中尺度流域土地利用/土地覆盖变化评估--以伊洛河中部地区为例   总被引：18，自引：7，他引：18  

李小建  刘钢军  钱乐祥  Jim Peterson 《地理科学》2001,21(4):289-296

将规范分析与实证分析相结合，提出了一个评估区域各点位土地利用／土地覆盖变化的新方法：（1）采用相对原则观察一时段内的变化方向；（2）物理模型与统计模型相结合，基于区域实际情况建立生境适宜性参照基准；（3）用多变量分析方法量度各点位与参照基准的差异。结合GIS和遥感技术，这种方法被应用于伊洛河中部地区的研究中。  相似文献   

The long-term salinity field in San Francisco Bay     

R.J. Uncles  D.H. Peterson 《Continental Shelf Research》1996,16(15):2005-2039

Data are presented on long-term salinity behaviour in San Francisco Bay, California. A two-level, width averaged model of the tidally averaged salinity and circulation has been written in order to interpret the long-term (days to decades) salinity variability. The model has been used to simulate daily averaged salinity in the upper and lower levels of a 51 segment discretization of the Bay over the 22-yr period 1967–1988. Monthly averaged surface salinity from observations and monthly-averaged simulated salinity are in reasonable agreement. Good agreement is obtained from comparison with daily averaged salinity measured in the upper reaches of North Bay.The salinity variability is driven primarily by freshwater inflow with relatively minor oceanic influence. All stations exhibit a marked seasonal cycle in accordance with the Mediterranean climate, as well as a rich spectrum of variability due to extreme inflow events and extended periods of drought. Monthly averaged salinity intrusion positions have a pronounced seasonal variability and show an approximately linear response to the logarithm of monthly averaged Delta inflow. Although few observed data are available for studies of long-term salinity stratification, modelled stratification is found to be strongly dependent on freshwater inflow; the nature of that dependence varies throughout the Bay. Near the Golden Gate, stratification tends to increase up to very high inflows. In the central reaches of North Bay, modelled stratification maximizes as a function of inflow and further inflow reduces stratification. Near the head of North Bay, lowest summer inflows are associated with the greatest modelled stratification. Observations from the central reaches of North Bay show marked spring-neap variations in stratification and gravitational circulation, both being stronger at neap tides. This spring-neap variation is simulated by the model. A feature of the modelled stratification is a hysteresis in which, for a given spring-neap tidal range and fairly steady inflows, the stratification is higher progressing from neaps to springs than from springs to neaps.The simulated responses of the Bay to perturbations in coastal sea salinity and Delta inflow have been used to further delineate the time-scales of salinity variability. Simulations have been performed about low inflow, steady-state conditions for both salinity and Delta inflow perturbations. For salinity perturbations a small, sinusoidal salinity signal with a period of 1 yr has been applied at the coastal boundary as well as a pulse of salinity with a duration of one day. For Delta inflow perturbations a small, sinusoidally varying inflow signal with a period of 1 yr has been superimposed on an otherwise constant Delta inflow, as well as a pulse of inflow with a duration of one day. Perturbations in coastal salinity dissipate as they move through the Bay. Seasonal perturbations require about 40–45 days to propagate from the coastal ocean to the Delta and to the head of South Bay. The response times of the model to perturbations in freshwater inflow are faster than this in North Bay and comparable in South Bay. In North Bay, time-scales are consistent with advection due to lower level, up-estuary transport of coastal salinity perturbations; for inflow perturbations, faster response times arise from both upper level, down-estuary advection and much faster, down-estuary migration of isohalines in response to inflow volume continuity. In South Bay, the dominant time-scales are governed by tidal dispersion.  相似文献   

Inclined pipe vesicles as indicators of flow direction in basalts: A critical appraisal     

G. L. Peterson  J. W. Hawkins Jr 《Bulletin of Volcanology》1971,35(2):369-382

Inclined pipe vesicles and stretched vesicles near the base of basalt flows have long been regarded as reliable flow-direction indicators. However, attempts to use such structures in the Santa Rosa Basalt of Southern California to determine regional flow patterns, paleoslope, and source of eruption yielded inconclusive and contradictory results. Orientations of 1070 vesicles at 37 localities were obtained directions of inclination from vertical were plotted on circular histograms. At any specific locality vesicle orientations typically are normally distributed through a 40–60 degree sector. Commonly a pronounced maximum lies within a 20–40 degree sector. Even at localities having bimodal or trimodal distribution patterns, most vesicles plot within a 90 degree sector. The frequency distribution of oriented vesicles at individual localities strongly suggests a limited direction of flow and implies a source in the opposite direction. Comparison of such «flow directions» from locality to locality within the same flow, however, yielded highly divergent results over short distances. Likewise, comparison of directions from different flows yielded results ranging from parallel to diametrically opposed. Composite circular histograms from three small mesas censisting of thin, flat-lying flows showed little apparent preferred direction of vesicle inclination. Possible reasons for the highly divergent readings include sub-flow surface irregularities, turbulent rather than laminar flow, and/or convection in the lava during cooling. Although inclined vesicles may well indicate motion in a flow, their use for determination of flow directions and for regional paleogeographic interpretations is questionable.  相似文献   

Spectral development of a solar X-ray burst observed on OSO-7     

D. L. McKenzie  D. W. Datlowe  L. E. Peterson 《Solar physics》1973,28(1):175-185

The UCSD solar X-ray instrument on the OSO-7 satellite observes X-ray bursts in the 2–300 keV range with 10.24 s time resolution. Spectra obtained from the proportional counter and scintillation counter are analyzed for the event of November 16, 1971, at 0519 UT in terms of thermal (exponential spectrum) and non-thermal (power law) components. The energy content of the approximately 20 × 10⁶K thermal plasma increased with the 60 s duration hard X-ray burst which entirely preceded the 5 keV soft X-ray maximum. If the hard X-rays arise by thick target bremsstrahlung, the nonthermal electrons above 10 keV have sufficient energy to heat the thermally emitting plasma. In the thin target case the collisional energy transfer from non-thermal electrons suffices if the power law electron spectrum is extrapolated below 10 keV, or if the ambient plasma density exceeds 4 × 10¹⁰ cm^–3.Formerly at UCSD.  相似文献   

A critique of the internal tracer method for estimating contaminant degradation rates     

Martian P  Sorenson KS  Peterson LN 《Ground water》2003,41(5):632-639

The internal tracer method for estimating contaminant degradation rates separates the attenuation effects not associated with degradation by using a codisposed recalcitrant internal tracer to normalize the degrading contaminant concentration. The remaining attenuation between the internal tracer and degrading contaminant is attributed to degradation and the degradation rate half-life is estimated from the first-order decay equation. An analytical solution of the advection- dispersion equation was used to evaluate flow-and-transport conditions that could result in incorrect estimates of contaminant degradation rate constants. Flow-and-transport characteristics that result in overestimating degradation rates were of particular interest because the internal tracer method often used to demonstrate natural attenuation can achieve remedial objectives. The analytical solution was also used to estimate the magnitude of error associated with using the internal tracer method at an example site and to explain different degradation rates estimated using tracers with different decay rate constants.  相似文献   

First Results from Viper: Detection of Small-scale Anisotropy at 40 GHz     

Peterson JB  Griffin GS  Newcomb MG  Alvarez DL  Cantalupo CM  Morgan D  Miller KW  Ganga K  Pernic D  Thoma M 《The Astrophysical journal》2000,535(2):L83-L86

Using all available major samples of Seyfert galaxies and their corresponding closely matched control samples of nonactive galaxies, we find that the bar ellipticities (or axial ratios) in Seyfert galaxies are systematically different from those in nonactive galaxies. Overall, there is a deficiency of bars with large ellipticities (i.e., "thin" or "strong" bars) in Seyfert galaxies compared to nonactive galaxies. Accompanied with a large dispersion due to small number statistics, this effect is strictly speaking at the 2 sigma level. To obtain this result, the active galaxy samples of near-infrared surface photometry were matched to those of normal galaxies in type, host galaxy ellipticity, absolute magnitude, and, to some extent, redshift. We discuss possible theoretical explanations of this phenomenon within the framework of galactic evolution, and, in particular, of radial gas redistribution in barred galaxies. Our conclusions provide further evidence that Seyfert hosts differ systematically from their nonactive counterparts on scales of a few kiloparsecs.  相似文献   

Geothermal investigations in the Bohus granite area in southwestern Sweden     

Ove Landstrm  Sven ke Larson  Gustaf Lind  David Malmqvist 《Tectonophysics》1980,64(1-2)

Heat generation and heat flow were determined for the Bohus granite massif in western Sweden. This is the start of a major program concerning geothermal energy in Sweden. Neutron activation analyses, temperature measurements, thermal conductivity measurements have been carried out. As was expected the result, 76 mW m⁻², shows that even old Precambrian shields locally exhibit much higher values than normal.  相似文献   

Risø 1978: Further investigations into the effects of local terrain irregularities on tower-measured wind profiles     

Ernest W. Peterson  Peter A. Taylor  Jørgen Højstrup  Niels Otto Jensen  Leif Kristensen  Erik L. Petersen 《Boundary-Layer Meteorology》1980,19(3):303-313

Observations of flow over complex terrain taken at Risø during June–July 1978 and numerical studies confirm earlier findings that small variations in surface elevation have significant effects on mean wind profiles. Measured shear stresses in the nonequilibrium region of the flow are consistent with theory but quite different from those obtained assuming simple flux-profile relationships. These findings imply that flux-profile relationships can be quite complicated over other than simple homogeneous terrain.  相似文献   

A deep-sea in-situ suspended sediment sampling system: Comment     

R.E. Peterson 《Marine Geology》1976,21(1):59-62

A recent article by Beer et al. (1974) in Marine Geology describes an in-situ suspended sediment sampling system which utilizes a pump/motor unit, filter holders, and a lead-acid battery power source. Two aspects of their article may be misleading: the use of certain filter material as X-ray diffraction mounts, and the technique by which an oil-filled battery case may be operated.  相似文献   

Searching for hidden Wolf–Rayet stars in the Galactic plane – 15 new Wolf–Rayet stars     

L. J. Hadfield  S. D. Van Dyk  P. W. Morris  J. D. Smith  A. P. Marston  D. E. Peterson 《Monthly notices of the Royal Astronomical Society》2007,376(1):248-262

We report the discovery of 15 previously unknown Wolf–Rayet (WR) stars found as part of an infrared (IR) broad-band study of candidate WR stars in the Galaxy. We have derived an empirically based selection algorithm which has selected ∼5000 WR candidate stars located within the Galactic plane drawn from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (mid-IR) and Two-Micron All-Sky Survey (near-IR) catalogues. Spectroscopic follow-up of 184 of these reveals 11 nitrogen-rich (WN) and four carbon-rich (WC) WR stars. Early WC subtypes are absent from our sample and none shows evidence for circumstellar dust emission. Of the candidates which are not WR stars, ∼120 displayed hydrogen emission-line features in their spectra. Spectral features suggest that the majority of these are in fact B supergiants/hypergiants, ∼40 of these are identified Be/B[e] candidates.
Here, we present the optical spectra for six of the newly detected WR stars, and the near-IR spectra for the remaining nine of our sample. With a WR yield rate of ∼7 per cent and a massive star detection rate of ∼65 per cent, initial results suggest that this method is one of the most successful means for locating evolved, massive stars in the Galaxy.  相似文献