Solar ultraviolet-B radiation and vitamin D: a cross-sectional population-based study using data from the 2007 to 2009 Canadian Health Measures Survey

Background: Exposure to solar ultraviolet-B (UV-B) radiation is a major source of vitamin D3. Chemistry climate models project decreases in ground-level solar erythemal UV over the current century. It is unclear what impact this will have on vitamin D status at the population level. The purpose of this study was to measure the association between ground-level solar UV-B and serum concentrations of 25-hydroxyvitamin D (25(OH)D) using a secondary analysis of the 2007 to 2009 Canadian Health Measures Survey (CHMS). Methods: Blood samples collected from individuals aged 12 to 79 years sampled across Canada were analyzed for 25(OH)D (n=4,398). Solar UV-B irradiance was calculated for the 15 CHMS collection sites using the Tropospheric Ultraviolet and Visible Radiation Model. Multivariable linear regression was used to evaluate the association between 25(OH)D and solar UV-B adjusted for other predictors and to explore effect modification. Results: Cumulative solar UV-B irradiance averaged over 91 days (91-day UV-B) prior to blood draw correlated significantly with 25(OH)D. Independent of other predictors, a 1 kJ/m 2 increase in 91-day UV-B was associated with a significant 0.5 nmol/L (95% CI 0.3-0.8) increase in mean 25(OH)D (P =0.0001). The relationship was stronger among younger individuals and those spending more time outdoors. Based on current projections of decreases in ground-level solar UV-B, we predict less than a 1 nmol/L decrease in mean 25(OH)D for the population. Conclusions: In Canada, cumulative exposure to ambient solar UV-B has a small but significant association with 25(OH)D concentrations. Public health messages to improve vitamin D status should target safe sun exposure with sunscreen use, and also enhanced dietary and supplemental intake and maintenance of a healthy body weight.

Growth and physiological responses of sunflower plants exposed to ultraviolet-B radiation

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Effects of UV-B radiation on Lecanicillium spp., biological control agents of the coffee leaf rust pathogen

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Effects of UV-B radiation on the antagonistic ability of Clonostachys rosea to Botrytis cinerea on strawberry leaf disc

Human activities are altering the concentrations of ozone in the troposphere and hence in the incidence of ultraviolet-B (UV-B) on Earth’s surface. Although representing only five percent of UV-B radiation striking the Earth's surface, this radiation has the potential to cause effects on biologically active molecules. Sensitivity to UV-B radiation is one of the limitations of biological control of plant pathogens in the field. The objectives of this work were to evaluate the effects of UV-B on several isolates of Clonostachys rosea, and the ability of an isolate of C. rosea, previously selected for its tolerant to UV-B radiation, to control Botrytis cinerea on strawberry leaves in controlled conditions (strawberry leaf discs). The germination of C. rosea conidia was inversely proportional to the irradiance. The most tolerant strain (LQC62) had relative germination of about 60% after irradiation of 4.2kJ/m2, and this strain was selected to be used in the subsequent studies. The data showed that even with exposure to UV-B radiation, C. rosea LQC62 controlled the pathogen. Conidial concentrations of strain LQC62 above 105 conidia/ml showed higher tolerance to UV-B radiation and increased ability to control more than 75% of the B. cinerea even with exposure to radiation. According to our results, in addition to showing less growth under UV-B, conidia of C. rosea had lower antagonistic ability. Further studies are needed to observe the tolerance of B. cinerea conidia to UV-B radiation and thereby prove that an environment with increased UV-B radiation may be favoring the pathogen due to a lower ability of C. rosea to control the pathogen in conditions of increased UV-B.

Ambient UV-B radiation causes deformities in amphibian embryos

There has been a great deal of recent attention on the suspected increase in amphibian deformities. However, most reports of amphibian deformities have been anecdotal, and no experiments in the field under natural conditions have been performed to investigate this phenomenon. Under laboratory conditions, a variety of agents can induce deformities in amphibians. We investigated one of these agents, UV-B radiation, in field experiments, as a cause for amphibian deformities. We monitored hatching success and development in long-toed salamanders under UV-B shields and in regimes that allowed UV-B radiation. Embryos under UV-B shields had a significantly higher hatching rate and fewer deformities, and developed more quickly than those exposed to UV-B. Deformities may contribute directly to embryo mortality, and they may affect an individual’s subsequent survival after hatching.

Synergism between UV-B radiation and a pathogen magnifies amphibian embryo mortality in nature.

Previous research has shown that amphibians have differential sensitivity to ultraviolet-B (UV-B) radiation. In some species, ambient levels of UV-B radiation cause embryonic mortality in nature. The detrimental effects of UV-B alone or with other agents may ultimately affect amphibians at the population level. Here, we experimentally demonstrate a synergistic effect between UV-B radiation and a pathogenic fungus in the field that increases the mortality of amphibian embryos compared with either factor alone. Studies investigating single factors for causes of amphibian egg mortality or population declines may not reveal the complex factors involved in declines.

Sensitivity of yellow passion fruit to ultraviolet-B radiation

The objective of this work was to evaluate the effects of UV-B radiation on the vegetative growth and on the gas exchange characteristics of passion fruit plants (Passiflora edulis) grown in greenhouse. The average unweighted UV-B radiation near the apex of the plants was 8 W m-2 for the UV-B treatment (high UV-B), and 0.8 W m-2 for the control plants (low UV-B). Plants were irradiated with UV-B for 7 hours per day, centered on solar noon, during 16 days. High UV-B radiation resulted in lower shoot dry matter accumulation per plant. The content of UV-B absorbing compounds and anthocyanins was increased in the plants exposed to high UV-B radiation, when compared with the control. UV-B radiation did not affect stomatal conductance or transpiration rate, but reduced photosynthesis and instantaneous water-use efficiency, and increased intercellular CO2 concentration. The accumulation of UV-B-absorbing compounds and anthocyanins did not effectively shield plants from supplementary UV-B radiation, since the growth and photosynthetic processes were significantly reduced.

Quantification of UV-B flux through time using UV-B-absorbing compounds contained in fossil Pinus sporopollenin

• UV-B radiation currently represents c. 1.5% of incoming solar radiation. However, significant changes are known to have occurred in the amount of incoming radiation both on recent and on geological timescales. Until now it has not been possible to reconstruct a detailed measure of UV-B radiation beyond c. 150 yr ago. • Here, we studied the suitability of fossil Pinus spp. pollen to record variations in UV-B flux through time. In view of the large size of the grain and its long fossil history, we hypothesized that this grain could provide a good proxy for recording past variations in UV-B flux. • Two key objectives were addressed: to determine whether there was, similar to other studied species, a clear relationship between UV-B-absorbing compounds in the sporopollenin of extant pollen and the magnitude of UV-B radiation to which it had been exposed; and to determine whether these compounds could be extracted from a small enough sample size of fossil pollen to make reconstruction of a continuous record through time a realistic prospect. • Preliminary results indicate the excellent potential of this species for providing a quantitative record of UV-B through time. Using this technique, we present the first record of UV-B flux during the last 9500 yr from a site near Bergen, Norway.

Efeito da radiação UV -B na interação Botrytis cinerea – clonostachys rosea em morangueiro e do ácido 4 - aminobenzóico no controle do patógeno em tabaco

Pós-graduação em Agronomia (Proteção de Plantas) - FCA

Sensitivity of yellow passion fruit plants to ultraviolet-B radiation

The objective of this work was to evaluate the effects of UV-B radiation on the vegetative growth and on the gas exchange characteristics of passion fruit plants (Passiflora edulis) grown in greenhouse. The average unweighted UV-B radiation near the apex of the plants was 8 W m-2 for the UV-B treatment (high UV-B), and 0.8 W m-2 for the control plants (low UV-B). Plants were irradiated with UV-B for 7 hours per day, centered on solar noon, during 16 days. High UV-B radiation resulted in lower shoot dry matter accumulation per plant. The content of UV-B absorbing compounds and anthocyanins was increased in the plants exposed to high UV-B radiation, when compared with the control. UV-B radiation did not affect stomatal conductance or transpiration rate, but reduced photosynthesis and instantaneous water‑use efficiency, and increased intercellular CO2 concentration. The accumulation of UV-B-absorbing compounds and anthocyanins did not effectively shield plants from supplementary UV-B radiation, since the growth and photosynthetic processes were significantly reduced.

Medición y predicción de la radiación solar global UV-B bajo cielos claros y sin nubes

Se presentan mediciones experimentales de la radiación solar ultravioleta en el rango B del espectro solar (UV-B) y la radiación ultravioleta en el rango total RUV (UV-A+UV-B) en días claros y sin nubes en Heredia, Costa Rica. Se utilizó una radiómetro UV-B, que mide la radiación solar en el rango espectral 280-315 nm, y un radiómetro RUV, que mide la radiación solar en el rango espectral 280-385 nm. La dependencia entre entre UV-B y RUV también fue investigada, y se encontró un excelente grado de asociación entre ambas. Además se detalló que UV-B representa solamente un 5,4% de RUV, a pesar de que UV-B es mil veces más potente que UV-A. Los valores de UV-B medidos in situ fueron comparados con los valores predichos por un modelo atmosférico espectral, el cual utiliza como datos de entrada: la hora del día, la latitud, la altitud, el albedo superficial, la distancia Tierra-Sol, la turbiedad atmosférica y el ozono atmosférico. La comparación entre los valores medidos y predichos dio resultados satisfactorios.

Regulation of the expression of NADP-malic enzyme by UV-B, red and far-red light in maize seedlings

The induction of nicotinamide adenine dinucleotide phosphate-malic enzyme (NADP-ME) in etiolated maize (Zea mays) seedlings by UV-B and UV-A radiation, and different levels of photosynthetically active radiation (PAR, 400-700 nm) was investigated by measuring changes in activity, protein quantity and RNA levels as a function of intensity and duration of exposure to the different radiations. Under low levels of PAR, exposure to UV-B radiation but not UV-A radiation for 6 to 24 h caused a marked increase in the enzyme levels similar to that observed under high PAR in the absence of UV-B. UV-B treatment of green leaves following a 12-h dark period also caused an increase in NADP-ME expression. Exposure to UV-B radiation for only 5 min resulted in a rapid increase of the enzyme, followed by a more gradual rise with longer exposure up to 6 h. Low levels of red light for 5 min or 6 h were also effective in inducing NADP-ME activity equivalent to that obtained with UV-B radiation. A 5-min exposure to far-red light following UV-B or red light treatment reversed the induction of NADP-ME, and this effect could be eliminated by further treatment with UV-B or red light. These results indicate that physiological levels of UV-B radiation can have a positive effect on the induction of this photosynthetic enzyme. The reducing power and pyruvate generated by the activity of NADP-ME may be used for respiration, in cellular repair processes and as substrates for fatty acid synthesis required for membrane repair.

GM-CSF (granulocyte-macrophage colony-stimulating factor): Modulation der durch UV-B-Strahlung induzierten Hautkarzinogenese

UV-B-Strahlung, die durch die fortschreitende Zerstörung der Ozonschicht zunimmt, ist hauptsächlich für das Entstehen von Basaliomen und Plattenepithelkarzinomen verantwort-lich, an denen jedes Jahr etwa 2-3 Millionen Menschen weltweit erkranken. UV-B indu-zierte Hautkarzinogenese ist ein komplexer Prozess, bei dem vor allem die mutagenen und immunsuppressiven Wirkungen der UV-B-Strahlung von Bedeutung sind. Die Rolle von GM-CSF in der Hautkarzinogenese ist dabei widersprüchlich. Aus diesem Grund wurde die Funktion von GM-CSF in vivo in der UV-B induzierten Hautkarzinogenese mittels zwei bereits etablierter Mauslinien untersucht: Erstens transgene Mäuse, die einen GM-CSF Antagonisten unter der Kontrolle des Keratin-10-Promotors in den suprabasalen Schichten der Epidermis exprimieren und zweitens solche, die unter dem Keratin-5-Promotor murines GM-CSF in der Basalschicht der Epidermis überexprimieren. Eine Gruppe von Tieren wurde chronisch, die andere akut bestrahlt. Die konstitutionelle Verfassung der Tiere mit erhöhter GM-CSF-Aktivität in der Haut war nach chronischer UV-B-Bestrahlung insgesamt sehr schlecht. Sie wiesen deshalb eine stark erhöhte Mortali-tät auf. Dies ist sowohl auf die hohe Inzidenz als auch dem frühen Auftreten der benignen und malignen Läsionen zurückzuführen. Eine verminderte GM-CSF Aktivität verzögerte dagegen die Karzinomentwicklung und erhöhte die Überlebensrate leicht. GM-CSF wirkt auf verschiedenen Ebenen tumorpromovierend: Erstens erhöht eine gesteigerte Mastzell-anzahl in der Haut der GM-CSF überexprimierenden Tiere per se die Suszeptibilität für Hautkarzinogenese. Zweitens stimuliert GM-CSF die Keratinozytenproliferation. Dadurch kommt es nach UV-B-Bestrahlung zu einer prolongierten epidermalen Hyperproliferation, die zur endogenen Tumorpromotion beiträgt, indem sie die Bildung von Neoplasien unter-stützt. Der Antagonist verzögert dagegen den Proliferationsbeginn, die Keratinozyten blei-ben demzufolge länger in der G1-Phase und der durch UV-B verursachte DNA-Schaden kann effizienter repariert werden. Drittens kann GM-CSF die LCs nicht als APCs aktivie-ren und eine Antitumorimmunität induzieren, da UV-B-Strahlung zur Apoptose von LCs bzw. zu deren Migration in Richtung Lymphknoten führt. Zusätzlich entwickeln GM-CSF überexprimierende Tiere in ihrer Haut nach UV-B-Bestrahlung ein Millieu von antago-nistisch wirkenden Zytokinen, wie TNF-a, TGF-b1 und IL-12p40 und GM-CSF, die proinflammatorische Prozesse und somit die Karzinomentwicklung begünstigen. Der Anta-gonist hemmt nach UV-B-Bestrahlung die Ausschüttung sowohl von immunsuppressiven Zytokinen, wie etwa TNF-a, als auch solchen, die die Th2-Entwicklung unterstützen, wie etwa IL-10 und IL-4. Dies wirkt sich negativ auf die Karzinomentwicklung aus.

Respuesta de Vitis vinífera L. cv. Malbec a UV-B y ABA

Malbec es la variedad de uva tinta más importante en la vitivinicultura argentina, especialmente en Mendoza, donde se produce más del 80% del total nacional. Las zonas ubicadas a mayor altitud están experimentando un aumento en la superficie cultivada, ya que en ellas se producen uvas con altos contenidos de compuestos fenólicos, responsables de muchas de las características deseadas en los vinos tintos, por su valor organoléptico y capacidad antioxidante. A partir de estos antecedentes, se plantea como objetivo caracterizar la radiación UV-B que reciben los viñedos ubicados a mayor altitud en Mendoza, estudiando los efectos de UV-B, las aplicaciones de ABA y de su interacción, sobre aspectos fisiológicos y bioquímicos que afectan el crecimiento de las bayas (rendimiento cuantitativo) y la calidad enológica de Vitis vinifera L. cv. Malbec.