The effect of leaf-lobing on the interception of direct solar radiation

Summary The extent to which leaf-lobing influences the interception of direct solar radiation by individual plants was studied by means of computer simulations. The morphology, size and orientation ofAmbrosia artemisiifolia L. leaves were measured and used to construct a prototypeAmbrosia plant upon which a computer simulation was based. The leaf geometries of this simulation were then varied, and daily integrated irradiances (DII) were calculated for each variant plant simulation. Data indicate that lobedAmbrosia leaves do not confer an advantage to light-interception based upon values of DII. Simulated plants identical in all respects to the prototype, but with simple, elliptic leaves, had equivalent DII values to the prototype. Simulations with leaves in which gaps between lobes were filledin had reduced light-interception efficiencies compared to the prototype and to a simulation with elliptic-leaves. Lightinterception was maximized when leaves on distal nodes wereAmbrosia-like and leaves on proximal nodes were elliptic. The data are interpreted to indicate that lobingperse is not functionally advantageous to light-interception; however, gradients of leaf-lobing along the length of shoots may be very significant in terms of overall light interception.     

The induction of DNA strand breaks in normal human skin fibroblasts exposed to solar ultraviolet radiation

The levels of apparent DNA single-strand breaks (ssb) were measured, following a 0-20 h incubation of normal human skin fibroblasts exposed to the solar uv wavelengths produced by a fluorescent sunlamp. The ssb were determined using the alkaline elution assay, which was performed either without proteinase K (proK) or in its presence, so as to eliminate any DNA-protein crosslinks that may be present in the cells. Cells were irradiated with either 3 kJ/m2 of sunlamp uv greater than 295 nm, 150 kJ/m2 of sunlamp uv greater than 315 nm, or 150 kJ/m2 of sunlamp uv greater than 320 nm. These treatments resulted in the production of 5-10 ssb/10(10) Da. For the two shorter wavelength irradiations, the levels of ssb decreased rapidly upon incubation of the cells. However, when the elutions were performed using proK, the number of ssb increased about twofold following a 2-4 h incubation. In contrast, the levels of ssb decreased in the sunlamp uv greater than 320 nm irradiated cells for elutions performed with or without proK. These results suggest that under certain irradiation conditions, ssb are formed in cells upon incubation, which are hidden by the crosslinking of protein to DNA.     

Human projected area factors for detailed direct and diffuse solar radiation analysis

Projected area factors for individual segments of the standing and sedentary human body were modelled for both direct and diffuse solar radiation using detailed 3D geometry and radiation models. The local projected area factors with respect to direct short-wave radiation are a function of the solar azimuth angle () between 0°<<360° and the solar altitude () angles between –90°<<+90°. In case of diffuse solar radiation from the isotropic sky the local human projected area factors were modelled as a function of the ground albedo () ranging between 0<<1. The model was validated against available experimental data and showed good general agreement with projected area factors measured for both the human body as a whole and for local quantities. Scientists can use the equations to predict the inhomogeneous irradiation and absorption of direct and diffuse solar radiation and UV-radiation at surfaces of the human body. In conjunction with detailed multi-node models of human thermoregulation the equations can be used to predict the physiological implications of solar radiation and outdoor weather conditions on humans.     

Resistance of marine bacterioneuston to solar radiation

A total of 90 bacterial strains were isolated from the sea surface microlayer (i.e., bacterioneuston) and underlying waters (i.e., bacterioplankton) from two sites of the northwestern Mediterranean Sea. The strains were identified by sequence analysis, and growth recovery was investigated after exposure to simulated solar radiation. Bacterioneuston and bacterioplankton isolates were subjected to six different exposure times, ranging from 0.5 to 7 h of simulated noontime solar radiation. Following exposure, the growth of each isolate was monitored, and different classes of resistance were determined according to the growth pattern. Large interspecific differences among the 90 marine isolates were observed. Medium and highly resistant strains accounted for 41% and 22% of the isolates, respectively, and only 16% were sensitive strains. Resistance to solar radiation was equally distributed within the bacterioneuston and bacterioplankton. Relative contributions to the highly resistant class were 43% for gamma-proteobacteria and 14% and 8% for alpha-proteobacteria and the Cytophaga/Flavobacterium/Bacteroides (CFB) group, respectively. Within the gamma-proteobacteria, the Pseudoalteromonas and Alteromonas genera appeared to be highly resistant to solar radiation. The majority of the CFB group (76%) had medium resistance. Our study further provides evidence that pigmented bacteria are not more resistant to solar radiation than nonpigmented bacteria.     

A direct assay for detection of chemically induced changes in the rejoining kinetics of radiation induced DNA strand breaks

A simple and sensitive procedure for testing various chemicals affecting DNA repair is presented. Cells, either labelled with [3H]thymidine or [14C]thymidine, were drug-treated or used as references cells. Both cell populations were irradiated with 5 Gy. The number of DNA breaks were determined, after mixing of drug-treated and reference cells of different labelling, at various intervals by the DNA unwinding technique and the drug-dependent DNA breaks were calculated. The drugs benzamide, 3-aminobenzamide, novobiocin and 9-beta-D-arabinofuranosyladenine (araA), all known to affect DNA repair, were used to study their effect on the number of DNA strand breaks with the presented technique. It was found that the assay improved the accuracy in determining the influence of DNA repair inhibitors compared to indirect measurements.     

Potential solar radiation on plant shapes

The thesis is presented that most plant-shapes, especially trees, resemble a combination of geometrical shapes which present their non-opaque bodies to incoming radiation, which is partially absorbed by the foliage. Such a hypothesis makes possible the quantification of the budget of energy of the entire plant. This first report presents only the findings in regard to the receipt of direct and diffuse solar radiation from the sky (clear conditions), before reflection and absorption, on a variety of geometries which simulate common plant-shapes. An all-year simulation of potential insolation for such shapes was conducted for latitudes 0° to 90°. Each shape, latitude and each season exhibited its own characteristic patterns of the various energy cycles. Derived data differed materially from data applicable to horizontal surfaces. The simulated plant-shapes tended to avoid receipt of energy in the low latitudes, whereas the opposite occurred toward higher latitudes.

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Zusammenfassung Die meisten Pflanzenumrisse, speziell Bäume, ähneln einer Kombination geometrischer Formen. Die Bäume sind nicht-undurchsichtige Körper für einkommende Strahlung, die durch die Blätter teilweise absorbiert wird. Nach der Hypothese ist es möglich, den Energiehaushalt für die gesamte Pflanze zu quantifizieren. Dieser erste Bericht befasst sich nur mit den Ergebnissen der direkten und diffusen Sonnenstrahlung vom Himmel bei klaren Bedingungen vor Reflexion und Absorption bei einer Anzahl simulierter geometrischer Formen, die auf allgemeinen Pflanzenumrissen basieren. Eine ganzjährige Simulation der potentiellen Besonnung dieser Formen wurde für alle Breiten von 0° bis 90° berechnet. Jede Form, Breite und Jahreszeit zeigt ihre eigenen charakteristischen Verläufe der verschiedenen Energiezyklen. Die abgeleiteten Werte unterscheiden sich von den Werten, die auf horizontale Oberflächen anwendbar sind. Die simulierten Pflanzenkörper neigten zur Vermeidung von Energieaufnahme in niedrigen Breiten, während bei höheren Breiten das Umgekehrte auftrat.

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Resume Les formes extérieures des plantes et plus spécialement celles des arbres peuvent se ramener à des combinaisons de formes géométriques. Les arbres ne constituent pas des corps opaques pour le rayonnement, mais celuici n'est que partiellement absorbé par la couronne. Selon l'hypothèse présentée ici, il est possible de déterminer quantitativement le bilan énergétique de la plante entière. Ce premier mémoire se restreint à l'étude de l'absorption du rayonnement direct et diffus, c'est-à-dire du soleil et d'un ciel serein. Ces résultats sont calculés avant toute réflexion ou absorption par d'autres corps et se rapportent à un certain nombre de formes géométriques simulant des profils typiques d'arbres. On a ainsi calculé le gain énergétique de ces formes pour toute l'année et pour toutes les latitudes de 0° à 90°. Chaque profil, chaque latitude et chaque saison présente des caractéristiques propres quant à l'évolution des différents cycles d'énergie. Les valeurs ainsi obtenues se distinguent nettement de valeurs correspondantes se rapportant à des surfaces horizontales. Les profils de plantes examinés tendent à absorber aussi peu d'énergie que possible dans les basses latitudes, alors que c'est le contraire qui se produit au voisinage des pôles.

     

Mammalian genes preferentially co-retained in radiation hybrid panels tend to avoid coexpression

Coexpression has been frequently used to explore modules of functionally related genes in eukaryotic genomes. However, we found that genetically interacting mammalian genes identified through radiation hybrid (RH) genotypes tend not to be coexpressed across tissues. This pattern remained unchanged after controlling for potential confounding factors, including chromosomal linkage, chromosomal distance, and gene duplication. Because >99.9% of the genetically interacting genes were identified according to the higher co-retention frequencies, our observation implies that coexpression is not necessarily an indication of the need for the co-presence of two genes in the genome, which is a prerequisite for cofunctionality of their coding proteins in the cell. Therefore, coexpression information must be applied cautiously to the exploration of the functional relatedness of genes in a genome.     

From sunlight to phytomass: on the potential efficiency of converting solar radiation to phyto-energy

The relationship between solar radiation capture and potential plant growth is of theoretical and practical importance. The key processes constraining the transduction of solar radiation into phyto-energy (i.e. free energy in phytomass) were reviewed to estimate potential solar-energy-use efficiency. Specifically, the out-put:input stoichiometries of photosynthesis and photorespiration in C(3) and C(4) systems, mobilization and translocation of photosynthate, and biosynthesis of major plant biochemical constituents were evaluated. The maintenance requirement, an area of important uncertainty, was also considered. For a hypothetical C(3) grain crop with a full canopy at 30°C and 350 ppm atmospheric [CO(2) ], theoretically potential efficiencies (based on extant plant metabolic reactions and pathways) were estimated at c. 0.041 J J(-1) incident total solar radiation, and c. 0.092 J J(-1) absorbed photosynthetically active radiation (PAR). At 20°C, the calculated potential efficiencies increased to 0.053 and 0.118 J J(-1) (incident total radiation and absorbed PAR, respectively). Estimates for a hypothetical C(4) cereal were c. 0.051 and c. 0.114 J J(-1), respectively. These values, which cannot be considered as precise, are less than some previous estimates, and the reasons for the differences are considered. Field-based data indicate that exceptional crops may attain a significant fraction of potential efficiency.     

Single strand DNA breaks in rat brain cells exposed to microwave radiation

This investigation concerns with the effect of low intensity microwave (2.45 and 16.5 GHz, SAR 1.0 and 2.01 W/kg, respectively) radiation on developing rat brain. Wistar rats (35 days old, male, six rats in each group) were selected for this study. These animals were exposed for 35 days at the above mentioned frequencies separately in two different exposure systems. After the exposure period, the rats were sacrificed and the whole brain tissue was dissected and used for study of single strand DNA breaks by micro gel electrophoresis (comet assay). Single strand DNA breaks were measured as tail length of comet. Fifty cells from each slide and two slides per animal were observed. One-way ANOVA method was adopted for statistical analysis. This study shows that the chronic exposure to these radiations cause statistically significant (p<0.001) increase in DNA single strand breaks in brain cells of rat.     

Repair of radiation induced DNA double strand breaks by backup NHEJ is enhanced in G2

In higher eukaryotes DNA double strand breaks (DSBs) are repaired by homologous recombination (HRR) or non-homologous end joining (NHEJ). In addition to the DNA-PK dependent pathway of NHEJ (D-NHEJ), cells employ a backup pathway (B-NHEJ) utilizing Ligase III and PARP-1. The cell cycle dependence and coordination of these pathways is being actively investigated. We examine DSB repair in unperturbed G1 and G2 phase cells using mouse embryo fibroblast (MEF) mutants defective in D-NHEJ and/or HRR. WT and Rad54(-/-) MEFs repair DSBs with similar efficiency in G1 and G2 phase. LIG4(-/-), DNA-PKcs(-/-), and Ku70(-/-) MEFs show more pronounced repair defects in G1 than in G2. LIG4(-/-)/Rad54(-/-) MEFs repair DSBs as efficiently as LIG4(-/-) MEFs suggesting that the increased repair efficiency in G2 relies on enhanced function of B-NHEJ rather than HRR. In vivo and in vitro plasmid end joining assays confirm an enhanced function of B-NHEJ in G2. The results show a new and potentially important cell cycle regulation of B-NHEJ and generate a framework to investigate the mechanistic basis of HRR contribution to DSB repair.     

The effects of solar radiation on thermal comfort

The aim of this study was to investigate the relationship between simulated solar radiation and thermal comfort. Three studies investigated the effects of (1) the intensity of direct simulated solar radiation, (2) spectral content of simulated solar radiation and (3) glazing type on human thermal sensation responses. Eight male subjects were exposed in each of the three studies. In Study 1, subjects were exposed to four levels of simulated solar radiation: 0, 200, 400 and 600 Wm⁻². In Study 2, subjects were exposed to simulated solar radiation with four different spectral contents, each with a total intensity of 400 Wm⁻² on the subject. In Study 3, subjects were exposed through glass to radiation caused by 1,000 Wm⁻² of simulated solar radiation on the exterior surface of four different glazing types. The environment was otherwise thermally neutral where there was no direct radiation, predicted mean vote (PMV)=0±0.5, [International Standards Organisation (ISO) standard 7730]. Ratings of thermal sensation, comfort, stickiness and preference and measures of mean skin temperature (t_sk) were taken. Increase in the total intensity of simulated solar radiation rather than the specific wavelength of the radiation is the critical factor affecting thermal comfort. Thermal sensation votes showed that there was a sensation scale increase of 1 scale unit for each increase of direct radiation of around 200 Wm⁻². The specific spectral content of the radiation has no direct effect on thermal sensation. The results contribute to models for determining the effects of solar radiation on thermal comfort in vehicles, buildings and outdoors.     

Recruitment of ATM protein to double strand DNA irradiated with ionizing radiation.

The product of the ATM gene, which is mutated in ataxia telangiectasia, is a nuclear phosphoprotein, and it involves the activation of the p53 pathway after ionizing radiation. Here we show that the ATM protein is constitutively associated with double strand DNA and that the interaction increases when the DNA is exposed to ionizing radiation. The ATM protein also had affinity to restriction endonuclease PvuII-digested DNA, but not to UV-irradiated DNA nor X-irradiated single-stranded DNA. The immunoprecipitation experiment detected very weak association between ATM and DNA-PK proteins, and immunodepletion of DNA-PK showed little or no effect on the interaction of the ATM protein with damaged DNA, indicating that an interaction with DNA-PK might not be required for the recruitment of the ATM protein to damaged DNA. Furthermore, the association was also confirmed in xrs-5 and xrs-6e cells, which are Chinese hamster ovary mutant cell lines defective in Ku80 function. These results indicate that the ATM protein is recruited to the site of DNA damage and it recognizes double strand breaks by itself or through an association with other DNA-binding protein other than DNA-PK and Ku80 proteins.     

The direction of RecA protein assembly onto single strand DNA is the same as the direction of strand assimilation during strand exchange

The RecA protein of Escherichia coli optimally promotes DNA strand exchange reactions in the presence of the single strand DNA-binding protein of E. coli (SSB protein). Under these conditions, assembly of RecA protein onto single-stranded DNA (ssDNA) occurs in three steps. First, the ssDNA is rapidly covered by SSB protein. The binding of RecA protein is then initiated by nucleation of a short tract of RecA protein onto the ssDNA. Finally, cooperative polymerization of additional RecA protein accompanied by displacement of SSB protein results in a ssDNA-RecA protein filament (Griffith, J. D., Harris, L. D., and Register, J. C. (1984) Cold Spring Harbor Symp. Quant. Biol. 49, 553-559). We report here that RecA protein assembly onto circular ssDNA yields RecA protein-covered circles in which greater than 85% are completely covered by RecA protein with no remaining SSB protein-covered segments (as detected by electron microscopy). However, when linear ssDNA is used, 90% of the filaments contain a short segment at one end complexed with SSB protein. This suggests that RecA protein assembly is unidirectional. Visualization of the assembly of RecA protein onto either long ssDNA tails (containing either 5' or 3' termini) or ssDNA gaps generated in double strand DNA allowed us to determine that the RecA protein polymerizes in the 5' to 3' direction on ssDNA and preferentially nucleates at ssDNA-double strand DNA junctions containing 5' termini.     

Effects of tropical solar radiation on the motility of filamentous cyanobacteria

Abstract The effects of tropical solar radiation on the motility of the cyanobacteria Anabaena variabilis, Oscillatoria tenuis and two strains of Phormidium uncinatum were studied in Ghana (4.30°N). The percentages of motile filaments were drastically reduced by unfiltered solar radiation. Covering the organisms with various long pass or band pass filters (WG320, GG395 or UG5) revealed that the UV-B, UV-A and visible light components of the solar spectrum were all effective in impairing motility in these organisms. Only partial recovery was observed and only after short exposure times.     

Hornet peak flight activity is correlated with solar UV radiation: a multi-annual survey

This study deals with the effect which solar irradiation of short wavelength, particularly ultraviolet (UV), exerts on the activities of hornets. The findings are based on multi-annual observations carried out during the years 1985, 1989 and 1998 on hornet nests in the field. At the peak of UV radiation, which occurs at noon, hornet activity is greater by 1-2 orders of magnitude than that during the morning or evening hours. The main visible hornet activity appears to be the removal of soil particles from the nest so as to enlarge its volume, enable the building of additional combs and also increase the size of existing combs. Hornet flight during peak insolation hours is characterized by its briefness (5-20 seconds only) and brevity (to distances of 5-10 meters only) as compared to flights at other hours of the day. These prolonged, multi-annual observations lead to the conclusion that hornets are capable of converting the energy of UV radiation into a form amenable to metabolic usage. In this respect the hornet cuticle behaves as a thermophotovoltaic device, i.e., a semiconductor diode that converts photons radiating from the sunlight into electrical energy.