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1.
We present numerical investigations into the formation of massive stars from turbulent cores of density structure  ρ∝ r −1.5  . The results of five hydrodynamical simulations are described, following the collapse of the core, fragmentation and the formation of small clusters of protostars. We generate two different initial turbulent velocity fields corresponding to power-law spectra   P ∝ k −4  and   P ∝ k −3.5  , and we apply two different initial core radii. Calculations are included for both completely isothermal collapse, and a non-isothermal equation of state above a critical density  (10−14 g cm−3)  . Our calculations reveal the preference of fragmentation over monolithic star formation in turbulent cores. Fragmentation was prevalent in all the isothermal cases. Although disc fragmentation was largely suppressed in the non-isothermal runs due to the small dynamic range between the initial density and the critical density, our results show that some fragmentation still persisted. This is inconsistent with previous suggestions that turbulent cores result in the formation of a single massive star. We conclude that turbulence cannot be measured as an isotropic pressure term.  相似文献   
2.
A coupled deterministic hydrological and water temperature model, CEQUEAU, was modified to include soil temperature and crown closure in its calculation of local advective terms in the heat budget. The modified model was than tested to verify its sensitivity to these modifications. An analysis of the heat budget of a small forested catchment in eastern Canada revealed that the advective term related to interflow plays a significant role in the daily water heat budget, providing on average 28% of the local advective budget (which also includes advective heat terms from surface runoff and groundwater) and nearly 14% of the total heat budget (which includes all radiative terms at the water surface, convection and evaporation, as well as the local advective terms). Relative sensitivity indices (RSIs) were used to verify the impact of the newly introduced parameters and variables. Among them, parameters related to the forest cover (crown closure and leaf area index) have a maximum RSI of ?0·6; i.e. a 100% increase in value produces a 60% decrease in the local advective term. Parameters with the greatest influence are the volume of water contributing to interflow and the amplitude of the net radiative flux at the soil surface, which, if doubled, would double the contribution of the local interflow advective term to the heat budget. Copyright © 2003 John Wiley & Sons, Ltd.  相似文献   
3.
The boundaries of the polar caps of Mars have been measured on more than 3000 photographs since 1905 from the plate collection at the Lowell Observatory. For the Earth, the polar caps have been accurately mapped only since the mid 1960's when satellites were first available to synoptically view the polar regions. The polar caps of both planets wax and wane in response to changes in the seasons, and interannual differences in polar cap behavior on Mars as well as Earth are intimately linked to global energy balance. Data on the year to year variations in the extent of the north polar caps of Mars and Earth have been assembled and compared, although only 6 years of concurrent data were available for comparison.  相似文献   
4.
Seventy-seven gem opals from ten countries were analyzed by inductively coupled plasma-mass spectrometry (ICP-MS) through a dilution process, in order to establish the nature of the impurities. The results are correlated to the mode of formation and physical properties and are instrumental in establishing the geographical origin of a gem opal. The geochemistry of an opal is shown to be dependant mostly on the host rock, at least for examples from Mexico and Brazil, even if modified by weathering processes. In order of decreasing concentration, the main impurities present are Al, Ca, Fe, K, Na, and Mg (more than 500 ppm). Other noticeable elements in lesser amounts are Ba, followed by Zr, Sr, Rb, U, and Pb. For the first time, geochemistry helps to discriminate some varieties of opals. The Ba content, as well as the chondrite-normalized REE pattern, are the keys to separating sedimentary opals (Ba > 110 ppm, Eu and Ce anomalies) from volcanic opals (Ba < 110 ppm, no Eu or Ce anomaly). The Ca content, and to a lesser extent that of Mg, Al, K and Nb, helps to distinguish gem opals from different volcanic environments. The limited range of concentrations for all elements in precious (play-of-color) compared to common opals, indicates that this variety must have very specific, or more restricted, conditions of formation. We tentatively interpreted the presence of impurities in terms of crystallochemistry, even if opal is a poorly crystallized or amorphous material. The main replacement is the substitution of Si4+ by Al3+ and Fe3+. The induced charge imbalance is compensated chiefly by Ca2+, Mg2+, Mn2+, Ba2+, K+, and Na+. In terms of origin of color, greater concentrations of iron induce darker colors (from yellow to “chocolate brown”). This element inhibits luminescence for concentrations above 1000 ppm, whereas already a low content in U (≤ 1 ppm) induces a green luminescence.  相似文献   
5.
Numerical modelling was done at the Cold Lake Air Weapons Range, Canada, to test whether the dissolved RDX and nitrate detected in groundwater come from the same sources, and to predict whether contamination poses a threat to the surface water receptors near the site. Military live fire training activities may indeed pose a risk of contamination to groundwater resources, however field investigations on military bases are quite recent, and little information is available on the long-term behaviour of munition residues related contaminants. Very limited information was available about the contaminant source zones, which were assigned based on our knowledge of current training activities. The RDX plume was well represented with the model, but the heterogeneous distribution of nitrate concentrations was more difficult to reproduce. It was nonetheless determined that both contaminants originate from the same areas. According to the model, both contaminants should reach the nearby river, but concentrations in the river should remain very low if the source zone concentration does not change. Finally, the model allowed the recommendation of a new location for the main bombing target, which would offer added protection to the river and the lake into which it flows.  相似文献   
6.
7.
Sommaire La région étudiée s'étend au large du massif des Maures, du massif de l'Estérel, des chaînes calcaires provençales et de la bordure alpine (Figure 1). Cette partie de la marge continentale médíterranéenne a été étudiée dans l'optique de la géodynamique en appliquant un ensemble de méthodes géophysiques, géologiques, sédimentologiques et géochimiques.La Méditerranée est l'objet de nombreuses études générales et son histoire tectonique est encore très discutée. Les relations entre la zone centrale (zone A) et les massifs terrestres géologiquement bien connus peuvent aider à la compréhension du cadre structural. L'étude très détaillée présentée ici concerne la marge continentale au large de la Côte d'Azur. Une étude bathymétrique préliminaire avec des profils espacés d'un mille marin a permis de définir un plateau continental peu étendu, une pente continentale abrupte (10–20°) avec des blocs continentaux effondrés. De nombreux canyons empruntent des accidents anciens qui ont rejoué.Des profils en série de sismique continue (Sparker et air gun) ont permis de délimiter la zone A qui comporte de nombreux dômes, de suivre des accidents majeurs, et de montrer des phénomènes sédimentaires et de néotectonique très importants (glissements, effondrements). Ces profils ont été calés avec 50 carottages. Un effondrement de plus de 1000 m depuis le Pliocène a été mis en évidence.La structure profonde a été abordée avec une étude de magnétométrie marine. La synthèse des résultats de sismique réfraction, de gravimétrie et de magnétométrie fait apparître un bombement du manteau sous la zone A avec abaissement rapide de la discontinuité de Moho sous la marge, la présence de volcans enfouis au Sud d'Antibes et de grands accidents de direction NS et EW.L'intérêt de ces résultats a semblé suffisamment important pour qu'un point de cette zone soit proposé pour le programme de forage JOIDES en Méditerranée.
This paper deals with the region off the Maures and Estérel Massifs, the Provence calcareous ranges and the Alpine border (Figure 1). This portion of the Mediterranean continental margin has been investigated with the classical methods used in the geosciences: geophysics, geology, sedimentology, geochemistry.Many general studies are dealing with the Mediterranean and its tectonical history is still controversial. The relationship between the central zone (zone A) and the geologically well-known land massifs could help in understanding the structural framework. The present detailed study concerns the continental margin off Côte d'Azur. A relatively narrow continental shelf, a steep continental slope (10–20°) with collapsed continental blocks are defined by preliminary bathymetric studies with a spacing of one nautical mile. Many submarine canyons follow former faults which have been rejuvenated.A series of seismic reflection profiles (sparker and air-gun) provide limits for zone A (with many domes), allow tracing major faults and display important sedimentary and neotectonic processes (sliding, foundering). These profiles have been scaled with 50 cores. Evidence is brought forward for a local subsidence of over 1000 m. The deep structure has been investigated with marine magnetic methods. The results from seismic refraction, gravity and magnetics show a swell of the mantle beneath zone A, with a steep dipping of the M discontinuity under the margin, buried volcanoes south of Antibes and great faults striking NS or EW.These results seem to be important enough to propose a place in this zone of the Mediterranean as a JOIDES drilling site.


Maintenant au Centre Océanologique de Bretagne, B.P. 337, 29 Brest, France.  相似文献   
8.
A population of the intertidal barnacle, Balanus balanoides (L.) maintained on a raft in the Menai Strait was sampled regularly over a two-year period and pooled fractions analysed for zinc and other trace metals. The seasonal variation of zinc in three fractions (body, other soft tissues and shell) has been followed and related to physiological condition. The body accumulates zinc almost continuously whilst this trace metal accumulates in the ovary only as it develops and is lost in the gametes when these are laid. The newly formed egg-masses therefore may be the more useful sample for indicating zinc pollution.  相似文献   
9.
Environmental tracers sampled from the carbonate Madison aquifer on the eastern flank of the Black Hills, South Dakota, USA indicated the approximate locations of four major karst conduits. Contamination issues are a major concern because these conduits are characterized by direct connections to sinking streams, high groundwater velocities, and proximity to public water supplies. Objectives of the study were to estimate approximate conduit locations and assess possible anthropogenic influences associated with conduits. Anomalies of young groundwater based on chlorofluorocarbons (CFCs), tritium, and electrical conductivity (EC) indicated fast moving, focused flow and thus the likely presence of conduits. δ18O was useful for determining sources of recharge for each conduit, and nitrate was a useful tracer for assessing flow paths for anthropogenic influences. Two of the four conduits terminate at or near a large spring complex. CFC apparent ages ranged from 15 years near conduits to >50 years in other areas. Nitrate-N concentrations >0.4 mg/L in groundwater were associated with each of the four conduits compared with concentrations ranging from <0.1 to 0.4 mg/L in other areas. These higher nitrate-N concentrations probably do not result from sinking streams but rather from other areas of infiltration.  相似文献   
10.
Theoretical Ca X electron temperature sensitive emission line ratios, derived using electron excitation rates interpolated from accurateR-matrix calculations, are presented forR 1 =I(419.74 )/I(574.02 ,),R 2 =I(411.65 )/I(574.02 ),R 3 =I(419.74 )/I(557.75 ), andR 4 =I(411.65 )/I(557.75 ). A comparison of these with observational data for three solar flares, obtained by the Naval Research Laboratory's S082A slitless spectrograph on boardSkylab, reveals good agreement between theory and observation forR 1 andR 3 in one event, which provides limited support for the accuracy of the atomic data adopted in the analysis. However, in the other flares the observed values ofR 1R 4 are much larger than the theoretical high-temperature limits, which is probably due to blending of the 419.74 line with Civ 419.71 , and 411.65 with possibly Ciii 411.70 .  相似文献   
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