Academic literature on the topic 'Mercury Vapor Light'

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Journal articles on the topic "Mercury Vapor Light"

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Mohanraj, D., R. Janarthanan, and S. Suresh. "Response of Rice Pests to Mercury Vapor Light and Black Light Traps." International Rice Research Newsletter 14, no. 4 (1989): 37. https://doi.org/10.5281/zenodo.7146928.

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This article 'Response of Rice Pests to Mercury Vapor Light and Black Light Traps' appeared in the International Rice Research Newsletter series, created by the International Rice Research Institute (IRRI). The primary objective of this publication was to expedite communication among scientists concerned with the development of improved technology for rice and for rice based cropping systems. This publication will report what scientists are doing to increase the production of rice in as much as this crop feeds the most densely populated and land scarce nations in the world.
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Hughes, William A. "City of Portland Conversion to Cut-off Fixtures." International Astronomical Union Colloquium 112 (1991): 100. http://dx.doi.org/10.1017/s025292110000381x.

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In 1980, the City of Portland began a conversion project to change out all existing mercury vapor street lights to high pressure sodium. During the planning and design portion of the project, the City hired a consulting firm to look at our existing system and make recommendations as to light source and fixture configuration. After some on site studies of existing street lighting, it was recommended that all arterial streets of the City of Portland be converted from mercury vapor to high pressure cut-off fixtures, in order to cut down glare in the eyes of drivers. Secondly, it was recommended that, on arterial streets, the City could no longer afford to light “key-hole to key-hole.” It was important to confine the light to the street right-of-way.
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Nicolau, Talita, Núbio Gomes Filho, Jorge Padrão, and Andrea Zille. "A Comprehensive Analysis of the UVC LEDs’ Applications and Decontamination Capability." Materials 15, no. 8 (2022): 2854. http://dx.doi.org/10.3390/ma15082854.

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The application of light-emitting diodes (LEDs) has been gaining popularity over the last decades. LEDs have advantages compared to traditional light sources in terms of lifecycle, robustness, compactness, flexibility, and the absence of non-hazardous material. Combining these advantages with the possibility of emitting Ultraviolet C (UVC) makes LEDs serious candidates for light sources in decontamination systems. Nevertheless, it is unclear if they present better decontamination effectiveness than traditional mercury vapor lamps. Hence, this research uses a systematic literature review (SLR) to enlighten three aspects: (1) UVC LEDs’ application according to the field, (2) UVC LEDs’ application in terms of different biological indicators, and (3) the decontamination effectiveness of UVC LEDs in comparison to conventional lamps. UVC LEDs have spread across multiple areas, ranging from health applications to wastewater or food decontamination. The UVC LEDs’ decontamination effectiveness is as good as mercury vapor lamps. In some cases, LEDs even provide better results than conventional mercury vapor lamps. However, the increase in the targets’ complexity (e.g., multilayers or thicker individual layers) may reduce the UVC decontamination efficacy. Therefore, UVC LEDs still require considerable optimization. These findings are stimulating for developing industrial or final users’ applications.
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Darvishi, Ebrahim, Mohammad Javad Assari, Maryam Farhadian, Ebrahim Chavoshi, and Hamid Reza Ehsani. "Occupational exposure to mercury vapor in a compact fluorescent lamp factory: Evaluation of personal, ambient air, and biological monitoring." Toxicology and Industrial Health 35, no. 4 (2019): 304–13. http://dx.doi.org/10.1177/0748233719831531.

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Compact fluorescent lamps (CFLs) have become a popular lighting choice in recent years despite the good performance of light-emitting diode (LED) lamps. The CFLs that have been produced recently contain 1.5–3.5 mg Hg/lamp. There is evidence that even low doses of mercury are toxic. This study aimed to assess occupational exposure to mercury vapor in workers of a CFLs factory by determining mercury levels in personal and ambient air samples and urine of workers. This cross-sectional study was conducted on 59 workers in a CFLs factory in Iran. Personal and ambient air sampling of mercury vapor levels (MVLs) was performed during a workday. In total, 10 personal samples and 10 ambient air samples of mercury vapor were collected simultaneously from different units of the factory. Urine samples were collected before the work shift. Samples were analyzed using a cold-vapor atomic absorption spectrophotometer (CVAAS). The mean of the MVLs in the personal and ambient air samples was 14.78 ± 5.76 and 67.10 ± 59.37 µg.m−3, respectively. The highest MVL was measured for the production line supervisor (25 µg.m−3). There was a significant correlation between the MVLs in the ambient air and personal samples ( r = 0.84, p = 0.005). The mean urinary mercury level (UML) was 13.85 ± 13.14 µg/g creatinine. The UML of 86.4% workers was below the 20 µg/g creatinine recommended by the Centre of Environmental and Occupational Health in Iran. There were significant differences between the UMLs in different areas of the factory ( p = 0.041). Lamp breakage was an important determinant of exposure to mercury vapor; hence, effective programs to control mercury vapor are essential in the CFLs industry.
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van Grunsven, Roy H. A., Julia Becker, Stephanie Peter, Stefan Heller, and Franz Hölker. "Long-Term Comparison of Attraction of Flying Insects to Streetlights after the Transition from Traditional Light Sources to Light-Emitting Diodes in Urban and Peri-Urban Settings." Sustainability 11, no. 22 (2019): 6198. http://dx.doi.org/10.3390/su11226198.

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Among the different light sources used for street lighting, light-emitting diodes (LEDs) are likely to dominate the world market in the coming years. At the same time, the spectral composition of nocturnal illumination is changing. Europe and many other areas worldwide have implemented bans on energy-inefficient lamps, such as the still very common mercury vapor lamps. However, the impact of artificial light on insects is mostly tested with light-traps or flight-intercept traps that are used for short periods only. By comparing the numbers of insects attracted by street lamps before and after replacing mercury vapor light sources (MV) with light emitting diodes, we assessed the impact in more typical (urban and peri-urban) settings over several years. We found that LED attracted approximately half of the number of insects compared to MV lights. Furthermore, most insect groups are less drawn by LED than by MV, while Hymenoptera are less attracted by MV than by LED. Thus, the composition of the attracted communities differed between the light sources, which may impact ecosystem processes and functions. In green peri-urban settings more insects are attracted than in an urban setting, but the relative difference between the light sources is the same.
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Kolevzon, V., G. Gerbeth, and G. Pozdniakov. "Light-scattering study of the mercury liquid-vapor interface." Physical Review E 55, no. 3 (1997): 3134–42. http://dx.doi.org/10.1103/physreve.55.3134.

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Arroyo-Lamas, Nagore, Unai Ugalde, and Iciar Arteagoitia. "Decontamination of Ti Oxide Surfaces by Using Ultraviolet Light: Hg-Vapor vs. LED-Based Irradiation." Antibiotics 9, no. 11 (2020): 724. http://dx.doi.org/10.3390/antibiotics9110724.

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C-range Ultraviolet (UVC) mercury (Hg)-vapor lamps have shown the successful decontamination of hydrocarbons and antimicrobial effects from titanium surfaces. This study focused on surface chemistry modifications of titanium dental implants by using two different light sources, Hg-vapor lamps and Light Emitting Diodes (LEDs), so as to compare the effectivity of both photofunctionalization technologies. Two different devices, a small Hg-vapor lamp (λ = 254 nm) and a pair of closely placed LEDs (λ = 278 nm), were used to irradiate the implants for 12 min. X-ray Photoelectron Spectroscopy (XPS) was employed to characterize the chemical composition of the surfaces, analysing the samples before and after the lighting treatment, performing a wide and narrow scan around the energy peaks of carbon, oxygen and titanium. XPS analysis showed a reduction in the concentration of surface hydrocarbons in both UVC technologies from around 26 to 23.4 C at.% (carbon atomic concentration). Besides, simultaneously, an increase in concentration of oxygen and titanium was observed. LED-based UVC photofunctionalization has been suggested to be as effective a method as Hg-vapor lamps to remove the hydrocarbons from the surface of titanium dental implants. Therefore, due to the increase in worldwide mercury limitations, LED-based technology could be a good alternative decontamination source.
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Santiago-Jiménez, Quiyari J. "Two new species of Myrmedonota Cameron (Staphylinidae, Aleocharinae) from Mexico." ZooKeys 464 (December 16, 2014): 49–62. https://doi.org/10.3897/zookeys.464.8549.

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Two new species of Myrmedonota are described from Mexico. Illustrations and a distribution map are provided, as are keys to identify Myrmedonota known from the Nearctic and Neotropics. Specimens were collected by means of mercury vapor light traps or flight interception traps.
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Nguyen, Thuong Thi Kim, Huyen Thu Luu, Loi Duc Vu, Thao Thi Ta, and Giang Thi Huong Le. "Determination of Total Mercury in Solid Samples by Anodic Stripping Voltammetry." Journal of Chemistry 2021 (January 12, 2021): 1–8. http://dx.doi.org/10.1155/2021/8888879.

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The anodic stripping voltammetry (ASV) was investigated to determine total mercury in solid samples using a gold electrode. The mercury was deposited on the gold electrode in a preconcentration step. The oxidation peak of mercury was irreversible. The optimal conditions of the procedure were found to be as follows: 0.05 mol L−1 HCl solution, deposition potential −0.5 V vs. Ag/AgCl/KCls, deposition time 40 s, and sweep rate 0.04 V s−1. Under the optimal conditions, the peak current showed a linear dependence on Hg2+ concentration in the range from 0.01 to 0.1 mg l−1. The detection limit and quantification limit were 4.28 µg L−1 and 12.98 µg L−1, respectively. The mean recovery and relative standard deviation were 91.2% and 2.4% (n = 9). The procedure was successfully applied for determining total mercury in samples collected from Hanoi light bulb warehouse—The Rang Dong Light Source and Vacuum Flask JSC. The results were compared with cold vapor atomic absorption spectrometry (CV-AAS).
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DANCĂ, Paul Alexandru, Florentina BUNEA, Marius LUNGULESCU, Alin Alexandru ENACHE, Andreea-Elena RĂDOI, and Nicoleta NICULA. "Water Sterilization using Ultraviolet Light-Emitting Diodes." Electrotehnica, Electronica, Automatica 72, no. 1 (2024): 23–29. http://dx.doi.org/10.46904/eea.24.72.1.1108003.

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In order to provide adequate living conditions, it is crucial for each building to have access to essential utilities such as water, electricity, and sewage systems. In some regions, they may experience isolation, but they can still establish connections to distribution networks and fulfill basic living requirements. In such cases, local solutions like wells and septic tanks are implemented. The water sourced from these sources contains a multitude of viruses and bacteria that can have a detrimental effect on the health of anyone who consumes it. Numerous water filtration/sterilization options are available on the market, but they come with significant installation, maintenance, and operating expenses. The use of ultraviolet C (UVC) rays generated by mercury lamps for sterilization by irradiation is becoming increasingly popular due to its cost-effectiveness in terms of installation and maintenance. The main drawbacks of this technique are the high energy consumption and the potential danger of mercury exposure. This article describes the processes for designing, making, and testing two water filtration probes that use light-emitting diodes (LED) diodes to emit UVC rays. This solution lowers energy consumption eliminates the risk of mercury contamination, and leads to a decrease in maintenance costs, as the lifespan of diodes is longer than that of mercury vapor lamps. The two probes have LED diodes that emit at a wavelength of 275 nm, with a total radiant flux of 12 mW and 100 mW, respectively. Biological tests were carried out in the laboratory to assess the effects of these probes on an artificially contaminated water sample. The results obtained are satisfactory and comparable to those of sterilization devices with LED lamps.
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Dissertations / Theses on the topic "Mercury Vapor Light"

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McGeachie, W. J. "The effects of air temperature, wind vectors and nocturnal illumination on the behavior of moths at mercury-vapour light-traps." Thesis, Cranfield University, 1987. http://dspace.lib.cranfield.ac.uk/handle/1826/11424.

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Field experiments, with 125 watt Mercury-Vapour light-traps, are described in this Thesis. Catches of moths in water traps arranged in a circular mosaic pattern around the light-trap were distributed bivariate normal. Comparisons between the bivariate mean moth vector and the mean wind vector suggested that the wind vector determined the distribution of moths around the light-trap. In light winds, less than 1 metre/second, moths were randomly distributed around the trap. In stronger winds the direction of moth displacement from the trap was associated with the direction component of the mean wind velocity. A second experiment with light and water traps was used to estimate the effective light-trap radius. Two light-traps, surrounded by water traps, were separated by up to 25 metres on different evenings. When one light-trap was downwind of another the catch was significantly greater in the downwind trap. However, in crosswind conditions the two catches were similar. Bivariate methods were used to estimate that the effective trap radius was between 10 and 25 metres. A further experiment, using multivariate correlation and regression analysis, found that air temperature, windspeed and moonlight affected light-trap catches. An algorithm is described to enable the calculation of moonlight illuminance. Increased windspeed and increased moonlight illuminance tended to decrease the light-trap catch, however, increased air temperature was associated with an increase in light-trap catch. These effects varied depending on family and species. A final experiment used a remote sensing technique to estimate light-trap efficiency. A 10 cubic metre volume around the light-trap was observed using a video camera. Moth tracks recorded were classified into New Arrivals, Passers By and Local Flights. The number of these tracks was compared to the lighttrap catch so that efficiency estimates could be obtained. Results suggested that at ground level, 125 watt Mercury-Vapour light-traps are only 20 % efficient within this 10 cubic metre volume.
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McGeachie, William J. "The effects of air temperature, wind vectors and nocturnal illumination on the behaviour of moths at mercury-vapour light-traps." Thesis, Cranfield University, 1987. http://dspace.lib.cranfield.ac.uk/handle/1826/11424.

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Field experiments, with 125 watt Mercury-Vapour light-traps, are described in this Thesis. Catches of moths in water traps arranged in a circular mosaic pattern around the light-trap were distributed bivariate normal. Comparisons between the bivariate mean moth vector and the mean wind vector suggested that the wind vector determined the distribution of moths around the light-trap. In light winds, less than 1 metre/second, moths were randomly distributed around the trap. In stronger winds the direction of moth displacement from the trap was associated with the direction component of the mean wind velocity. A second experiment with light and water traps was used to estimate the effective light-trap radius. Two light-traps, surrounded by water traps, were separated by up to 25 metres on different evenings. When one light-trap was downwind of another the catch was significantly greater in the downwind trap. However, in crosswind conditions the two catches were similar. Bivariate methods were used to estimate that the effective trap radius was between 10 and 25 metres. A further experiment, using multivariate correlation and regression analysis, found that air temperature, windspeed and moonlight affected light-trap catches. An algorithm is described to enable the calculation of moonlight illuminance. Increased windspeed and increased moonlight illuminance tended to decrease the light-trap catch, however, increased air temperature was associated with an increase in light-trap catch. These effects varied depending on family and species. A final experiment used a remote sensing technique to estimate light-trap efficiency. A 10 cubic metre volume around the light-trap was observed using a video camera. Moth tracks recorded were classified into New Arrivals, Passers By and Local Flights. The number of these tracks was compared to the lighttrap catch so that efficiency estimates could be obtained. Results suggested that at ground level, 125 watt Mercury-Vapour light-traps are only 20 % efficient within this 10 cubic metre volume.
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Krbal, Michal. "Účinnost přeměny elektrické energie na světlo u současných světelných zdrojů." Master's thesis, Vysoké učení technické v Brně. Fakulta elektrotechniky a komunikačních technologií, 2010. http://www.nusl.cz/ntk/nusl-218541.

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The goal of this diploma’s thesis is to inform about present development of light sources, new technologies and about achieved parameters of these light sources. The thesis is mainly directed to describe efficiency of transformation electric energy to light at single types of light sources. There are described the concrete technical parameters of sources quoted by manufacturers and the contructional solution of single types of light sources. There is created a graphic comparation of electrotechnical and light parameters of the light sources.
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Books on the topic "Mercury Vapor Light"

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Claudia, Karstedt, ed. Lügendes Licht: Die dunklen Seiten der Energiesparlampe. S. Hirzel Verlag, 2011.

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Book chapters on the topic "Mercury Vapor Light"

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Barocchi, F., M. Sampoli, F. Hensel, J. Rathenow, and R. Winter. "The Depolarized Interaction Induced Light Scattering Spectrum of Mercury Vapor at Low Density." In Collision- and Interaction-Induced Spectroscopy. Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0183-7_26.

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El-Kader, M. S. A., and S. M. El-Sheikh. "Collision-Induced Light Scattering Spectra of Mercury Vapor at Different Temperatures." In International Conference of Computational Methods in Sciences and Engineering 2004 (ICCMSE 2004). CRC Press, 2019. http://dx.doi.org/10.1201/9780429081385-271.

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Rytuba, James J. "Epithermal Precious-Metal and Mercury Deposits in the Sonoma and Clear Lake Volcanic Fields, California." In Active Geothermal Systems and Gold-Mercury Deposits in the Sonoma-Clear Lake Volcanic Fields, California. Society of Economic Geologists, 1993. http://dx.doi.org/10.5382/gb.16.03.

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Abstract Epithermal precious-metal and mercury deposits are present in the Sonoma and Clear Lake volcanic fields of central California and several hot springs in the Clear Lake volcanic field are presently depositing mercury and gold. The deposits and hot springs are associated with late Miocene to Holocene volcanic centers developed above a zone of thin crust and hot asthenosphere termed a slab window (Dickinson and Snyder, 1979, Benz and others, 1992) as the end of Pacific plate subduction was marked by the passage of the Mendocino triple junction along the California coast. Mercury deposition is actively occurring at the Sulphur Bank mercury mine, but no precious metals are present there because the geothermal system is vapor-dominated. In the water dominated geothermal systems at Wilbur Springs (Peters, 1990, Donnelly and others, 1993) and springs near the Cherry Hill gold deposit, both cinnabar and gold are being deposited (Pearcy and Petersen, 1990). Transport of mercury and gold is in a fluid which also contains high concentrations of petroleum and associated methane and CO2 derived from thermal degradation of organic matter in sedimentary rocks (Peabody, 1989). Chemical and isotopic analysis of oxygen and deuterium of the hot springs indicate that three types of fluid are present: moderate chloride, isotopically heavy, evolved formation fluid equilibrated with oceanic sedimentary rocks; evolved meteoric water; and isotopically light meteoric water (Peters, 1990,1991, Sherlock and Jowett, 1992, and Donnelly-Nolan and others, 1993). High concentrations of Hg, As, Sb, Au, and Ag occur in precipitates from hot springs composed dominantly of the isotopically heavy fluid, but not in the moderate-temperature, oxidized springs that are mixtures of these two fluid types (Peters, 1990, Donnelly-Nolan and others, 1993). The McLaughlin gold deposit (initial reserves of 2.9 million oz of gold) is economically the most important deposit in the Clear Lake and Sonoma volcanic fields. This precious metal-mercury hydrothermal system developed within and adjacent to andesitic vents and dikes emplaced along the Stony Creek fault zone (Lehrman, 1986). Gold occurs in opal, chalcedony, and quartz veins, and the highest gold values typically occur in amber to brown opal containing petroleum. Gold occurs in several sites within the petroleum-bearing opal: as a filling of 2050 micron- diameter oval voids representing large fluid inclusions; as 2-4 micron size crystals that coalesce to form dendrites of gold along primary vein banding; and in syneresis cracks which cut the vein banding. Oxide phases of Ga, In, Sn, and Ni are present within the petroleum-bearing opal. The isotopically heavy McLaughlin ore fluid plots in the field of andesitic magma volatiles (Hedenquist and Aoki, 1990, Giggenbach, 1987) and evolved formation waters (Sherlock and Jowett, 1992) suggesting that these two components are present Andesitic vents and dikes at the McLaughlin gold deposit suggest that a larger intrusion underlies the area and provided the heat source for the hydrothermal system. Andesitic vents along the Stony Creek fault provided a conduit for volatiles degassing from the intrusion to become entrained within the hydrothermal fluid composed of gas-oil-field water derived from the Great Valley sequence. The McLaughlin gold deposit reflects the complex interaction of three types of fluid each transporting a different elemental suite: evolved gas-oil field formation water transporting petroleum, Ga, In, Sn, Ni, and Hg; andesitic magmatic fluid transporting Au, Ag, Hg, Sb, and As; and near-surface meteoric water. Prospective areas for precious metal hot-spring deposits occur in the volcanic-structural environment above the thin crust and hot asthenosphere within the slab window in the Coast Ranges and parts of the Great Valley sequence where blind thrusts and associated faults are intruded by Pliocene to Holocene intrusive rocks. Mercury deposits with little or no gold content form along major structures from gas-oil field fluids with little or no magmatic component in the fluid and contain petroleum, Ni, Ga, In, Sn, and other transition elements. Epithermal gold deposits contain a significant magmatic component characterized by Au, Ag, As, Sb, and Hg as well as a gas-oil- field fluid component characterized by petroleum and transition metals. Both deposit types may occur along the same structures.
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Sherlock, Ross L. "The Genesis of the Mclaughlin Mine Sheeted Vein Complex, Fluid Inclusion and Stable Isotope Evidence." In Active Geothermal Systems and Gold-Mercury Deposits in the Sonoma-Clear Lake Volcanic Fields, California. Society of Economic Geologists, 1993. http://dx.doi.org/10.5382/gb.16.19.

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Abstract The McLaughlin Mine is a hot-spring type gold-mercury deposit located in the Coast Ranges of northern California. The “sheeted vein complex” is the center of the hot-spring system that formed the McLaughlin deposit. The sheeted vein complex merges from a subaerial siliceous sinter into a bilaterally symmetric, subparallel, multistage vein swarm. The precious metals are well zoned with gold largely restricted to the upper 200 m of the deposit. Silver can dominate anywhere in the system but is always more abundant than gold below 200 m. Below 350 m, silver is rare, gold has not been observed and mineralization is dominated by base metal sulfides. Fluid inclusion analysis suggest that the ore forming fluids were low salinity NaCl dominated, low CO2 fluids. The deepest samples (> 800 m below the paleosurface) have an average temperature of 235°C. The ascending hydrothermal fluid intersected the hydrostatic boiling curve at ~400 m below the surface and paralleled the hydrostatic boiling curve to the surface. Boiling of an ascending hydrothermal fluid accounts for the metal zoning observed in the sheeted vein complex. During boiling CO2 is partitioned into the vapor phase faster than H2S, resulting in the deeper portion. 3f the ore body being enriched in silver with respect to gold and the shallow portions of the ore body enriched in gold with respect to silver. On the basis of the physical and chemical conditions of the ore forming fluids, gold grade, as well as silica and temperature gradients the hydrothermal fluid is undersaturated with respect to gold prior to the onset of boiling. There is a strong trend for increasingly light δ18Oqtz with depth. The most isotopically enriched samples are from the subaerial sinter and the lightest sample are from the deepest samples. This trend is a temperature effect and is the result of increasing fractionation with decreasing temperature. The oxygen isotopic composition of the hydrothermal fluid remained fairly constant at ~93%o. The oxygen and deuterium composition of the hydrothermal fluids are consistent with a meteoric water origin. The hydrothermal fluids have a pronounced oxygen shift due to water/rock interaction but do not have a deuterium shift. The water/rock ratios are low but similar to other geothermal systems in the Coast Ranges and other epithermal deposits emplaced within sedimentary sequences.
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Conference papers on the topic "Mercury Vapor Light"

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Lin, H.-B., J. D. Eversole, and A. J. Campillo. "Resonance light scattering in coated microspheres." In OSA Annual Meeting. Optica Publishing Group, 1989. http://dx.doi.org/10.1364/oam.1989.wl4.

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Small spherical particles (from 5 to 30 µm) were charged and suspended in an electric quadrupole trap which was mounted in a chamber connected to a vacuum pump. The particles were coated with a liquid having a relatively low vapor pressure at normal atmosphere (such as glycerine). When the chamber was evacuated, light from a He-Ne laser scattered at right angles from the coated particle was monitored as the liquid coating shrank due to evaporation. Sharp variations in the scattered light intensity as a function of changing particle size are termed Mie resonances or partial wave resonances occurring when the wavelength and particle radius match a spherical cavity-type mode. For the large layer thickness, this resonance spectrum matches that of the homogeneous liquid droplet (both experimentally and computationally). However, significant deviations occur when the layer thickness comes within a few optical wavelengths of the core surface. Observations were made for glass, mercury, and polystyrene cores. An exact computational model for concentric spheres with differing indices of refraction accounts for much of the observed spectra. Discrepancies are discussed in terms of the model restrictions of concentricity and step function layer-core boundary.
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Barocchi, F., M. Sampoli, and L. Ulivi. "Collision induced light scattering in metal vapors: The mercury spectra." In The 13th international conference on spectral line shapes. AIP, 1997. http://dx.doi.org/10.1063/1.51800.

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