The composition of spherules and other features on shatter cone surfaces from the Vredefort structure,South Africa     

N.C. Gay  N.R. Comins  C. Simpson 《Earth and Planetary Science Letters》1978,41(3):372-380

Minute spherules and other glassy objects have been found on the surfaces of shatter cones in the sedimentary rocks forming the collar around the Vredefort ring structure. The composition of twenty-five of these spherules was determined using an energy-dispersive X-ray analysis system attached to a scanning electron microscope. These results show that spherules can be classified into a Si-, Al-rich variety, an Fe-rich variety and an intermediate variety.At first, the origin of the spherules appeared enigmatic: we considered that they could have been of organic origin; that they may represent dust or fly ash particles due to atmospheric pollution; or that they may result from processes operating during shatter cone formation. For analytical and logical reasons, we argue that the first two possible modes of origin can be discounted. Instead, it is suggested that the spherules result from melts generated by friction on the host rock surfaces during the formation of shatter cones. The variations in composition of the individual spherules may indicate selective melting of different parts of the rock surface or that the melts may have been affected by liquid immiscibility processes. This argument is reinforced by the striking analogy between the particles discussed here and those found in lunar samples.  相似文献   

Parameterization of Entrainment in a Sheared Convective Boundary Layer Using a First-order Jump Model   总被引：1，自引：0，他引：1  

Si-Wan Kim  Soon-Ung Park  David Pino  Jordi Vilà-Guerau de Arellano 《Boundary-Layer Meteorology》2006,120(3):455-475

Basic entrainment equations applicable to the sheared convective boundary layer (CBL) are derived by assuming an inversion layer with a finite depth, i.e., the first-order jump model. Large-eddy simulation data are used to determine the constants involved in the parameterizations of the entrainment equations. Based on the integrated turbulent kinetic energy budget from surface to the top of the CBL, the resulting entrainment heat flux normalized by surface heat flux is a function of the inversion layer depth, the velocity jumps across the inversion layer, the friction velocity, and the convection velocity. The developed first-order jump model is tested against large-eddy simulation data of two independent cases with different inversion strengths. In both cases, the model reproduces quite reasonably the evolution of the CBL height, virtual potential temperature, and velocity components in the mixed layer and in the inversion layer.The part of this work was done when the first author visited at NCAR.  相似文献   

Performance comparison of semicodeless GPS receivers for LEO satellites   总被引：1，自引：0，他引：1  

Oliver Montenbruck  Miquel Garcia-Fernandez  Jacob Williams 《GPS Solutions》2006,10(4):249-261

This report provides a detailed performance analysis of three semicodeless dual-frequency GPS receivers for use in low Earth orbit (LEO). The test set comprises the IGOR receiver, which represents a follow-on of the flight-proven BlackJack receiver, as well as two geodetic receivers (NovAtel OEM4-G2 and Septentrio PolaRx2), which are entirely based on commercial-off-the-shelf technology (COTS). All three receivers are considered for upcoming flight projects or experiments and have undergone at least a preliminary environmental qualification program. Using extensive signal simulator tests, the cold start signal acquisition, tracking sensitivity, differential code biases, raw measurement accuracy, and navigation accuracy of each receiver have been assessed. All tests are based on a common scenario that is representative of an actual space mission and provides a realistic simulation of the signal dynamics and quality on a scientific LEO satellite. Compared to the other receivers, the IGOR instrument exhibits a superior tracking sensitivity and is thus best suited for occultation measurements with low tangent point altitudes. The OEM4-G2 and PolaRx2 receivers are likewise shown to properly track dual-frequency GPS signals and normal signal levels and to provide accurate code and carrier phase measurements. Given their limited resource requirements, these receivers appear well suited for precise orbit determination applications and ionospheric sounding onboard of microsatellites with tight mission budgets.  相似文献   

Evaluation of Transient Electromagnetic Soundings for Deep Detection of Conductive Fluids   总被引：1，自引：0，他引：1  

Mark Stewart  Michael C. Gay 《Ground water》1986,24(3):351-356

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Water-body reflectance: Dependence on optical depth     

Lemus  L.  Gay  C. 《Theoretical and Applied Climatology》1984,35(1-2):137-145

Theoretical and Applied Climatology - The two-stream approximation of the radiative transfer equation is used to compute the water-body reflectance as a function of optical depth. From this...  相似文献   

Saharan Dust Transport and High-Latitude Glacial Climatic Variability: The Alboran Sea Record   总被引：1，自引：0，他引：1  

Ana Moreno  Isabel Cacho  Miquel Canals  Maarten A. Prins  María-Fernanda Snchez-Goi  Joan O. Grimalt  Gert Jan Weltje 《Quaternary Research》2002,58(3):318

Millennial to submillennial marine oscillations that are linked with the North Atlantic's Heinrich events and Dansgaard–Oeschger cycles have been reported recently from the Alboran Sea, revealing a close ocean-atmosphere coupling in the Mediterranean region. We present a high-resolution record of lithogenic fraction variability along IMAGES Core MD 95-2043 from the Alboran Sea that we use to infer fluctuations of fluvial and eolian inputs to the core site during periods of rapid climate change, between 28,000 and 48,000 cal yr B.P. Comparison with geochemical and pollen records from the same core enables end-member compositions to be determined and to document fluctuations of fluvial and eolian inputs on millennial and faster timescales. Our data document increases in northward Saharan dust transports during periods of strengthened atmospheric circulation in high northern latitudes. From this we derive two atmospheric scenarios which are linked with the intensity of meridional atmospheric pressure gradients in the North Atlantic region.  相似文献   

Particle fluxes dynamics in Blanes submarine canyon (Northwestern Mediterranean)     

Diana Zúñiga  M. Mar Flexas  Anna Sanchez-Vidal  Johan Coenjaerts  Antoni Calafat  Gabriel Jordà  Jordi García-Orellana  Joan Puigdefàbregas  Miquel Canals  Manuel Espino  Francesc Sardà  Joan B. Company 《Progress in Oceanography》2009,82(4):239-251

Within the framework of the multidisciplinary RECS project and with the aim of describing the particle flux transfer from the continental shelf to the deep basin, an array of five mooring lines equipped with a total of five pairs of PPS3/3 sequential-sampling sediment traps and RCM-7/8 current meters were deployed 30 m above the bottom from March 2003 to March 2004 inside and outside the Blanes Canyon. One mooring line was located in the upper canyon at 600 m depth, one in the canyon axis at 1700 m depth and other two close to the canyon walls at 900 m depth. A fifth mooring line was deployed in the continental open slope at 1500 m water depth.The highest near-bottom downward particle flux (14.50 g m⁻² d⁻¹) was recorded at the trap located in the upper canyon (M1), where continental inputs associated with the presence of the Tordera River are most relevant. On the other hand, the downward fluxes (4.35 g m⁻² d⁻¹) in the canyon axis (M2) were of the same order as those found in the western flank (M3) of the canyon. Both values were clearly higher than the value (1.95 g m⁻² d⁻¹) recorded at the eastern canyon wall (M4). The open slope (M5) mass flux (5.42 mg m⁻² d⁻¹) recorded by the sediment trap located outside the canyon system was three orders of magnitude lower than the other values registered by the inner canyon stations. The relevance of our data is that it explains how the transport pathway in the canyon occurs through its western flank, where a more active and persistent current toward the open ocean was recorded over the entire year of the experiment.Off-shelf sediment transport along the canyon axis showed clear differences during the period of the study, with some important events leading to strong intensifications of the current coupled with large transport of particle fluxes to the deepest parts of the canyon. Such events are primarily related to increases in river discharge and the occurrence of strong storms and cascading events during the winter.In summary, in this study it is shown that the dynamics of the water masses and the currents in the study area convert the sharp western flank of the Blanes Canyon in a more active region that favors erosion processes than the eastern flank, which has a smoother topography and where the absence of erosional conditions yields to steadier sedimentary processes.  相似文献   

Testing the predictive power of seagrass depth limit models     

Carlos M. Duarte  Núria Marbà  Dorte Krause-Jensen  María Sánchez-Camacho 《Estuaries and Coasts》2007,30(4):652-656

The power of equations predicting seagrass depth limit (Z_c) from light extinction (K _z) was tested on data on seagrass depth limits collected from the literature. The test data set comprised 424 reports of seagrass colonization depth and water transparency, including data for 10 seagrass species. This data set confirmed the strong negative relationship betweenZ _c andK _z. The regression equation in Duarte (1991) overestimated the realized seagrass colonization depths at colonization depths < 5 m, while there was no prediction bias above this threshold. These results indicated that seagrass colonizing turbid waters (K _z 0.27 m^-1) have higher apparent light requirements than those growing in clearer waters. The relationship between seagrass colonization depth and light attenuation shifts at a threshold of light attenuation of 0.27 m^-1, requiring separate equations to predictZ _c for seagrass growing in more turbid waters and clearer waters, and to set targets for seagrass restoration and conservation efforts.  相似文献   

Seismic anomalies in the aftershock sequence of November 16, 2000, in Papua New Guinea     

D. Caccamo  F. Parrillo  S. D’Amico  F. M. Barbieri  C. Laganà 《Izvestiya Physics of the Solid Earth》2007,43(8):662-668

The study of seismic anomalies, related both to the temporal trend of aftershock sequences and to the temporal series of mainshocks, is important for an understanding of the physical processes relating to the existence and the characteristics of seismic precursors. The purpose of this work is to highlight some methodological aspects related to the observation of possible anomalies in the temporal decay of an aftershock sequence. It is realized by means of several parameters. We focused our work on an analysis of the Papua New Guinea seismic sequence that occurred on November 16, 2000. The magnitude of the mainshock is M = 8.2. The observed temporal series of shocks per day can be considered as a sum of a deterministic contribution and a stochastic contribution. If the decay can be modeled as a nonstationary Poisson process where the intensity function is equal to n(t) = K(t + c)^−p + K ₁, the number of aftershocks in a small time interval Δt is the mean value n(t)Δt, with a standard deviation σ = √n(t)Δt. We observe that there are some variations in seismicity that can be considered as seismic anomalies before the occurrence of a large aftershock. The data, checked according to completeness criteria, come from the website of the USGS NEIC data bank (). The text was submitted by the authors in English.  相似文献   

Photometric lightcurves and pole determination of 433 Eros     

F. Scaltriti  V. Zappalà 《Icarus》1976,28(1):29-35

Fourteen photometric lightcurves of 433 Eros were made at the Astronomical Observatory of Torino during the 1974–75 close passage. The absolute magnitude of the primary maximum (10^m78), the phase coefficient (0.023 mag/degree), the synodic and sidereal period of rotation (0^d.21956 and 0^d.21959, respectively) and the ecliptic coordinates of the pole (λ = 17°, β = 10°) were deduced.  相似文献