronomical Society》2006,372(1):425-442
68.
Photoclinometry is the most common method used to obtain high-resolution topographic maps of planetary terrain. We derive the likelihood function of photoclinometric surface slope from (1) the probability distribution of the measured photon count of natural sunlight through a Charge-Coupled Device (CCD) including uncertainty due to camera shot noise, camera read noise, small-scale albedo fluctuation and atmospheric haze, and (2) a photometric model relating photocount to surface orientation. We then use classical estimation theory to determine the theoretically exact biases and errors inherent in photoclinometric surface slope and show when they may be approximated by asymptotic expressions for sufficiently high sample size. We show how small-scale albedo variability often dominates biases and errors, which may become an order of magnitude larger than surface slopes when surface reflectance has a weak dependence on surface tilt. We provide bounds on the minimum possible error of any unbiased photoclinometric surface slope estimate, and compute the sample sizes necessary to constrain errors within desired design thresholds. 相似文献
69.
Donna L. Whitney Nicholas C. A. Seaton 《Contributions to Mineralogy and Petrology》2010,160(4):591-607
Polycrystalline garnets are common in metamorphic rocks and may form as a result of close spacing of nuclei (if clustering
is early) or impingement of larger grains (if clustering occurs later in the growth history). The timing of clustering relative
to garnet growth is relevant to understanding the formation and evolution of porphyroblasts and evaluating the significance
(if any) of clustering. Electron backscattered diffraction (EBSD) analysis of garnet-bearing metamorphic rocks reveals the
presence of polycrystalline garnet in nine localities examined in this study: the northern Appalachians (Vermont, Maine, New
York, USA); North American Cordillera (North Cascades Range, Washington; Snake Range, Nevada, USA); western Rocky Mountains
(British Columbia, Canada); southern Menderes Massif (Turkey); Santander Massif (Colombia); and the Sanandaj–Sirjan zone (Hamadan,
Iran). In some samples, polycrystals comprise ~20–30% of garnets analyzed, and chemical and textural evidence suggests that
early coalescence of garnet polycrystals is common. Some early-coalescing polycrystals exhibit growth zoning that is concentric
about the geometric center of the polycrystal. In thin section, these garnets may be undetectable as polycrystals based on
morphology or zoning. In some polycrystals, zoning is unrelated to the location of internal grain boundaries; in others, Fe–Mn–Mg
zoning has a different pattern than that of Ca; zoning patterns may vary on the scale of a single thin section. In addition,
some polycrystals are characterized by high-angle misorientation boundaries that may be in special (non-random) orientations,
an observation that indicates that these polycrystals are not random clusters of grains. The presence of internal grain boundaries
may affect diffusion pathways and length scales, and may facilitate communication of porphyroblast interiors with matrix phases,
thereby influencing reaction history of the rock and the composition/zoning of garnet. 相似文献
70.
Paul Duuring Wouter Bleeker Steve W. Beresford Nicholas Hayward 《Mineralium Deposita》2010,45(3):281-311
Perseverance is a world-class, komatiite-hosted nickel sulphide deposit situated in the well-endowed Leinster nickel camp
of the Agnew–Wiluna greenstone belt, Western Australia. The mine stratigraphy at Perseverance trends north-northwest (NNW),
dips steeply to the west, and is overturned. Stratigraphic footwall units lie along the western margin of the Perseverance
Ultramafic Complex (PUC). The PUC comprises a basal nickel sulphide-bearing orthocumulate- to mesocumulate-textured komatiite
that is overlain by a thicker, nickel sulphide-poor, dunite lens. Hanging wall rocks include rhyodacite that is texturally
and compositionally similar to footwall volcanic rocks. These rocks separate the PUC from a second sequence of nickeliferous,
E-facing, spinifex-textured komatiite units (i.e. the East Perseverance komatiite). Past workers argue for a conformable stratigraphic
contact between the PUC and the East Perseverance komatiite and conclude that the PUC is extrusive. This study, however, clearly
demonstrates that these komatiite sequences are discordant, implying that the PUC may have intruded rhyodacite country rock
as a sill with subsequent structural juxtaposition against the East Perseverance komatiite. Early N–S shortening associated
with the regional DI deformation event (corresponding to the local DP1 to DP3 events at Perseverance) resulted in the heterogeneous partitioning of strain along the margins of the competent dunite. A
mylonite developed in the more ductile footwall rocks along the footwall margin of the PUC, while isoclinal F3 folds, such as the Hanging wall limb and Felsic Nose folds, formed in low-mean stress domains along the fringes of the elongated
dunite lens. Strata-bound massive and disseminated nickel sulphides were passively fold thickened in hinge areas of isoclinal
folds, whereas basal massive sulphides lubricated fold limbs and promoted thrust movement along shallowly dipping lithological
contacts. Massive sulphides were physically remobilised up to 20 m from their primary footwall position into deposit-scale
fold hinges to form the 1A and Felsic Nose orebodies. First-order controls on the geometry of the Perseverance deposit include
the thermomechanical erosion of footwall rocks and the channelling of the mineralised komatiitic magma. Second- or third-order
controls are several postvolcanic deformation events, which resulted in the progressive folding and shearing of the footwall
contact, as well as the passive fold thickening of massive and disseminated sulphide orebodies. Massive sulphides were physically
remobilised into multiple generations of fold hinges and shear zones. Important implications for near-mine exploration in
the Leinster camp include identifying nickeliferous komatiite units, defining their three-dimensional geometry, and targeting
fold hinge areas. Fold plunge directions and stretching lineations are indicators of potential plunge directions of massive
sulphide orebodies. 相似文献