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La mesura de la irradiància solar en superfície es fa mitjançant piranòmetres amb sensor termoelèctric o amb sensor de silici. Aquests darrers presenten una resposta espectral no uniforme i limitada a la banda de 400 a 1100 nm, i, a més, la seva sensibilitat depèn fortament de la temperatura. Els piranòmetres termoelèctrics, en canvi, presenten una resposta espectral uniforme en la banda solar, i un coeficient de temperatura reduït. L’objectiu de l’estudi que es presenta ha estat millorar l’acord entre les mesures d’irradiància global preses amb un piranòmetre termoelèctric CM11 de Kipp & Zonen, i diversos piranòmetres fotovoltaics o de silici Li200SA de Li-Cor. Com que la resposta angular dels sensors s’aparta en general de la resposta cosinus ideal, es proposen unes correccions a tal efecte. S’han analitzat les dades minutals corresponents a un cicle anual de mesures d’irradiància preses pels dos tipus de piranòmetres a l’estació radiomètrica de la Universitat de Girona. Les correccions proposades per la resposta angular dels instruments es basen en bibliografia prèvia, i també en simulacions realitzades amb un model espectral de transferència radiativa multicapa. La simulació ha permès obtenir correccions per compensar les diferents respostes angulars i espectrals dels dos tipus d’instruments. Per a cels serens, les correccions angulars i espectrals milloren notablement l’acord entre les mesures dels dos tipus de piranòmetres. També es proposa una correcció de l’efecte de la temperatura sobre la mesura dels piranòmetres de silici, obtinguda empíricament. Malgrat que les correccions s’han obtingut per a cels serens, han estat també aplicades a condicions de cel ennuvolat, caracteritzades objectivament mitjançant un algorisme basat en mesures d’irradiància global i difusa. Finalment s’ha comprovat que les correccions també milloren l’acord entre les mesures dels dos tipus de sensors independentment de l’extensió de la coberta de núvols

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The interest in solar ultraviolet (UV) radiation from the scientific community and the general population has risen significantly in recent years because of the link between increased UV levels at the Earth's surface and depletion of ozone in the stratosphere. As a consequence of recent research, UV radiation climatologies have been developed, and effects of some atmospheric constituents (such as ozone or aerosols) have been studied broadly. Correspondingly, there are well-established relationships between, for example, total ozone column and UV radiation levels at the Earth's surface. Effects of clouds, however, are not so well described, given the intrinsic difficulties in properly describing cloud characteristics. Nevertheless, the effect of clouds cannot be neglected, and the variability that clouds induce on UV radiation is particularly significant when short timescales are involved. In this review we show, summarize, and compare several works that deal with the effect of clouds on UV radiation. Specifically, works reviewed here approach the issue from the empirical point of view: Some relationship between measured UV radiation in cloudy conditions and cloud-related information is given in each work. Basically, there are two groups of methods: techniques that are based on observations of cloudiness (either from human observers or by using devices such as sky cameras) and techniques that use measurements of broadband solar radiation as a surrogate for cloud observations. Some techniques combine both types of information. Comparison of results from different works is addressed through using the cloud modification factor (CMF) defined as the ratio between measured UV radiation in a cloudy sky and calculated radiation for a cloudless sky. Typical CMF values for overcast skies range from 0.3 to 0.7, depending both on cloud type and characteristics. Despite this large dispersion of values corresponding to the same cloud cover, it is clear that the cloud effect on UV radiation is 15–45% lower than the cloud effect on total solar radiation. The cloud effect is usually a reducing effect, but a significant number of works report an enhancement effect (that is increased UV radiation levels at the surface) due to the presence of clouds. The review concludes with some recommendations for future studies aimed to further analyze the cloud effects on UV radiation

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Solos de Referência compõem um conjunto de classes de solos representativo de determinada região. O conhecimento de características desses solos pode ser utilizado na solução de problemas de manejo em solos similares. O objetivo deste trabalho foi quantificar os teores disponíveis por diferentes extratores e as frações de Mn e Fe nos Solos de Referência de Pernambuco, visando avaliar a capacidade destes solos em suprir esses elementos para as plantas, bem como a relação entre diversos extratores do "disponível" e as formas dos micronutrientes nos solos. Os teores dos micronutrientes foram determinados com os extratores Mehlich-1, Mehlich-3, DTPA e EDTA nas amostras dos dois primeiros horizontes dos solos. As amostras foram também extraídas, seqüencialmente, para separar os elementos nas frações: trocável, matéria orgânica, óxido de ferro amorfo e óxido de ferro cristalino. De acordo com os resultados, a fração trocável e a matéria orgânica foram as principais responsáveis pela retenção e disponibilidade de Mn nos solos estudados. Quanto ao Fe, a fração matéria orgânica foi responsável pelos teores disponíveis, considerando os teores muito baixos na forma trocável. Os teores disponíveis de Mn e Fe na maioria dos Solos de Referência de Pernambuco foram considerados de médio a alto, com pouco potencial para deficiências a curto e médio prazo. Os extratores Mehlich-1 e DTPA apresentaram as melhores correlações com as formas mais biodisponíveis de Mn e Fe e foram considerados adequados para avaliação da disponibilidade desses elementos nos solos do Estado.

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OBJECTIVE To identify metabolic pathways that may underlie susceptibility or resistance to high-fat diet-induced hepatic steatosis. RESEARCH DESIGN AND METHODS We performed comparative transcriptomic analysis of the livers of A/J and C57Bl/6 mice, which are, respectively, resistant and susceptible to high-fat diet-induced hepatosteatosis and obesity. Mice from both strains were fed a normal chow or a high-fat diet for 2, 10, and 30 days, and transcriptomic data were analyzed by time-dependent gene set enrichment analysis. Biochemical analysis of mitochondrial respiration was performed to confirm the transcriptomic analysis. RESULTS Time-dependent gene set enrichment analysis revealed a rapid, transient, and coordinate upregulation of 13 oxidative phosphorylation genes after initiation of high-fat diet feeding in the A/J, but not in the C57Bl/6, mouse livers. Biochemical analysis using liver mitochondria from both strains of mice confirmed a rapid increase by high-fat diet feeding of the respiration rate in A/J but not C57Bl/6 mice. Importantly, ATP production was the same in both types of mitochondria, indicating increased uncoupling of the A/J mitochondria. CONCLUSIONS Together with previous data showing increased expression of mitochondrial β-oxidation genes in C57Bl/6 but not A/J mouse livers, our present study suggests that an important aspect of the adaptation of livers to high-fat diet feeding is to increase the activity of the oxidative phosphorylation chain and its uncoupling to dissipate the excess of incoming metabolic energy and to reduce the production of reactive oxygen species. The flexibility in oxidative phosphorylation activity may thus participate in the protection of A/J mouse livers against the initial damages induced by high-fat diet feeding that may lead to hepatosteatosis.