959 resultados para UV-RADIATION


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Abstract Background The use of lignocellulosic constituents in biotechnological processes requires a selective separation of the main fractions (cellulose, hemicellulose and lignin). During diluted acid hydrolysis for hemicellulose extraction, several toxic compounds are formed by the degradation of sugars and lignin, which have ability to inhibit microbial metabolism. Thus, the use of a detoxification step represents an important aspect to be considered for the improvement of fermentation processes from hydrolysates. In this paper, we evaluated the application of Advanced Oxidative Processes (AOPs) for the detoxification of rice straw hemicellulosic hydrolysate with the goal of improving ethanol bioproduction by Pichia stipitis yeast. Aiming to reduce the toxicity of the hemicellulosic hydrolysate, different treatment conditions were analyzed. The treatments were carried out according to a Taguchi L16 orthogonal array to evaluate the influence of Fe+2, H2O2, UV, O3 and pH on the concentration of aromatic compounds and the fermentative process. Results The results showed that the AOPs were able to remove aromatic compounds (furan and phenolic compounds derived from lignin) without affecting the sugar concentration in the hydrolysate. Ozonation in alkaline medium (pH 8) in the presence of H2O2 (treatment A3) or UV radiation (treatment A5) were the most effective for hydrolysate detoxification and had a positive effect on increasing the yeast fermentability of rice straw hemicellulose hydrolysate. Under these conditions, the higher removal of total phenols (above 40%), low molecular weight phenolic compounds (above 95%) and furans (above 52%) were observed. In addition, the ethanol volumetric productivity by P. stipitis was increased in approximately twice in relation the untreated hydrolysate. Conclusion These results demonstrate that AOPs are a promising methods to reduce toxicity and improve the fermentability of lignocellulosic hydrolysates.

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UVA light (320–400 nm) represents approximately 95% of the total solar UV radiation that reaches the Earth’s surface. UVA light induces oxidative stress and the formation of DNA photoproducts in skin cells. These photoproducts such as pyrimidine dimers (cyclobutane pyrimidine dimers, CPDs, and pyrimidine (6-4) pyrimidone photoproducts, 6-4PPs) are removed by nucleotide excision repair (NER). In this repair pathway, the XPA protein is recruited to the damage removal site; therefore, cells deficient in this protein are unable to repair the photoproducts. The aim of this study was to investigate the involvement of oxidative stress and the formation of DNA photoproducts in UVA-induced cell death. In fact, similar levels of oxidative stress and oxidised bases were detected in XP-A and NER-proficient cells exposed to UVA light. Interestingly, CPDs were detected in both cell lines; however, 6-4PPs were detected only in DNA repairdeficient cells. XP-A cells were also observed to be significantly more sensitive to UVA light compared to NER-proficient cells, with an increased induction of apoptosis, while necrosis was similarly observed in both cell lines. The induction of apoptosis and necrosis in XP-A cells using adenovirus-mediated transduction of specific photolyases was investigated and we confirm that both types of photoproducts are the primary lesions responsible for inducing cell death in XP-A cells and may trigger the skin-damaging effects of UVA light, particularly skin ageing and carcinogenesis.

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DNA damage induced by ultraviolet (UV) radiation can be removed by nucleotide excision repair through two sub-pathways, one general (GGR) and the other specific for transcribed DNA (TCR), and the processing of unrepaired lesions trigger signals that may lead to cell death. These signals involve the tumor suppressor p53 protein, a central regulator of cell responses to DNA damage, and the E3 ubiquitin ligase Mdm2, that forms a feedback regulatory loop with p53. The involvement of cell cycle and transcription on the signaling to apoptosis was investigated in UVB-irradiated synchronized, DNA repair proficient, CS-B (TCR-deficient) and XP-C (GGR-deficient) primary human fibroblasts. Cells were irradiated in the G1 phase of the cell cycle, with two doses with equivalent levels of apoptosis (low and high), defined for each cell line. In the three cell lines, the low doses of UVB caused only a transient delay in progression to the S phase, whereas the high doses induced permanent cell cycle arrest. However, while accumulation of Mdm2 correlated well with the recovery from transcription inhibition at the low doses for normal and CS-B fibroblasts, for XP-C cells this protein was shown to be accumulated even at UVB doses that induced high levels of apoptosis. Thus, UVB-induced accumulation of Mdm2 is critical for counteracting p53 activation and apoptosis avoidance, but its effect is limited due to transcription inhibition. However, in the case of XP-C cells, an excess of unrepaired DNA damage would be sufficient to block S phase progression, which would signal to apoptosis, independent of Mdm2 accumulation. The data clearly discriminate DNA damage signals that lead to cell death, depending on the presence of UVB-induced DNA damage in replicating or transcribing regions.

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This thesis wad aimed at the study and application of titanium dioxide photocatalytic activity on ceramic materials. As a matter of fact, photocatalysis is a very promising method to face most of the problems connected with the increasing environmental pollution. Furthermore, titanium dioxide, in its anatase crystallographic phase, is one of the most investigated photocatalytic material and results to be perfectly compatible with silicate body mixes. That goal was pursued by two different strategies: 1. the addition to a body mix used for heavy clay products of several titania powders, with different mean crystallite size, surface area, morphology and anatase/rutile ratio and a titania nanosuspension as well. The titania addition followed two procedures: bulk and spray addition over the ceramic samples surface. Titania was added in two different percentages: 2.5 and 7.5 wt.% in both of the methods. The ceramic samples were then fired at three maximum temperatures: 900, 950 and 1000 °C. Afterwards, the photocatalytic activity of the prepared ceramic samples was evaluated by following the degradation of an organic compound in aqueous medium, under UV radiation. The influence of titania morphological characteristics on the photoactivity of the fired materials was studied by means of XRD and SEM observations. The ceramic samples, sprayed with a slip containing 7.5 wt.% of titania powder and fired at 900 °C, have the best photoactivity, with a complete photo-decomposition of the organic compound. At 1000 °C no sample acted as a photocatalyst due to the anatase-to-rutile phase transformation and to the reaction between titania and calcium and iron oxides in the raw materials. 2. The second one foresaw the synthesis of TiO2-SiO2 solid solutions, using the following stoichiometry: Ti1-xSixO2 where x = 0, 0.1, 0.3 and 0.5 atoms per formula unit (apfu). The mixtures were then fired following two thermal cycles, each with three maximum temperatures. The effect of SiO2 addition into the TiO2 crystal structure and, consequently, on its photocatalytic activity when fired at high temperature, was thoroughly investigated by means of XRD, XPS, FE-SEM, TEM and BET analysis. The photoactivity of the prepared powders was assessed both in gas and liquid phase. Subsequently, the TiO2-SiO2 solid solutions, previously fired at 900 °C, were sprayed over the ceramic samples surface in the percentage of 7.5 wt.%. The prepared ceramic samples were fired at 900 and 1000 °C. The photocatalytic activity of the ceramic samples was evaluated in liquid phase. Unfortunately, that samples did not show any appreciable photoactivity. In fact, samples fired at 900 °C showed a pretty low photoactivity, while the one fired at 1000 °C showed no photoactivity at all. This was explained by the excessive coarsening of titania particles. To summarise, titania particle size, more than its crystalline phase, seems to have a relevant role in the photocatalytic activity of the ceramic samples.

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Gli argomenti trattati all’interno di questa tesi di dottorato riguardano la sintesi e la modifica di polimeri ottenuti a partire da fonti rinnovabili. L’acido polilattico (PLA) è stato modificato per ottenere film estensibili per uso alimentare. La scelta del materiale si è basata sull’analisi del suo ciclo di vita e perché è riconosciuto come sicuro per l’utilizzo nel campo alimentare. Le formulazioni testate, a base di PLA, sono state preparate con l’aggiunta di una serie di additivi utilizzati per migliorare le proprietà meccaniche del materiale. La lavorazione è stata eseguita mediante estrusione, ottenendo dei pellet a composizione omogenea successivamente lavorati nell’estrusore a bolla, modalità industriale di produzione dei film estensibili. È stata poi effettuata la sintesi diretta di nuovi poliesteri insaturi a base di dimetil succinato e 1,6-esandiolo. L’insaturazione della catena è stata ottenuta mediante l’uso, durante la sintesi, di derivati dell’olio di ricino, l’acido ricinoleico e il suo derivato insaturo metil undecenoato. Un’altra molecola insatura utilizzata è stata il citronellolo, scelto tra i terpeni. I polimeri così ottenuti sono stati modificati tramite reazioni radicaliche indotte con radiazioni UV utilizzando sostanze antibatteriche (sale 3-esadecil-1-vinilimidazolo bromuro) al fine di ottenere materiali con attività biocida a lungo termine e senza rilascio. Si è proceduto inoltre alla polimerizzazione reversibile di monomeri furanici con oli vegetali utilizzando una strategia di tipo double click. Si è partiti dalla sintesi di monomeri derivanti da oli vegetali contenenti eterocicli furanici attaccati mediante addizione tiol-enica (prima reazione click chemistry) e si è proseguito con la loro successiva polimerizzazione attraverso una reazione di tipo Diels-Alder con molecole con gruppi maleimmidici (seconda reazione click chemistry). I polimeri così ottenuti sono materiali potenzialmente auto-riparanti, grazie alla possibilità di spostare l’equilibrio verso i prodotti o i reagenti semplicemente variando le condizioni di temperatura.

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Ozon (O3) ist in der Atmosphäre ein wichtiges Oxidanz und Treibhausgas. Während die höchsten Konzentrationen in der Stratosphäre beobachtet werden und die vor der gefährlichen UV-Strahlung schützende Ozonschicht bilden, können sich signifikante Änderungen der Ozon-Konzentration in der Region der Tropopause auf das Klima der Erde auswirken. Des Weiteren ist Ozon eine der Hauptquellen für das Hydroxylradikal (OH) und nimmt damit entscheidend Einfluss auf die Oxidationskraft der Atmosphäre. Der konvektive Transport von Ozon und seinen Vorläufergasen aus Regionen nahe der Erdoberfläche in die freie Troposphäre beeinflusst das Budget dieser Spezies in der Tropopausenregion.rnDie Datengrundlage der Studie in der vorliegenden Arbeit basiert auf den flugzeuggetragenen Messkampagnen GABRIEL 2005 (Suriname, Südamerika) sowie HOOVER I 2006 und HOOVER II 2007 (beide in Europa). Mit dem zur Verfügung stehenden Datensatz wird das Ozonbudget in der freien, unbelasteten Hintergrundatmosphäre und in der durch hochreichende Konvektion gestörten, oberen Troposphäre untersucht. Anhand der auf in-situ Messungen von O3, NO, OH, HO2 und dem aktinischen Strahlungsfluss basierten Berechnung der Netto-Ozonproduktionsrate (NOPR) werden für das Messgebiet Ozontendenzen in der unbelasteten Troposphäre abgeleitet und mit Simulationen des globalen Chemie-Transport-Modells MATCH-MPIC verglichen. Mit Hilfe zweier Fallstudien in den Tropen in Südamerika und den mittleren Breiten in Europa werden die Auswirkungen von hochreichender Konvektion auf die obere Troposphäre quantifiziert.rnDie Ergebnisse zeigen für die Grenzschicht in niedrigen und mittleren Breiten eine eindeutige Tendenz zur Produktion von Ozon, was für den tropischen Regenwald in der Messregion nicht der allgemeinen Erwartung entsprach, nach der diese Region durch die Zerstörung von Ozon charakterisiert sein sollte. In der oberen Troposphäre ab etwa 7 km wird für die beiden Regionen eine leichte Tendenz zur Ozonproduktion beobachtet. Signifikante Unterschiede zeigen die Ergebnisse für die mittlere Troposphäre. Während die Tropen in dieser Region durch eine eindeutige Tendenz zur Zerstörung von Ozon charakterisiert sind, lässt sich über den mittleren Breiten zwar eine hohe photochemische Aktivität aber keine derart klare Tendenz feststellen. Die hohen Breiten zeichnen sich durch eine neutrale Troposphäre in Bezug auf die Ozontendenz aus und weisen kaum photochemische Aktivität auf. Der Vergleich dieser Ergebnisse mit dem MATCH-MPIC Modell zeigt in weiten Teilen der Messregionen eine grundlegende Übereinstimmung in der Tendenz zur Produktion oder Zerstörung von Ozon. Die absoluten Werte werden vom Modell aber generell unterschätzt. Signifikante Unterschiede zwischen in-situ Daten und Modellsimulationen werden in der Grenzschicht über dem tropischen Regenwald identifiziert.rnDer Einfluss der Konvektion ist durch eine signifikant erhöhte NOPR gekennzeichnet. In dieser Arbeit wird in den Tropen mit einem Median-Wert von 0.20 ppbv h−1 eine um den Faktor 3.6 erhöhte NOPR im Vergleich zur ungestörten oberen Troposphäre abgeschätzt. In den mittleren Breiten führt die um eine Größenordnung höhere NO-Konzentration zu einem Wert von 1.89 ppbv h−1, was einer Überhöhung um einen Faktor 6.5 im Vergleich zum ungestörten Zustand entspricht. Diese Ergebnisse zeigen für beide Regionen in der oberen Troposphäre eine erhöhte Ozonproduktion als Folge konvektiver Aktivität. rnrnHochreichende Konvektion ist zudem ein sehr effektiver Mechanismus für den Vertikaltransport aus der Grenzschicht in die obere Troposphäre. Die schnelle Hebung in konvektiven Wolken führt bei Spurengasen mit Quellen an der Erdoberfläche zu einer Erhöhung ihrer Konzentration in der oberen Troposphäre. Die hochgradig löslichen Spurenstoffe Formaldehyd (HCHO) und Wasserstoffperoxid (H2O2) sind wichtige Vorläufergase der HOx-Radikale. Es wird angenommen, dass sie aufgrund ihrer Löslichkeit in Gewitterwolken effektiv ausgewaschen werden.rnIn der vorliegenden Arbeit wird eine Fallstudie von hochreichender Konvektion im Rahmen des HOOVER II Projekts im Sommer 2007 analysiert. Am 19.07.2007 entwickelten sich am Nachmittag am Südostrand eines in nordöstlicher Richtung ziehenden mesoskaligen konvektiven Systems drei zunächst isolierte konvektive Zellen. Flugzeuggetragene Messungen in der Aus- und der Einströmregion einer dieser Gewitterzellen stellen einen exzellenten Datensatz bereit, um die Auswirkungen von hochreichender Konvektion auf die Verteilung verschiedener Spurengase in der oberen Troposphäre zu untersuchen. Der Vergleich der Konzentrationen von Kohlenstoffmonoxid (CO) und Methan (CH4) zwischen der oberen Troposphäre und der Grenzschicht deutet auf einen nahezu unverdünnten Transport dieser langlebigen Spezies in der konvektiven Zelle hin. Die Verhältnisse betragen (0.94±0.04) für CO und (0.99±0.01) für CH4. Für die löslichen Spezies HCHO und H2O2 beträgt dieses Verhältnis in der Ausströmregion (0.55±0.09) bzw. (0.61±0.08). Dies ist ein Indiz dafür, dass diese Spezies nicht so effektiv ausgewaschen werden wie angenommen. Zum besseren Verständnis des Einflusses der Konvektion auf die Budgets dieser Spezies in der oberen Troposphäre wurden im Rahmen dieser Arbeit Boxmodell-Studien für den Beitrag der photochemischen Produktion in der Ausströmregion durchgeführt, wobei die gemessenen Spezies und Photolysefrequenzen als Randbedingungen dienten. Aus den Budgetbetrachtungen für HCHO und H2O2 wird eine Auswascheffizienz von (67±24) % für HCHO und (41±18) % für H2O2 abgeschätzt. Das für H2O2 überraschende Ergebnis lässt darauf schließen, dass dieses Molekül in einer Gewitterwolke deutlich effektiver transportiert werden kann, als aufgrund seiner hohen Löslichkeit aus der Henry-Konstanten zu erwarten wäre. Das Ausgasen von gelöstem H2O2 beim Gefrieren eines Wolkentropfens, d.h. ein Retentionskoeffizient kleiner 1, ist ein möglicher Mechanismus, der zum beobachteten Mischungsverhältnis dieser löslichen Spezies in der Ausströmregion beitragen kann.

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Two phosphoramidite building blocks were synthesized that can easily be deprotected by UV light to reveal natural abasic sites in oligoribonucleotides as well as in oligodeoxyribonucleotides. Another building block which releases a 2 ′-O-methylated abasic site upon UV radiation is also described.

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OBJECTIVE: To explore the role of pro-apoptotic signals following tissue injury and how these may promote a progression of further cell death. METHODS: Laser treated porcine articular cartilage disks were maintained in culture media. The collected media at various time periods (3, 6, 9, 12, 24 and 48 h), was called treated conditioned media (TCM). Non-laser treated cartilage disks were used to create control conditioned media (CCM). Each disk was subsequently maintained for 28 days and used in confocal microscopic assessment to document the progression of the damaged area. Isolated porcine chondrocytes were cultured in monolayer, and were exposed to TCM, CCM or normal culture medium (NM). As a positive inducer of apoptosis, the monolayer cells were exposed to UV radiation for 10 min and cultured in NM. Following 24 h exposure, the cells were harvested and stained with the appropriate combination of fluorescent dyes and processed via flow cytometry. RESULTS: All cultured cells exposed to TCM displayed a caspase-3 positive subpopulation, a loss of CMXRos, and with a reduced or lost NO signal. CCM exposure signals were comparable to the NM treatments with all having retained CMXRos, NO and without evidence of caspase-3 activity. UV treatment also induced a reduction in NO, but both CMXRos and caspase-3 positive, representing an earlier stage of apoptosis and suggesting that the mode of cell death via UV and TCM exposure are via different processes. The investigation of a dose (100%, 50%, 25% and 12.5%) and time (0.5, 1, 3, 9, 12 h) response to TCM exhibited that all treatments observed an increase in caspase-3 positive cells and a reduction in NO and CMXRos. CONCLUSION: The usefulness of FCM can be used in the study of cell viability and apoptosis. Such a system may be useful in the study of mechanisms of disease such as osteoarthritis, thus may be of practical use for the pharmaceutical industry for screening associated drugs.

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Wood plastic composites (WPCs) have gained popularity as building materials because of their usefulness in replacing solid wood in a variety of applications. These composites are promoted as being low-maintenance, high-durability products. However, it has been shown that WPCs exposed to weathering may experience a color change and/or loss in mechanical properties. An important requirement for building materials used in outdoor applications is the retention of their aesthetic qualities and mechanical properties during service life. Therefore, it is critical to understand the photodegradation mechanisms of WPCs exposed to UV radiation and to develop approaches to stabilize these composites (both unstabilized and stabilized) as well as the effect of weathering on the color fade and the retention of mechanical properties were characterized. Since different methods of manufacturing WPCs lead to different surface characteristics, which can influence weathering, the effect of manufacturing method on the photodegradation of WPCs was investigated first. Wood flour (WF) filled high-density polyethylene (HDPE) composite samples were either injection molded, extruded, or extruded and then planed. Fourier transform infrared (FTIR) spectroscopy was used to monitor the surface chemistry of the manufactured composites. The spectra showed that the surface of planed samples had more wood component than extruded and injection molded samples, respectively. After weathering, the samples were analyzed for color fade, and loss of flexural properties. The final lightness of the composites was not dependent upon the manufacturing method. However the mechanical property loss was dependent upon manufacturing method. The samples with more wood component at the surface (planed samples) experienced a larger percentage of total loss in flexural properties after weathering due to a greater effect of moisture on the samples. The change in surface chemistry of HDPE and WF/HDPE composites after weathering was studied using spectroscopic techniques. X-ray photoelectron spectroscopy (XPS) was used to characterize the occurrence of surface oxidation whereas FTIR spectroscopy was used to monitor the development of degradation products, such as carbonyl groups and vinyl groups, and to determine changes in HDPE crystallinity. Surface oxidation occurred immediately after exposure for both the neat HDPE and WF/HDPE composites. After weathering, the surface of the WF/HDPE composites was oxidized to a greater extent than the neat HDPE after weathering. This suggests that photodegradation is exacerbated by the addition of the carbonyl functional groups of the wood fibers within the HDPE atrix during composite manufacturing. While neat HDPE may undergo cross-linking in the initial stages of accelerated weathering, the WF may physically hinder the ability of the HDPE to cross-link resulting in the potential for HDPE chain scission to dominate in the initial weathering stages of the WF/HDPE composites. To determine which photostabilizers are most effective for WF/HDPE composites, factorial experimental designes were used to determine the effects of adding two hindered amine light stabilizers, an ultraviolet absorber, and a pigment on the color made and mechanical properties of both unweathered and UV weathered samples. Both the pigment and ultraviolet absorber were more effective photostabilizers for WF/HDPE composites than hinder amine light stabilizers. The ineffectiveness of hindered amine light stabilizers in protecting WPCs against UV radiation was attribuated to the acid/base reactions occurring between the WF and hindered amine light stabilizer. The efficiency of an ultraviolet absorber and/or pigment was also examined by incorporating different concentration of an ultraviolet absorber and/or pigment into WF/HDPE composites. Color change and flexural properties were determined after accelerated UV weathering. The lightness of the composite after weathering was influenced by the concentration of both the ultraviolet absorber by masking the bleaching wood component as well as blocking UV light. Flexural MOE loss was influenced by an increase in ultraviolet absorber concentration, but increasing pigment concentration from 1 to 2% had little influence on MOE loss. However, increasing both ultraviolet absorber and pigment concentration resulted in improved strength properties over the unstabilized composites after 3000 h of weather. Finally, the change in surface chemistry due to weathering of WF/HDPE composites that were either unstabilized or stabilized with an ultraviolet absorber and/or pigment was analyzed using FTIR spectroscopy. The samples were tested for loss in modulus of elasticity, carbonyl and vinyl group formation at the surface, and change in HDPE crystallinity. It was concluded that structural changes in the samples; carbonyl group formation, terminal vinyl group formation, and crystallinity changes cannot reliably be used to predict changes in modulus of elasticity using a simple linear relationship. The effect of cross-linking, chain scission, and crystallinity changes due to ultraviolet exposure as well as the interfacial degradation due to moisture exposure are inter-related factors when weathering HDPE and WF/HDPE composites.

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We investigate the effects of a recently proposed 21st century Dalton minimum like decline of solar activity on the evolution of Earth's climate and ozone layer. Three sets of two member ensemble simulations, radiatively forced by a midlevel emission scenario (Intergovernmental Panel on Climate Change RCP4.5), are performed with the atmosphere-ocean chemistry-climate model AOCCM SOCOL3-MPIOM, one with constant solar activity, the other two with reduced solar activity and different strength of the solar irradiance forcing. A future grand solar minimum will reduce the global mean surface warming of 2 K between 1986–2005 and 2081–2100 by 0.2 to 0.3 K. Furthermore, the decrease in solar UV radiation leads to a significant delay of stratospheric ozone recovery by 10 years and longer. Therefore, the effects of a solar activity minimum, should it occur, may interfere with international efforts for the protection of global climate and the ozone layer.

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Previous studies have highlighted the severity of detrimental effects for life on earth after an assumed regionally limited nuclear war. These effects are caused by climatic, chemical and radiative changes persisting for up to one decade. However, so far only a very limited number of climate model simulations have been performed, giving rise to the question how realistic previous computations have been. This study uses the coupled chemistry climate model (CCM) SOCOL, which belongs to a different family of CCMs than previously used, to investigate the consequences of such a hypothetical nuclear conflict. In accordance with previous studies, the present work assumes a scenario of a nuclear conflict between India and Pakistan, each applying 50 warheads with an individual blasting power of 15 kt ("Hiroshima size") against the major population centers, resulting in the emission of tiny soot particles, which are generated in the firestorms expected in the aftermath of the detonations. Substantial uncertainties related to the calculation of likely soot emissions, particularly concerning assumptions of target fuel loading and targeting of weapons, have been addressed by simulating several scenarios, with soot emissions ranging from 1 to 12 Tg. Their high absorptivity with respect to solar radiation leads to a rapid self-lofting of the soot particles into the strato- and mesosphere within a few days after emission, where they remain for several years. Consequently, the model suggests earth's surface temperatures to drop by several degrees Celsius due to the shielding of solar irradiance by the soot, indicating a major global cooling. In addition, there is a substantial reduction of precipitation lasting 5 to 10 yr after the conflict, depending on the magnitude of the initial soot release. Extreme cold spells associated with an increase in sea ice formation are found during Northern Hemisphere winter, which expose the continental land masses of North America and Eurasia to a cooling of several degrees. In the stratosphere, the strong heating leads to an acceleration of catalytic ozone loss and, consequently, to enhancements of UV radiation at the ground. In contrast to surface temperature and precipitation changes, which show a linear dependence to the soot burden, there is a saturation effect with respect to stratospheric ozone chemistry. Soot emissions of 5 Tg lead to an ozone column reduction of almost 50% in northern high latitudes, while emitting 12 Tg only increases ozone loss by a further 10%. In summary, this study, though using a different chemistry climate model, corroborates the previous investigations with respect to the atmospheric impacts. In addition to these persistent effects, the present study draws attention to episodically cold phases, which would likely add to the severity of human harm worldwide. The best insurance against such a catastrophic development would be the delegitimization of nuclear weapons.

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Infectious keratoconjunctivitis (IKC) caused by Mycoplasma conjunctivae is a widespread ocular affection of free-ranging Caprinae in the Alpine arc. Along with host and pathogen characteristics, it has been hypothesized that environmental factors such as UV light are involved in the onset and course of the disease. This study aimed at evaluating the role of topographic features as predisposing or aggravating factors for IKC in Alpine chamois (Rupicapra rupicapra rupicapra) and Alpine ibex (Capra ibex ibex). Geospatial analysis was performed to assess the effect of aspect (northness) and elevation on the severity of the disease as well as on the mycoplasmal load in the eyes of affected animals, using data from 723 ibex and chamois (583 healthy animals, 105 IKC-affected animals, and 35 asymptomatic carriers of M. conjunctivae), all sampled in the Swiss Alps between 2008 and 2010. An influence of northness was not found, except that ibex with moderate and severe signs of IKC seem to prefer more north-oriented slopes than individuals without corneal lesions, possibly hinting at a sunlight sensitivity consequent to the disease. In contrast, results suggest that elevation influences the disease course in both ibex and chamois, which could be due to altitude-associated environmental conditions such as UV radiation, cold, and dryness. The results of this study support the hypothesis that environmental factors may play a role in the pathogenesis of IKC.

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Most skin cancers induced in mice by Ultraviolet (UV) radiation express highly immunogenic Tumor specific transplantation antigens (TSTAs) and thus exhibit a regressor phenotype. In this study, I have used cloned genes encoding tumor antigens and oncogenes in conjunction with DNA transfection technique to isolate and characterize regressor variants from progressor tumors and vice versa. The purpose of this study was (1) to determine whether the product of a cloned gene (216) from UV-1591 tumor, which encodes a novel MHC class I antigen can function as a tumor rejection antigen when expressed on unrelated, nonantigenic, murine tumor cells or whether its function is restricted to UV-induced tumors, and (2) to determine the processes by which progressor variants derived from a regressor UV-2240 cell line by transfection with an activated Ha-ras oncogene escape the immune defenses of the normal immunocompetent host.^ To answer the first question, a spontaneously transformed, nonimmunogenic cell line (10T-1) was cotransfected with DNA from p216 and pSV2-neo plasmids. Results demonstrate that the product of a cloned TSTA gene from a UV-induced murine tumor is capable of functioning as a tumor rejection antigen when expressed on unrelated, nonantigenic tumor cells. In addition, these results indicate that this approach could be used to augment the immune response against poorly antigenic tumors.^ To answer the second question, progressor variants were isolated from a highly antigenic UV radiation-induced C3H mouse regressor fibrosarcoma cell line, UV-2240, by transfection with an activated Ha-ras oncogene. Subcutaneous injection of Ha-ras-transfected UV-2240 cells into immunocompetent C3H mice produced tumors in 4 of 36 animals. In addition, the Ha-ras-induced progressor variants produced experimental lung metastasis in both normal C3H and nude mice, although they induced more lung nodules in nude mice than in normal C3H mice. Results indicate that the progressor phenotype of the Ha-ras-induced tumor variants is not due to loss of TSTAs or MHC class I antigens. This implies that some tumors can escape the immune defenses of the normal immunocompetent host by mechanisms other than the loss of TSTAs and MHC class I antigens. (Abstract shortened with permission of author.) ^

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Stable isotope ratios of nitrate preserved in deep ice cores are expected to provide unique and valuable information regarding paleoatmospheric processes. However, due to the post-depositional loss of nitrate in snow, this information may be erased or significantly modified by physical or photochemical processes before preservation in ice. We investigated the role of solar UV photolysis in the post-depositional modification of nitrate mass and stable isotoperatios at Dome C, Antarctica, during the austral summer of 2011/2012. Two 30 cm snow pits were filled with homogenized drifted snow from the vicinity of the base. One of these pits was covered with a plexiglass plate that transmits solar UV radiation, while the other was covered with a different plexiglass plate having a low UV transmittance. Samples were then collected from each pit at a 2–5 cm depth resolution and a 10-day frequency. At the end of the season, acomparable nitrate mass loss was observed in both pits for the top-level samples (0–7 cm) attributed to mixing with the surrounding snow. After excluding samples impacted by the mixing process, we derived an average apparent nitrogen isotopic fractionation (15" app/of role in driving the isotopic fractionation of nitrate in snow.We have estimated a purely photolytic nitrogen isotopic fractionation (15"photo) of -55.8 12.0 ‰ from the difference in the derived apparent isotopic ractionations of the two experimental fields, as both pits were exposed to similar physical processes except exposure to solar UV. This value is in close agreement with the 15" photo value of -47.9 6.8 ‰ derived in a laboratory experiment simulated for Dome C conditions (Berhanu et al., 2014). We have also observed an insensitivity of 15" with depth in the snowpack under the given experimental setup. This is due to the uniform attenuation of incoming solar UV by snow, as 15" is strongly dependent on the spectral distribution of the incoming light flux. Together with earlier work, the results presented here represent a strong body of evidence that solar UV photolysis is the most relevant post-depositional process modifying the stable isotope ratios of snow nitrate at low-accumulation sites, where many deep ice cores are drilled. Nevertheless, modeling the loss of nitrate in snow is still required before a robust interpretation of ice core records can be provided.

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Stratospheric ozone is of major interest as it absorbs most harmful UV radiation from the sun, allowing life on Earth. Ground-based microwave remote sensing is the only method that allows for the measurement of ozone profiles up to the mesopause, over 24 hours and under different weather conditions with high time resolution. In this paper a novel ground-based microwave radiometer is presented. It is called GROMOS-C (GRound based Ozone MOnitoring System for Campaigns), and it has been designed to measure the vertical profile of ozone distribution in the middle atmosphere by observing ozone emission spectra at a frequency of 110.836 GHz. The instrument is designed in a compact way which makes it transportable and suitable for outdoor use in campaigns, an advantageous feature that is lacking in present day ozone radiometers. It is operated through remote control. GROMOS-C is a total power radiometer which uses a pre-amplified heterodyne receiver, and a digital fast Fourier transform spectrometer for the spectral analysis. Among its main new features, the incorporation of different calibration loads stands out; this includes a noise diode and a new type of blackbody target specifically designed for this instrument, based on Peltier elements. The calibration scheme does not depend on the use of liquid nitrogen; therefore GROMOS-C can be operated at remote places with no maintenance requirements. In addition, the instrument can be switched in frequency to observe the CO line at 115 GHz. A description of the main characteristics of GROMOS-C is included in this paper, as well as the results of a first campaign at the High Altitude Research Station at Jungfraujoch (HFSJ), Switzerland. The validation is performed by comparison of the retrieved profiles against equivalent profiles from MLS (Microwave Limb Sounding) satellite data, ECMWF (European Centre for Medium-Range Weather Forecast) model data, as well as our nearby NDACC (Network for the Detection of Atmospheric Composition Change) ozone radiometer measuring at Bern.