A density-dependent multi-species model to assess groundwater flow and nutrient transport in the coastal Keauhou aquifer,Hawai‘i,USA     

Okuhata  Brytne K.  El-Kadi  Aly I.  Dulai  Henrietta  Lee  Jonghyun  Wada  Christopher A.  Bremer  Leah L.  Burnett  Kimberly M.  Delevaux  Jade M. S.  Shuler  Christopher K. 《Hydrogeology Journal》2022,30(1):231-250

Hydrogeology Journal - Fresh groundwater is a critical resource supporting coastal ecosystems that rely on low-salinity, nutrient-rich groundwater discharge. This resource, however, is subject to...  相似文献   

Levels of heavy metals in some Red Sea fish before hot brine pools mining     

Rifaat G.M. Hanna   《Marine pollution bulletin》1989,20(12):631-635

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Challenges in global ballast water management   总被引：3，自引：0，他引：3  

Endresen Ø  Lee Behrens H  Brynestad S  Bjørn Andersen A  Skjong R 《Marine pollution bulletin》2004,48(7-8):615-623

Ballast water management is a complex issue raising the challenge of merging international regulations, ship's specific configurations along with ecological conservation. This complexity is illustrated in this paper by considering ballast water volume, discharge frequency, ship safety and operational issues aligned with regional characteristics to address ecological risk for selected routes. A re-estimation of ballast water volumes gives a global annual level of 3500 Mton. Global ballast water volume discharged into open sea originating from ballast water exchange operations is estimated to approximately 2800 Mton. Risk based decision support systems coupled to databases for different ports and invasive species characteristics and distributions can allow for differentiated treatment levels while maintaining low risk levels. On certain routes, the risk is estimated to be unacceptable and some kind of ballast water treatment or management should be applied.  相似文献   

Linking the Chassigny meteorite and the Martian surface rock Backstay: Insights into igneous crustal differentiation processes on Mars     

Hanna NEKVASIL  Francis M. McCUBBIN  Andrea HARRINGTON  Stephen ELARDO  Donald H. LINDSLEY 《Meteoritics & planetary science》2009,44(6):853-869

Abstract— In order to use igneous surface lithologies to constrain Martian mantle characteristics, secondary processes that lead to compositional modification of primary mantle melts must be considered. Crystal fractionation of a mantle‐derived magma at the base of the crust followed by separation and ascent of residual liquids to the surface is common in continental hotspot regions on Earth. The possibility that this process also takes place on Mars was investigated by experimentally determining whether a surface rock, specifically the hawaiite Backstay analyzed by the MER Spirit could produce a known cumulate lithology with a deep origin (namely the assemblages of the Chassigny meteorite) if trapped at the base of the Martian crust. Both the major cumulus and melt inclusion mineral assemblages of the Chassigny meteorite were produced experimentally by a liquid of Backstay composition within the pressure range 9.3 to 6.8 kbar with bulk water contents between 1.5 and 2.6 wt%. Experiments at 4.3 and 2.8 kbar did not produce the requisite assemblages. This agreement suggests that just as on Earth, Martian mantle‐derived melts may rise to the surface or remain trapped at the base of the crust, fractionate, and lose their residual liquids. Efficient removal of these residual liquids at depth would yield a deep low‐silica cumulate layer for higher magmatic water content; at lower magmatic water content this cumulate layer would be basaltic with shergottitic affinity.  相似文献   

A limit on the number density of bright z≈ 7 galaxies     

Elizabeth R. Stanway  Malcolm N. Bremer  Valentina Squitieri  Laura S. Douglas  Matthew D. Lehnert 《Monthly notices of the Royal Astronomical Society》2008,386(1):370-376

We present a survey of bright optical dropout sources in two deep, multiwavelength surveys comprising 11 widely separated fields, aimed at constraining the galaxy luminosity function at   z ≈ 7  for sources at  5–10  L * ( z = 6)  . Our combined survey area is 225 arcmin² to a depth of   J _AB= 24.2  (3σ) and 135 arcmin² to   J = 25.3  (4σ). We find that infrared data longwards of 2 μm are essential for classifying optical dropout sources, and in particular for identifying cool Galactic star contaminants. Our limits on the number density of high-redshift sources are consistent with current estimates of the Lyman break galaxy luminosity function at   z = 6  .  相似文献   

William Smith's map brought alive by digital remastering     

Alan R. Butcher  Duncan Pirrie  Gavyn K. Rollinson  Hanna Horsch  Stephen P. Hesselbo  Michael Owen  David Haberlah 《Geology Today》2020,36(5):175-182

The geological mapping carried out by William Smith, which resulted in the publication of his famous map in 1815, was remarkable in many respects, not least because it relied on him being able to make consistent and accurate observations on the rock types he encountered during his fieldwork. This ability, gained from his many years studying rocks, allowed him to observe features with his own eyes (or at the very least, with the aid of a simple magnifying device) that others could not. We take a new look at William Smith's original stratigraphical sequences, and with samples collected from his classic field areas (many of which are around the city of Bath, Somerset, UK), demonstrate how spatial mineralogy mapping can be incorporated into the modern age of digital mapping.  相似文献   

Insurgent participation: consensus and contestation in planning the redevelopment of Berlin-Tempelhof airport     

Hanna Hilbrandt 《Urban geography》2017,38(4):537-556

Despite decades of debate, participatory planning continues to be contested. More recently, research has revealed a relationship between participation and neoliberalism, in which participation works as a post-political tool—a means to depoliticize planning and legitimize neoliberal policy-making. This article argues that such accounts lack attention to the opportunities for opposing neoliberal planning that may be inherent within participatory processes. In order to further an understanding of the workings of resistance within planning, it suggests the notion of insurgent participation—a mode of contentious intervention in participatory approaches. It develops this concept through the analysis of various participatory approaches launched to regenerate the former airport Berlin-Tempelhof. A critical reading of participation in Tempelhof reveals a contradictory process. Although participatory methods worked to mobilize support for predefined agendas, their insurgent participation also allowed participants to criticize and shape the possibilities of engagement, challenge planning approaches and envision alternatives to capitalist imperatives.  相似文献   

Do CRISTA Experiment/Campaign Data Represent a Typical Situation or Not?     

Laštovička  Jan  Burešová  Dalia  Boška  Josef  Bremer  Jurgen  Märcz  Ferenc 《Studia Geophysica et Geodaetica》1997,41(2):171-180

Data from four A3 radio wave circuits in central Europe are used to analyse the representativeness of the ionization and gravity wave activity pattern in the lower ionosphere (85 – 100 km) in the CRISTA experiment interval (3 – 12 November 1994) for the given conditions. It has been found that the CRISTA experiment interval was run under conditions, which are highly representative both of October – November 1994 and autumn, low-moderate solar activity, the descending phase of solar cycle conditions, i.e. CRISTA measurements may be considered to provide values identical with, or close to climatological values (at least for central Europe, h = 85 – 100 km).  相似文献   

Reducing global GHG emissions by replicating successful sector examples: the ‘good practice policies’ scenario     

Mark Roelfsema  Hanna Fekete  Niklas Höhne  Michel den Elzen  Nicklas Forsell  Takeshi Kuramochi 《Climate Policy》2018,18(9):1103-1113

This article shows the potential impact on global GHG emissions in 2030, if all countries were to implement sectoral climate policies similar to successful examples already implemented elsewhere. This assessment was represented in the IMAGE and GLOBIOM/G4M models by replicating the impact of successful national policies at the sector level in all world regions. The first step was to select successful policies in nine policy areas. In the second step, the impact on the energy and land-use systems or GHG emissions was identified and translated into model parameters, assuming that it would be possible to translate the impacts of the policies to other countries. As a result, projected annual GHG emission levels would be about 50 GtCO₂e by 2030 (2% above 2010 levels), compared to the 60 GtCO₂e in the ‘current policies’ scenario. Most reductions are achieved in the electricity sector through expanding renewable energy, followed by the reduction of fluorinated gases, reducing venting and flaring in oil and gas production, and improving industry efficiency. Materializing the calculated mitigation potential might not be as straightforward given different country priorities, policy preferences and circumstances.

Key policy insights

• Considerable emissions reductions globally would be possible, if a selection of successful policies were replicated and implemented in all countries worldwide.

• This would significantly reduce, but not close, the emissions gap with a 2°C pathway.

• From the selection of successful policies evaluated in this study, those implemented in the sector ‘electricity supply’ have the highest impact on global emissions compared to the ‘current policies’ scenario.

• Replicating the impact of these policies worldwide could lead to emission and energy trends in the renewable electricity, passenger transport, industry (including fluorinated gases) and buildings sector, that are close to those in a 2°C scenario.

• Using successful policies and translating these to policy impact per sector is a more reality-based alternative to most mitigation pathways, which need to make theoretical assumptions on policy cost-effectiveness.

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Detection of X-ray emission from the host clusters of 3CR quasars     

C. S. Crawford  I. Lehmann  A. C. Fabian  M. N. Bremer  G. Hasinger 《Monthly notices of the Royal Astronomical Society》1999,308(4):1159-1172

We report the detection of extended X-ray emission around several powerful 3CR quasars with redshifts out to 0.73. The ROSAT HRI images of the quasars have been corrected for spacecraft wobble and compared with an empirical point-spread function. All the quasars examined show excess emission at radii of 15 arcsec and more, the evidence being strong for the more distant objects and weak only for the two nearest ones, which are known from other wavelengths not to lie in strongly clustered environments. The spatial profile of the extended component is consistent with thermal emission from the intracluster medium of moderately rich host clusters to the quasars. The total luminosities of the clusters are in the range ∼4×10⁴⁴–3×10⁴⁵ erg s⁻¹, assuming a temperature of 4 keV. The inner regions of the intracluster medium are, in all cases, dense enough to be part of a cooling flow.  相似文献