965 resultados para UV-Ozone
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A number of liquid argon time projection chambers (LAr TPCs) are being built or are proposed for neutrino experiments on long- and short baseline beams. For these detectors, a distortion in the drift field due to geometrical or physics reasons can affect the reconstruction of the events. Depending on the TPC geometry and electric drift field intensity, this distortion could be of the same magnitude as the drift field itself. Recently, we presented a method to calibrate the drift field and correct for these possible distortions. While straight cosmic ray muon tracks could be used for calibration, multiple coulomb scattering and momentum uncertainties allow only a limited resolution. A UV laser instead can create straight ionization tracks in liquid argon, and allows one to map the drift field along different paths in the TPC inner volume. Here we present a UV laser feed-through design with a steerable UV mirror immersed in liquid argon that can point the laser beam at many locations through the TPC. The straight ionization paths are sensitive to drift field distortions, a fit of these distortion to the linear optical path allows to extract the drift field, by using these laser tracks along the whole TPC volume one can obtain a 3D drift field map. The UV laser feed-through assembly is a prototype of the system that will be used for the MicroBooNE experiment at the Fermi National Accelerator Laboratory (FNAL).
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Ozone-depleting substances emitted through human activitiescause large-scale damage to the stratospheric ozone layer, and influence global climate. Consequently, the production of many of these substances has been phased out; prominent examples are the chlorofluorocarbons (CFCs), and their intermediate replacements, the hydrochlorofluorocarbons (HCFCs). So far, seven types of CFC and six types of HCFC have been shown to contribute to stratospheric ozone destruction 1,2. Here, we report the detection and quantification of a further three CFCs and one HCFC. We analysed the composition of unpolluted air samples collected in Tasmania between 1978 and 2012, and extracted from deep firn snow in Greenland in 2008, using gas chromatography with mass spectrometric detection. Using the firn data, we show that all four compounds started to emerge in the atmosphere in the 1960s. Two of the compounds continue to accumulate in the atmosphere. We estimate that, before 2012, emissions of all four compounds combined amounted to more than 74,000 tonnes. This is small compared with peak emissions of other CFCs in the 1980s of more than one million tonnes each year 2. However, the reported emissions are clearly contrary to the intentions behind the Montreal Protocol, and raise questions about the sources of these gases.
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Vorbesitzer: Eljāqīm Carmoly; Abraham Merzbacher
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After major volcanic eruptions the enhanced aerosol causes ozone changes due to greater heterogeneous chemistry on the particle surfaces (HET-AER) and from dynamical effects related to the radiative heating of the lower stratosphere (RAD-DYN). We carry out a series of experiments with an atmosphere–ocean–chemistry–climate model to assess how these two processes change stratospheric ozone and Northern Hemispheric (NH) polar vortex dynamics. Ensemble simulations are performed under present day and preindustrial conditions, and with aerosol forcings representative of different eruption strength, to investigate changes in the response behaviour. We show that the halogen component of the HET-AER effect dominates under present-day conditions with a global reduction of ozone (−21 DU for the strongest eruption) particularly at high latitudes, whereas the HET-AER effect increases stratospheric ozone due to N2O5 hydrolysis in a preindustrial atmosphere (maximum anomalies +4 DU). The halogen-induced ozone changes in the present-day atmosphere offset part of the strengthening of the NH polar vortex during mid-winter (reduction of up to −16 m s-1 in January) and slightly amplify the dynamical changes in the polar stratosphere in late winter (+11 m s-1 in March). The RAD-DYN mechanism leads to positive column ozone anomalies which are reduced in a present-day atmosphere by amplified polar ozone depletion (maximum anomalies +12 and +18 DU for present day and preindustrial, respectively). For preindustrial conditions, the ozone response is consequently dominated by RAD-DYN processes, while under present-day conditions, HET-AER effects dominate. The dynamical response of the stratosphere is dominated by the RAD-DYN mechanism showing an intensification of the NH polar vortex in winter (up to +10 m s-1 in January). Ozone changes due to the RAD-DYN mechanism slightly reduce the response of the polar vortex after the eruption under present-day conditions.
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Adaptations to new pollinators involve multiple floral traits, each requiring coordinated changes in multiple genes. Despite this genetic complexity, shifts in pollination syndromes have happened frequently during angiosperm evolution. Here we study the genetic basis of floral UV absorbance, a key trait for attracting nocturnal pollinators. In Petunia, mutations in a single gene, MYB-FL, explain two transitions in UV absorbance. A gain of UV absorbance in the transition from bee to moth pollination was determined by a cis-regulatory mutation, whereas a frameshift mutation caused subsequent loss of UV absorbance during the transition from moth to hummingbird pollination. The functional differences in MYB-FL provide insight into the process of speciation and clarify phylogenetic relationships between nascent species.
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In a period of increasing concern about food safety, food poisoning outbreaks where unpasterurized apple cider or apple juice was found contaminated with Escherichia coli 0157:H7 reinforces the need for using the best technologies in apple cider production. Most apple cider is sold as an unpasteurized raw product. Because of their acidity, it was believed that juice products do not usually contain microorganisms such as E. coli 0157:H7, Salmonella, and Crytosporidium. Yet all of these foodborne pathogens are capable of being transmitted in unpasteurized juices. It is known that these pathogens can survive for several weeks in a variety of acidic juices. Although heat pasteurization is probably the best method to eliminate these pathogens, it is not the most desirable method as it changes sensory properties and also is very costly for small to mid-sized apple cider processors. Pasteurization of apple cider with Ultraviolet Irradiation (UV) is a potential alternative to heat pasteurization. Germicidal W irradiation is effective in inactivating microorganisms without producing undesirable by-products and changing sensory properties. Unpasteurized raw apple cider from a small local processor was purchased for this study. The effects of physical parameters, exposure time and dosage on the W treatment efficacy were examined as well as the effects of the UV light on apple cider quality. W light with principal energy at a wavelength of 254.7 nm, was effective in reducing bacteria (E .coli, ATCC 25922) inoculated apple cider. The W dosage absorbed by the apple cider was mathematically calculated. A radiation dose of 8,777 μW-s/cm2 reduced bacteria an average of 2.20 logs and in multiple passes, the FDA mandated 5-log reduction was achieved. Sensory analysis showed there was no significant difference between the W treated and non-treated cider. Experiments with W treated apple cider indicated a significant (p < 0.01) extension of product shelf life through inhibition of yeast and mold growth. The extension of the researched performed is applicable to other fruit juice processing operations.
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Excessive exposure to the UV radiation present in sunlight can lead to the development of skin cancer in humans. Majority of the UV-induced skin tumors in immune-competent mice are highly antigenic in nature. Additionally, they exhibit a high frequency of mutations in the p53 gene, which arise very early in the course of UV radiation and most of them disappear before the development of skin tumors. ^ Initially, this study was to determine whether UV radiation induces skin tumors much earlier in immune deficient Rag2 knockout mice than in immune-competent mice, and if so, compare their antigenic properties and p53 mutation spectra. However, chronic UV irradiation (10 kJ/m2) induced myeloproliferative disease (MPD) as early as 4 weeks in Rag2 knockout mice instead of skin tumors. Conversely, unirradiated Rag2 knockout mice developed MPD at a low frequency, but the frequency increased with the animal's age. Although the UV-irradiated wild type mice (B6129) developed MPD, its frequency was lower and the occurrence much later than the Rag2 knockout mice. ^ This observation led to our new hypothesis that UV irradiation plays a role in the development of MPD in Rag2 knockout mice. After 4 weeks of UV radiation, both histopathology (myeloid:erythroid ratio, number of blast cells) and flow cytometry (mature myeloid, granulocytes and immature cells) demonstrated an increased number of mice affected with the disease in the UV-irradiated Rag2 knockout group than the other groups. ^ We also investigated the role of cytokines and absence of T and B cells in the development of MPD in the Rag2 knockout mice. Results indicated that IL-3 and IL-3Rα chain expression was upregulated in the spleens of the UV-irradiated Rag2 knockout mice (4 weeks). Reconstitution of the Rag2 knockout mice with T and B cells abrogated the UV-accelerated development of MPD. Both histopathology and flow cytometric analysis (mature myeloid cells, granulocytes) showed a decrease in the number of mice affected with the disease in the UV-irradiated, reconstituted group rather than any other group. In summary, this study provides the first experimental evidence that exposure to UV irradiation can lead to the development of MPD in immune deficient mice. ^
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Skin cancer is the most common malignancy in humans. Although highly treatable, non-melanoma skin cancer is commonly followed by other non-cutaneous malignancies. Ultraviolet radiation (UVR) acts as both tumor initiator and promoter, and also results in the suppression of specific immune responses. The systemic suppression of immune responses is initiated by DNA damage, which promotes IL-10 production, an important cytokine as anti-IL-10 can abrogate the suppression, and upregulates the pro-apoptotic proteins Fas and Fas ligand (FasL). FasL is a critical factor for UV-induced immune suppression, and the suppressor cell induced by UV expresses FasL. ^ We hypothesized that the microenvironment affects Fas/FasL interactions, and that these interactions are important to the phenomenon of UV induced immune suppression. To determine the effects of the interaction of FasL and IL-10, splenocytes isolated from C57Bl/6 mice were cultured in the presence or absence of IL-10 post-mitogenic activation. We determined that IL-10 protects from Fas-mediated apoptosis by lowering Fas sensitivity and lowering the levels of either Fas or FasL. This protection is stronger when IL-10 is given immediately after mitogenic activation, and does not increase any of the inhibitors of apoptosis studied. In vivo, splenocytes from UV-irradiated mice are resistant to Fas-mediated apoptosis and present very high levels of IL-10, lowered Fas sensitivity and lowered caspase cleavage despite higher expression of Fas and FasL than non-irradiated mice. ^ UV-induced immune suppression affects female mice preferentially, which led us to look at prolactin as a possible component of this suppression since this hormone has also been associated with increased skin carcinogenesis. The interaction of FasL and prolactin results in suppression of the delayed type hypersensitivity response to Candida albicans. This lack of response depends on FasL as is not seen in gld mice. Similar to UV-induced immune suppression, the suppression is caused by a Th2 deviation, and correlates with a significant increase in Fas expression. In the presence of UV, the effects of prolactin seemed to be protective, and UV actually restores the DTH response.^ Taken together, these observations suggest that the microenvironment dictates the outcome of the interaction of FasL with Fas going from promoting apoptosis to preventing apoptosis or mediating a Th2 deviation and suppression of a Th1 response. ^
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Exposure to UVB radiation induces local and systemic immune suppression, evidenced by inhibition of the contact hypersensitivity response (CHS). Epidermal dendritic cells, the primary antigen presenting cells responsible for the induction of CHS, are profoundly altered in phenotype and function by UVB exposure and possess UV-specific DNA damage upon migrating to skin-draining lymph nodes. Expression of the proapoptotic protein FasL has been demonstrated in both skin and lymph node cells following UVB exposure. Additionally, functional FasL expression has recently been demonstrated to be required in the phenomenon of UV-induced immune suppression. To test the hypothesis that FasL expression by DNA-damaged Langerhans cells migrating to the skin-draining lymph nodes is a crucial event in the generation of this phenomenon, mice were given a single 5KJ/m2 UV-B exposure and sensitized to 0.5% FITC through the exposed area. Dendritic cells (DC) harvested from skin-draining lymph nodes (DLN) 18 hours following sensitization by magnetic CD11c-conjugated microbeads expressed high levels of Iab, CD80 and CD86, DEC-205 and bore the FITC hapten, suggesting epidermal origin. Radioimmunoassay of UV-specific DNA damage showed that DC contained the vast majority of cyclobutane pyrimidine dimers (CPDs) found in the DLN after UVB and exhibited increased FasL mRNA expression, a result which correlated with greatly increased FasL-mediated cytotoxicity. The ability of DCs to transfer sensitization to naïve hosts was lost following UVB exposure, a phenomenon which required DC FasL expression, and was completely reversed by cutaneous DNA repair. Collectively, these results demonstrate the central importance of DNA damage-induced FasL expression on migrating dendritic cells in mediating UV-induced suppression of contact hypersensitivity. ^
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There is evidence that ultraviolet radiation (UVR) is increasing over certain locations on the Earth's surface. Of primary concern is the annual pattern of ozone depletion over Antarctica and the Southern Ocean. Reduction of ozone concentration selectively limits absorption of solar UV-B (290–320 nm), resulting in higher irradiance at the Earth's surface. The effects of ozone depletion on the human population and natural ecosystems, particularly the marine environment, are a matter of considerable concern. Indeed, marine plankton may serve as sensitive indicators of ozone depletion and UV-B fluctuations. Direct biological effects of UVR result from absorption of UV-B by DNA. Once absorbed, energy is dissipated by a variety of pathways, including covalent chemical reactions leading to the formation of photoproducts. The major types of photoproduct formed are cyclobutyl pyrimidine dimer (CPD) and pyrimidine(6-4)pyrimidone dimer [(6-4)PD]. Marine plankton repair these photoproducts using light-dependent photoenzymatic repair or nucleotide excision repair. The studies here show that fluctuations in CPD concentrations in the marine environment at Palmer Station, Antarctica correlate well with ozone concentration and UV-B irradiance at the Earth's surface. A comparison of photoproduct levels in marine plankton and DNA dosimeters show that bacterioplankton display higher resistance to solar UVR than phytoplankton in an ozone depleted environment. DNA damage in marine microorganisms was investigated during two separate latitudinal transects which covered a total range of 140°. We observed the same pattern of change in DNA damage levels in dosimeters and marine plankton as measured using two distinct quantitative techniques. Results from the transects show that differences in photosensitivity exist in marine plankton collected under varying UVR environments. Laboratory studies of Antarctic bacterial isolates confirm that marine bacterioplankton possess differences in survival, DNA damage induction, and repair following exposure to UVR. Results from DNA damage measurements during ozone season, along a latitudinal gradient, and in marine bacterial isolates suggest that changes in environmental UVR correlate with changes in UV-B induced DNA damage in marine microorganisms. Differences in the ability to tolerate UVR stress under different environmental conditions may determine the composition of the microbial communities inhabiting those environments. ^