A numerical simulation of the effects of changing vegetation type on surface hydroclimatology     

Piers J. Sellers  John G. Lockwood 《Climatic change》1981,3(2):121-136

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Seasonal changes in the depth distributions of interstitial salinities in the Fraser River estuary,British Columbia     

Peter M. Chapman 《Estuaries and Coasts》1981,4(3):226-228

The vertical distribution of interstitial salinities to a depth of 6 cm in subtidal estuarine sediments was measured monthly from June 1977 to August 1978 in mud substrates in the Fraser River estuary, British Columbia. Measurements were made at six stations ranging from oligohaline to polyhaline. The results of this study demonstrated that vertical salinity gradients were present, particularly in the mesohaline zone of the estuary, in the sediments and that the magnitude of these gradients changes seasonally.  相似文献   

Exploration geochemistry—Distribution of elements and recognition of anomalies     

G. J. S. Govett  W. D. Goodfellow  R. P. Chapman  C. Y. Chork 《Mathematical Geosciences》1975,7(5-6):415-446

The exploration geochemist faces a serious problem in reconciling theoretical statistics with the empirical distribution of elements in materials in the earth's crust. The results of computer-simulation experiments being conducted by the Exploration Geochemistry Group at the University of New Brunswick illustrate some of the problems of the relation between frequency distributions and spatial distributions of elements and raise some interesting questions about sampling patterns and physical size of samples. Most importantly, the simulation experiments and empirical examples support the contention that attempts to make an assumption of normality more efficient by performing log transformations on positively skewed data may defeat the purpose of statistical analysis for exploration work. New developments in computer-data presentation and interpretation, including population sorting and classification, illustrate the increasing use of the computer in exploration geochemistry.  相似文献   

Convective Heat Transfer in Selected Geologic Situations     

Kevin Kilty  David S. Chapman 《Ground water》1980,18(4):386-394

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The impact of precipitation on speed–flow relationships along a UK motorway corridor     

Elizabeth Hooper  Lee Chapman  Andrew Quinn 《Theoretical and Applied Climatology》2014,117(1-2):303-316

Although the fundamental traffic diagram provides the characteristics of a typical road traffic speed–flow relationship, little consideration has been given to the impact of adverse weather conditions on the relationship and the subsequent impact on local speed–flow. For the first time, this study uses precipitation radar along with a state-of-the art traffic information system to ascertain the relationship between speed–flow and precipitation on a UK transport corridor at the local (junction to junction) scale. It is evident that precipitation causes a significant reduction in speed and maximum flow on many links of the corridor as well as a downward reduction in the overall speed-flow relationship. With increased instances of heavy precipitation predicted in the UK as a result of climate change, these findings highlight the subsequent impact on journey travel times and associated economic costs.  相似文献   

Canada-France-Hawaii Telescope's “redeye” infrared camera system: Array performance     

Christopher Clark  Doug Simons  Steven Massey  Christopher Hunter  Scott Chapman 《Experimental Astronomy》1994,3(1-4):123-124

The Canada-France-Hawaii Telescope (CFHT) has recently commissioned two facility infrared cameras for astronomical observations in the 1.0 to 2.5 micron region. These cameras use NICMOS3 256×256 pixel arrays fabricated from Hg:Cd:Te. We report here on array performance and discuss two unique features of these arrays, namely corner glow and residual images. We have developed techniques for reducing corner glow and a method of clearing residual image charge. We discuss our techniques and their side effects.  相似文献   

Estimation of ocean-bottom properties by matched-field inversion ofacoustic field data     

Dosso  S.E. Yeremy  M.L. Ozard  J.M. Chapman  N.R. 《Oceanic Engineering, IEEE Journal of》1993,18(3):232-239

A method for estimating properties of the ocean bottom such as bathymetry and geoacoustic parameters such as sound speed, density and attenuation, using matched-field inversion is considered. The inversion can be formulated as an optimization problem by assuming a discrete model of unknown parameters and a bounded search space for each parameter. The optimization then involves finding the set of parameter values which minimizes the mismatch between the measured acoustic field and modeled replica fields. Since the number of possible models can be extremely large, the method of simulated annealing, which provides an efficient optimization that avoids becoming trapped in suboptimal solutions, has been used. The matching fields are computed using a normal mode model. In inversions for range-dependent parameters, the adiabatic approximation is employed. This allows mode values to be precomputed for a grid of parameter values and stored in look-up tables for fast reference, which greatly improves computational efficiency. Synthetic inversion examples are presented for realistic range-independent and range-dependent environments  相似文献   

The Growth of Facular Area Surrounding Large, Decaying Sunspots     

G. A. Chapman  A. S. Hoffer 《Solar physics》2006,237(2):321-328

In a previous paper, we investigated the facular area around 31 decaying sunspots of varied size. The growth of facular area as a function of spot decay was marginally significant (r ² = 0.1255, p = 0.05). Using new data, this paper examines the change in facular area surrounding large decaying sunspots some of which grew very rapidly. The data are from full-disk photometric images taken with CFDT2 (2.5″ pixels). For 10 sunspots, we find a statistically significant increase in facular area as a function of the spot decay rate with a regression coefficient, squared, of r ² = 0.611 (p < 0.02).  相似文献   

The Chinese comet observation in AD 773 January     

J. Chapman  M. Csikszentmihalyi  R. Neuhuser 《Astronomische Nachrichten》2014,335(9):964-967

The strong ¹⁴C increase in the year AD 774/5 detected in one German and two Japanese trees was recently suggested to have been caused by an impact of a comet onto Earth and a deposition of large amounts of ¹⁴C into the atmosphere (Liu et al. 2014). The authors supported their claim using a report of a historic Chinese observation of a comet ostensibly colliding with Earth's atmosphere in AD 773 January. We show here that the Chinese text presented by those authors is not an original historic text, but that it is comprised of several different sources. Moreover, the translation presented in Liu et al. is misleading and inaccurate. We give the exact Chinese wordings and our English translations. According to the original sources, the Chinese observed a comet in mid January 773, but they report neither a collision nor a large coma, just a long tail. Also, there is no report in any of the source texts about “dust rain in the daytime” as claimed by Liu et al. (2014), but simply a normal dust storm. Ho (1962) reports sightings of this comet in China on AD 773 Jan 15 and/or 17 and in Japan on AD 773 Jan 20 (Ho 1962). At the relevant historic time, the Chinese held that comets were produced within the Earth's atmosphere, so that it would have been impossible for them to report a “collision” of a comet with Earth's atmosphere. The translation and conclusions made by Liu et al. (2014) are not supported by the historical record. Therefore, postulating a sudden increase in ¹⁴C in corals off the Chinese coast precisely in mid January 773 (Liu et al. 2014) is not justified given just the ²³⁰Th dating for AD 783 ± 14. (© 2014 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

The effect of lensing on the identification of SCUBA galaxies     

S. C. Chapman  Ian Smail  R. J. Ivison  A. W. Blain 《Monthly notices of the Royal Astronomical Society》2002,335(1):L17-L21

Spectroscopic surveys of submillimetre(submm)-selected sources have uncovered optically bright galaxies at   z ≲ 1  close to the positions of several submm sources. Naive statistical analyses suggest that these galaxies are associated with the submm emission. However, in some cases, it is difficult to understand this association given the relatively modest redshifts and unprepossessing spectral characteristics of the galaxies. These are in stark contrast to those expected from the massive dust-enshrouded starbursts and AGN thought to power the bulk of the bright submm population. We present new observations of optically bright counterparts to two luminous submm sources, along with a compilation of previously proposed optically bright counterparts with   z ≲ 1  . We suggest that the majority of these associations between bright galaxies and submm sources may be as a result of the action of the foreground galaxies as gravitational lenses on the much fainter and more distant submm sources. We discuss the implications of this conclusion for our understanding of the SCUBA population.  相似文献