Suitability of Hydrologic Evaluation of Landfill Performance (HELP) model of the US Environmental Protection Agency for the simulation of the water balance of landfill cover systems

 Cover systems are widely used to safeguard landfills and contaminated sites. The evaluation of the water balance is crucial for the design of landfill covers. The Hydrologic Evaluation of Landfill Performance (HELP) model of the US Environmental Protection Agency was developed for this purpose. This paper discusses some limitations of version 2 of this model and some operational difficulties for the use of this model in Germany, which has been developed for the United States. The model results are tested against field data of the water balance, measured on test fields on the Georgswerder landfill in Hamburg. Theoretically, HELP considers gravitational forces as driving forces of water flow only. Therefore capillary barriers cannot be simulated. Furthermore, the formation of and the flow through macropores are not considered, a main critical process that the diminishes the effectiveness of compacted soil liners. In the output comparison, the matching of measured and simulated data is quite good for lateral drainage, but failed for surface runoff and liner leakage through compacted soil liners. A further validation study is planned for HELP version 3 using a broader range of test field data. Received: 10 January 1995 · Accepted: 14 November 1995     

用数值模拟方法研究第四纪古气候──以LLN二维模式为例

本文着重介绍LLN模式对中晚第四纪大陆冰量变迁的模拟研究。由于天文学研究已经推算出大气层顶部太阳辐射过去和将来的长期变化，因而对本文的LLN二维模式而言，能否有效地进行古气候模拟在很大程度上取决于对古CO₂浓度的重建。随着对第四纪CO₂历史研究的不断深入，LLN模式对古气候长期变迁的模拟已从最初的末次冰期－间冰期延伸到0.6Ma B.P..。模拟的大陆冰量变化与地质记录对比良好，二者在与地球轨道要素有关的天文频率上的波动具有很高的相关性。     

LONG-TERM VARIATIONS IN INSOLATION AND THEIR EFFECTS ON CLIMATE, THE LLN EXPERIMENTS

Used to test the Milankovitch theory over the last glacial-interglacial cycles, the Louvain-la-Neuve two-dimension Northern Hemisphere climate model shows that orbital and CO2 variations induce, in the climate system, feedbacks sufficient to generate the low frequency part of the climatic variations over the last 200 kyr. Initiation and termination of glacial cycles cannot indeed be explained without invoking both the fast feedbacks associated with atmospheric processes (water vapor, cloud, snow and sea ice) and the slower feedbacks associated with coupling to other parts of the climate system, in particular the land ice-sheet buildup and disintegration. This model shows that long-term changes in the Earth's orbital parameters lead to variations in the amount of solar radiation received at the top of the atmosphere, which in turn act as a pacemaker for climatic variations at the astronomical frequencies, through induced albedo-temperature and greenhouse gases-temperature feedbacks. Spectral analysis of the Northern Hemisphere global ice volume variations simulated under both insolation and CO2 forcings reproduces correctly the relative intensity of the peaks at the orbital frequencies as seen in SPECMAP data. Except for variations with time scales shorter than 5 kyr, the simulated long-term variations of total ice volume are comparable to that reconstructed from deep-sea cores. For example, the model simulates glacial maxima of similar amplitudes at 134 kyr BP and 15 kyr BP, followed by abrupt deglaciations.     

Deep-sea carbonates: Reading the carbon-isotope signal

The carbon isotope signal in deep-sea sediments reflects a mix of (1) global changes in the rates of exchange of the ocean's carbon reservoir with biosphere, soil, and sediments, (2) global and regional changes in surface water productivity, (3) internal shifts in water-mass structure and circulation (basin-basin fractionation, oxygen minimum development), and (4) organism-specific fractionation effects due to changes in micro-habitat and/or ontogenic fractionation (»vital effects«). Additional complications arise from differential preservation. It is impossible to entirely isolate these various factors. As a rule of thumb, long period signals that are parallel for planktonic and benthic data reflect external (global) fractionation patterns, whilst short-period signals are more likely tied to internal patterns (water-mass fractionation). The various approaches to interpretation are illustrated with three case studies: the Glacial-Holocene transition, the Messinian Carbon Shift, and the Miocene Monterey Excursion.

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Zusammenfassung Das Kohlenstoff-Isotopensignal in den Tiefseesedimenten spiegelt ein Zusammenspiel wider, das (1) von den globalen Austauschraten des ozeanischen Kohlenstoffreservoirs mit der Biosphäre, den Böden und den Sedimenten gesteuert wird, (2) in dem ein globaler und regionaler Wechsel in der Produktivität des Oberflächenwassers und (3) interne Veränderungen in der Wassermassen-Struktur und -Zirkulation (Becken-zu-Becken-Fraktionierung, Sauerstoffminimumentwicklung) zum Ausdruck kommen, und (4) in dem eine spezifische Fraktionierung hervorgerufen durch die Milieuänderung im Lebensraum der Organismen und/oder ontogenetische Fraktionierung (»Vitaleffekte«) erscheint. Zusätzliche Komplikationen entstehen aus unterschiedlichen Erhaltungsmöglichkeiten. Es ist unmöglich, alle diese verschiedenen Faktoren vollständig zu isolieren. Als Faustregel kann man annehmen, daß langpenodische Signale, die parallel mit Plankton- und Benthosentwicklungen verlaufen, externe globale Fraktionierungstrends widerspiegeln, während kurzzeitige Signale eher an interne Muster gebunden sind (Fraktionierung innerhalb der Wassermassen). Die verschiedenen Möglichkeiten der Interpretation werden an speziellen Fällen diskutiert: am Übergang Pleistozän zu Holozän, an der Veränderung des Kohlenstoffverhältnisses im Messinium und an dem Monerey-Maximum im Miozän.

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Résumé Le signal isotopique du carbone enregistré dans les sédiments océaniques résulte d'un ensemble de mécanismes qui reflètent: 1) les variations globales dans l'intensité des échanges entre le réservoir du carbone de l'océan et la biosphère, les sols et les sédiments, 2) les variations globales et régionales de productivité des eaux de surface, 3) les changements dans la structure et la circulation des masses d'eaux (fractionnement de bassin à bassin, développement d'un niveau à minimum d'oxygène), et 4) les effets de fractionnement propres aux organismes, dûs à des changements de micro-habitat et/ou à un fractionnement au cours de l'ontogénie (»effet vital«). La préservation différentielle ajoute certaines difficultés d'interprétation. Il n'est pas possible d'isoler entièrement chacun de ces différents facteurs. D'une manière générale les signaux à longue période dont les variations sont parallèles pour les données planctoniques et benthiques correspondent à un fractionnement dû à des facteurs externes (globaux), alors que les signaux à courte période sont plus vraisemblablement liés à des facteurs internes (fractionnement des masses d'eaux). Trois cas étudiés permettent d'illustrer ces différents types d'interprétation: la transition Glaciaire/Holocène, le »décrochement Messinien« et l'»enrichissement de Monterey« au Miocène.

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Geochemical studies in the Indian Pass and Picacho Peak Bureau of Land Management Wilderness study areas, imperial county, Southern California

The U.S. Geological Survey has conducted geochemical studies in the Indian Pass (CDCA-355), 124 km², and Picacho Peak (CDCA-355A), 23 km², Wilderness Study Areas (WSA's) as part of a program to evaluate the mineral resource potential of designated areas in the California Desert Conservation Area. These two WSA's are of particular interest because they lie within a region which has intermittently produced significant quantities of Au since the mid-1800's, and is currently the site of much exploration activity for additional Au resources. Within a 15-km radius of the WSA's, there is one actively producing gold mine, a major deposit which began production in 1986, and one recently announced discovery. In the reconnaissance geochemical surveys of the two WSA's - 177 μm (-80 mesh) stream sediments, heavy-mineral concentrates from stream sediments, and rocks were prepared and analyzed.Four areas of possible exploration interest were identified within the WSA's. The first area is characterized by anomalous W and Bi in nonmagnetic heavy-mineral concentrates, and is underlain primarily by the Mesozoic Orocopia Schist which has been intruded by monzogranite of Oligocene age. Alteration and mineralization appear to be localized near the intrusive contact. The mineralized rock at the surface contains secondary Cu and Fe minerals where the monzogranite intrudes the metabasite horizons of the Orocopia Schist and scheelite where the monzogranite intrudes marble within the Orocopia Schist.The second area is characterized by anomalous As, Sb, Ba, B, and Sr in nonmagnetic heavy-mineral concentrates and by anomalous As in - 177 μm stream sediments. Geologically, this area is underlain by metasedimentary and metavolcanic rocks of Jurassic(?) age; a biotite monzogranite of Jurassic(?) age; and Tertiary volcanic and hypabyssal rocks composed of flows, domes, and tuffs of intermediate to silicic composition. All these rock types are cut by a set of north-south-striking normal faults. The anomalies in the heavy-mineral concentrates are believed to be related to silica-clay alteration observed in the vicinity of some of these faults.     

Fundamental processes controlling the first stage of alteration of a basalt glass by seawater: an experimental study between 200° and 320°C

The first stage of alteration of a basalt glass by seawater has been studied experimentally between 200° and 320°C under vapor pressure, following both the chemical evolution of the reacting solutions during the experiments and the chemical and mineralogical transformations of the altered glass surface via microprobe, scanning transmission electron microscope and resonant nuclear reactions.The alteration is controlled by diffusion of dissolved species through an altered layer and not by surface chemical reaction. Selective removal of cations with respect to SiO₂ leads to the formation of a thick, porous protonated surface layer enriched in SiO₂. Aqueous diffusion of dissolved species from the reacting glass and from solution through the pores of this layer results in the formation of an amorphous silicate gel which is the precursor of normal crystalline clays (saponites) appearing in a later stage.Computer simulations of the alteration generated with the EQ3/6 computer software package account for the chemical composition of the rim and the sequence of secondary minerals found in the experiments.     

The Origin and Distribution of Salts on Alluvial Fans in The Atacama Desert,Northern Chile

The Atacama Desert has been predominantly hyperarid since the middle Miocene. Combined ionic and X-ray diffraction analysis shows that calcium sulphate is prevalent on three similar alluvial fans in salar basins across a transect of different environments in Antofagasta Province, northern Chile. Differences between the fans were largely due to the effect of local factors on salt input, secondary redistribution and deposit preservation. Thus carbonate was notable in the High Andes (fan C) and Pre-Cordillera (fan B), whereas in the Central Valley (fan A) greater qualities of the more soluble salts (chlorides and nitrates) probably reflect the higher level of aridity and an oceanic source (the camanchaca). Calcium sulphate distribution on the alluvial fans and on adjacent hilltops indicates an aeolian origin. Evidence from the Pre-Cordillera (fan B), however, suggests that salt input may have been episodic, related to changes in conditions within the general aridity and possibly to stone pavement and soil development. Calcium sulphate sources range from an input in Andean precipitation and the camanchaca to abundant regional evaporite deposits. It is probable, however, that products of Andean volcanism constitute the dominant primary source of calcium sulphate, and that the salt has subsequently been distributed widely within the endoreic basins of the region by a combination of groundwater, surface flow and the wind. © 1997 John Wiley & Sons, Ltd.     

The planet formation imager

The Planet Formation Imager (PFI, www.planetformationimager.org) is a next-generation infrared interferometer array with the primary goal of imaging the active phases of planet formation in nearby star forming regions. PFI will be sensitive to warm dust emission using mid-infrared capabilities made possible by precise fringe tracking in the near-infrared. An L/M band combiner will be especially sensitive to thermal emission from young exoplanets (and their disks) with a high spectral resolution mode to probe the kinematics of CO and H₂O gas. In this paper, we give an overview of the main science goals of PFI, define a baseline PFI architecture that can achieve those goals, point at remaining technical challenges, and suggest activities today that will help make the Planet Formation Imager facility a reality.