Effect of space flight conditions on properties of hydrocarbon-oxidizing bacteria

Results of experiments on the Mir space station (EO-25 and EO-26) demonstrated that the conditions of orbital flight, primarily the cosmic radiation, was a mutagenic factor affecting both the genotype and phenotype of an oil-oxidizing bacterial strain, Mycobacterium flavescens EX-91. The emerging mutants differed from original culture by the rate of colony growth and the ability to ferment certain carbohydrates or synthesize beta-galactosidase. Changes in the rate of utilization of raw oil and individual hydrocarbon types (constituting model mixtures) suggest that cosmic radiation may serve as a means of obtaining mutant clones of microorganisms with new properties.     

The Effects of Increasing UV-B Radiation on Pigmentation, Growth and Survival of Coregonid Embryos and Larvae

In the northern regions UV-B radiation levels have increased due to ozone depletion. A two-week laboratory experiment was conducted to measure the effects of UV-B radiation on the pigmentation, growth, oxygen consumption rate and survival of whitefish, Coregonus lavaretus, and vendace, Coregonus albula, larvae. In May newly hatched embryos were exposed in laboratory aquaria to three CIE weighted UV-B radiation levels: subambient (daily dose 1.37kJm^–2), 9% (1.81kJm^–2) and 34% higher (2.24kJm^–2) than ambient. Control embryos and larvae were not exposed to UV-B. Larvae of whitefish and vendace that were irradiated with highest UV-B level had 32% and 31% more melanin than control larvae, respectively, which we interpret as an apparent induced response. In controls, the species difference revealed 53% more melanin in vendace larvae than in whitefish larvae. UV-B radiation had no effect on the mortality of either species, the survival being high in all treatments (>90%). Additionally, neither growth rate nor the metabolic rate of larvae of either species was affected by UV-B radiation. Thus, in relation to future scenarios UV-B radiation may not be a threat to whitefish or vendace larvae in current or expected radiation levels.     

Mating type regulates the radiation-associated stimulation of reciprocal translocation events in Saccharomyces cerevisiae

Both ultraviolet (UV) and ionizing radiation were observed to stimulate mitotic, ectopic recombination between his3 recombinational substrates, generating reciprocal translocations in Saccharomyces cervisiae (yeast). The stimulation was greatest in diploid strains competent for sporulation and depends upon both the ploidy of the strain and heterozygosity at the MAT locus. The difference in levels of stimulation between MATa/MAT diploid and MAT haploid strains increases when cells are exposed to higher levels of UV radiation (sevenfold at 150 J/m²), whereas when cells are exposed to higher levels of ionizing radiation (23.4 krad), only a twofold difference is observed. When the MAT gene was introduced by DNA transformation into a MATa/mat::LEU2 ⁺ diploid, the levels of radiation-induced ectopic recombination approach those obtained in a strain that is heterozygous at MAT. Conversely, when the MATA gene was introduced by DNA transformation into a MAT haploid, no enhanced stimulation of ectopic recombination was observed when cells were irradiated with ionizing radiation but a threefold enhancement was observed when cells were irradiated with UV The increase in radiation-stimulated ectopic recombination resulting from heterozygosity at MAT correlated with greater spontaneous ectopic recombination and higher levels of viability after irradiation. We suggest that MAT functions that have been previously shown to control the level of mitotic, allelic recombination (homolog recombination) also control the level of mitotic, radiation-stimulated ectopic recombination between short dispersed repetitive sequences on non-homologous chromosomes.     

NUNDO: a numerical model of a human torso phantom and its application to effective dose equivalent calculations for astronauts at the ISS

The health effects of cosmic radiation on astronauts need to be precisely quantified and controlled. This task is important not only in perspective of the increasing human presence at the International Space Station (ISS), but also for the preparation of safe human missions beyond low earth orbit. From a radiation protection point of view, the baseline quantity for radiation risk assessment in space is the effective dose equivalent. The present work reports the first successful attempt of the experimental determination of the effective dose equivalent in space, both for extra-vehicular activity (EVA) and intra-vehicular activity (IVA). This was achieved using the anthropomorphic torso phantom RANDO^® equipped with more than 6,000 passive thermoluminescent detectors and plastic nuclear track detectors, which have been exposed to cosmic radiation inside the European Space Agency MATROSHKA facility both outside and inside the ISS. In order to calculate the effective dose equivalent, a numerical model of the RANDO^® phantom, based on computer tomography scans of the actual phantom, was developed. It was found that the effective dose equivalent rate during an EVA approaches 700 μSv/d, while during an IVA about 20 % lower values were observed. It is shown that the individual dose based on a personal dosimeter reading for an astronaut during IVA results in an overestimate of the effective dose equivalent of about 15 %, whereas under an EVA conditions the overestimate is more than 200 %. A personal dosemeter can therefore deliver quite good exposure records during IVA, but may overestimate the effective dose equivalent received during an EVA considerably.     

Light quantity and quality interactions in the control of elongation growth in light-grown Chenopodium rubrum L. seedlings

The spectral control of hypocotyl elongation in light-grown Chenopodium rubrum L. seedlings has been studied. The results showed that although the seedlings responded to changes in the quantity of combined red and far-red radiation, they were also very sensitive to changes in the quantity of blue radiation reaching the plant. Altering the proportion of red: far-red radiation in broad waveband white light caused marked differences in hypocotyl extension. Comparison of the responses of green and chlorophyll-free seedlings indicated no qualitative difference in the response to any of the light sources used, although photosynthetically incompetent plants were more sensitive to all wavelengths. Blue light was found to act primarily of a photoreceptor which is different from phytochrome. It is concluded that hypocotyl extension rate in vegetation shade is photoregulated by the quantity of blue light and the proportion of red: far-red radiation. In neutral shade, such as that caused by stones or overlying soil, hypocotyl extension appears to be regulated primarily by the quantity of light in the blue waveband and secondarily by the quantity of light in the red and far-red wavebands.Abbreviations B blue - FR far-red - k ₁, k ₂ rate constants for photoconverison of Pr to Pfr and Pfr to Pr, respective - k ₁/k ₁ +k ₂= phytochrome photoequilibrium - k ₁ +k ₂= phytochrome cycling rate - Pr=R absorbing form of phytochrome - Pfr=FR absorbing form of phytochrome - P_tot Pr+Pfr - PAR photosynthetically active radiation = 400–700 nm - R red - WL white light     

Estimating the intensity of male-driven evolution in rodents by using X-linked and Y-linked Ube 1 genes and pseudogenes

Using sequence data from the last introns of ZFX and ZFY genes, we previously estimated the male-to-female ratio () of mutation rate to be close to 6 in higher primates and 1.8 in rodents. As the mutation rate may vary among different regions of the mammalian genome, it is interesting to see whether sequence data from other regions will give similar estimates. In this study, we have determined the partial genomic sequences of the ubiquitin-activating enzyme El genes (Ube 1x and Ube 1y for the X-linked and Y-linked homologues, respectively) of mice and rats and two mouse Ube 1y pseudogenes. From the intron sequences of the Ube 1 genes, we calculated the divergence of the Y-linked genes (Y = 0.161) and that of the X-linked genes (X = 0.107) between mouse and rat, and found the Y/X ratio to be 1.50. This ratio led to an estimate of = 2.0 with a 95% confidence interval of (1.0, 3.9). Similar estimates of were obtained if mouse Ube 1y pseudogenes were used instead of the mouse Ube 1y functional gene. These estimates are consistent with our previous estimate for rodents and suggest that the sex ratio of mutation rate in rodents is approximately only one-third of that in higher primates. Our estimate of the divergence time between Ube 1x and Ube 1y supports the view that the two genes separated before the eutherian radiation.Correspondence to: W.-H. Li     

Cytosine methylation and the fate of CpG dinucleotides in vertebrate genomes

Summary The dinucleotide CpG is a hotspot for mutation in the human genome as a result of (1) the modification of the 5 cytosine by cellular DNA methyltransferases and (2) the consequent high frequency of spontaneous deamination of 5-methyl cytosine (5mC) to thymidine. DNA methylation thus contributes significantly, albeit indirectly, to the incidence of human genetic disease. We have attempted to estimate for the first time the in vivo rate of deamination of 5mC from the measured rate of 5mC deamination in vitro and the known error frequency of the cellular G/T mismatch-repair system. The accuracy and utility of this estimate (m _d ) was then assessed by comparison with clinical data, and an improved estimate of m _d (1.66x10^-16 s^-1) was derived. Comparison of the CpG mutation rates exibited by globin gene and pseudogene sequences from human, chimpanzee and macaque provided further estimates of m _d , all of which were consistent with the first. Use of this value in a mathematical model then permitted the estimation of the length of time required to produce the level of CpG suppression currently found in the bulk DNA of vertebrate genomes. This time span, approximately 450 million years, corresponds closely to the estimated time since the emergence and adaptive radiation of the vertebrates and thus coincides with the probable advent of heavily methylated genomes. An accurate estimate of the 5mC deamination rate is important not only for clinical medicine but also for studies of gene evolution. Our data suggest both that patterns of vertebrate gene methylation may be comparatively stable over relatively long periods of evolutionary time, and that the rate of CpG deamination can, under certain limited conditions, serve as a molecular clock.     

Protective Role of Glutathione Synthesis on Radiation-Induced DNA Damage in Rabbit Brain

1. Radiotherapy has attracted increasing interest in recent years. It is known that ionizing radiation induces oxygen radical injury, whereas oxidative stress by the radiation can cause cellular responses to defense cellular injury. In this study, the metabolism of antioxidants in response to ionizing radiation to the brain was studied in the brain using experimental rabbits.2. Ionizing radiation to the hemicerebrum caused an increase in the levels of glutathione (GSH) and the activity of a GSH synthesizing enzyme, -glutamylcysteine synthetase (-GCS), and Cu,Zn-superoxide dismutase (Cu,Zn-SOD). Ionizing radiation also induced DNA-damage estimated by the formation of 8-hydroxydeoxyguanosine. These changes were dependent on the radiation dose.3. Previous intrathecal-administration of buthionine sulfoximine (100 M), a specific inhibitor of -GCS, increased DNA damage by radiation in the radiated hemicerebrum. That of S-methyl GSH, on the other hand, resulted in a significant reduction of DNA damage by radiation.4. These results suggest that synthesis of GSH and Cu,Zn-SOD is responsive to ionizing radiation and this induction of antioxidants may play a role in reducing tissue damage in radiotherapy.     

Four mutants of Micrococcus radiodurans defective in the ability to repair DNA damaged by mitomycin-C, two of which have wild-type resistance to ultraviolet radiation

Summary Four genes concerned with the resistance of wild-type Micrococcus radiodurans to the lethal action of mitomycin-C (MTC), mtcA, mtcB, uvsA and uvsB, have been identified by isolating mutants sensitive to MTC.Two strains of M. radiodurans, 302 and 262 carrying mutations in mtcA and mtcB respectively, are between forty and sixty times as sensitive as the wild-type to MTC, only slightly more sensitive than the wild-type to ionizing () radiation and have the same resistance as the wild-type to ultraviolet (u.v.) radiation. Strain 302 can be transformed at a high frequency to wild-type resistance to MTC with DNA from strain 262, and vice versa, indicating that mtcA and mtcB have different genetic locations.Two further strains of M. radiodurans, 303 and 263 having mutations in uvsA and uvsB respectively are only from four to eight times as sensitive as the wild-type to MTC, seven to thirteen times as sensitive to -radiation but between twenty to thirty-three times as sensitive to u.v. radiation. Strain 303 can be transformed with DNA from strain 263, or vice versa, to wild-type resistance to u.v. radiation, implying that uvsA and uvsB also have different genetic locations. M. radiodurans strain 301 which is mutant in both mtcA and uvsA, and strain 261 which is mutant in mtcB and uvsB are twenty to forty times as sensitive as the wild-type to both MTC and u.v. radiation and seven to ten times as sensitive to radiation. Neither mtcA and uvsA nor mtcB and uvsB are closely linked.None of the mutant strains is deficient in recombination, as measured by transformation. The repair of MTC-induced DNA damage in M. radiodurans must be different from that described for Escherichia coli.     

Simulations of the MATROSHKA experiment at the international space station using PHITS

Concerns about the biological effects of space radiation are increasing rapidly due to the perspective of long-duration manned missions, both in relation to the International Space Station (ISS) and to manned interplanetary missions to Moon and Mars in the future. As a preparation for these long-duration space missions, it is important to ensure an excellent capability to evaluate the impact of space radiation on human health, in order to secure the safety of the astronauts/cosmonauts and minimize their risks. It is therefore necessary to measure the radiation load on the personnel both inside and outside the space vehicles and certify that organ- and tissue-equivalent doses can be simulated as accurate as possible. In this paper, simulations are presented using the three-dimensional Monte Carlo Particle and Heavy-Ion Transport code System (PHITS) (Iwase et al. in J Nucl Sci Tech 39(11):1142–1151, 2002) of long-term dose measurements performed with the European Space Agency–supported MATROSHKA (MTR) experiment (Reitz and Berger in Radiat Prot Dosim 120:442–445, 2006). MATROSHKA is an anthropomorphic phantom containing over 6,000 radiation detectors, mimicking a human head and torso. The MTR experiment, led by the German Aerospace Center (DLR), was launched in January 2004 and has measured the absorbed doses from space radiation both inside and outside the ISS. Comparisons of simulations with measurements outside the ISS are presented. The results indicate that PHITS is a suitable tool for estimation of doses received from cosmic radiation and for study of the shielding of spacecraft against cosmic radiation.     

Some improvements in calculating the plant stand surface albedo and its influence on ground surface temperature

It is shown that better results are obtained in calculating the surface albedo of a plant stand for near-infrared solar radiation using the modified two-stream approximation in favor of the Schwarzschild one. These evaluations of the plant stand surface albedo were obtained by assuming the values for scattering parameters of upward ₀ and diffusive solar radiation in the plant stand, by applying the delta-Eddington approximation. However, more accurate evaluations of ₀ and can be obtained by using Rayleigh's phase scattering functions for radiative scattering in a plant stand. Furthermore, much attention is devoted to testing the influence of the plant stand albedo for the visible part of solar radiation (for which the Schwarzchild approximation is valid) on ground surface temperature. The ground surface temperature was calculated by the force-restore method; the greatest ground surface temperature corrections were obtained in cases where the surface beneath the plant stand is covered with snow. The influence on ground surface temperature of high absorption and scattering in dense plant stands with horizontal foliage was also tested. Again significant corrections of ground surface temperature were obtained, taking into consideration the given characteristics of a plant stand compared to a standard albedo value.List of symbols A albedo of direct radiation in plant canopy - A _D albedo of diffuse radiation in plant canopy - A _p albedo of the ground surface - A _Q total albedo in plant canopy - a proportion of gaps in plant canopy characteristic of surface evaporation - _w constant - parameter of upward scattering diffuse radiation - ₀ parameter of upward scattering direct radiation - C _g soil volumetric heat capacity - C _p air specific heat - C _DH aerodynamic transfer coefficient for heat - C _DE aerodynamic transfer coefficient for moisture - d depth of soil - sun's declination - azimuth of incident radiation - azimuth of diffuse radiation - characteristic of the radiative sources - G foliage orientation function - g parameter in delta-Eddington approximation - g _z parameter for near-infrared radiation - _L scattering phase function radiation - _D diffuse solar radiation flux - _G soil heat flux - _H air sensible heat flux - _L air latent heat flux - _O solar constant - _R net longwave radiation flux - _S direct solar radiation flux - h _o height of the sun - i intensity of diffuse radiation - k von Karman constant - L leaf area index - L _v coefficient for latent heat of evaporation - _g soil heat conductivity - n/N relative cloudiness - solid angle - frequency of temperature wave - Q _a specific humidity of air - Q _w specific humidity of saturated air - R _L coefficient of plant reflectivity - r direction of diffuse radiation - direction of incident radiation - r _o direction of solar radiation - r _s resistance of the leaf stomata - p _o air density - S intensity of direct solar radiation - Stefan-Boltzman constant - T _a air temperature - T _G ground surface temperature - T _c cloud temperature - T ₁ feaf temperature - T _* air temperature scale - t time - t time step - zenith angle of diffuse radiation - zenith angle of incident radiation - ₀ zenith angle of solar radiation - U _* friction velocity scale - V near-surface wind velocity - W _g soil water content - W _L scattering coefficient in plant canopy - W _sat saturated soil water content - z vertical direction     

Effects of temperature and X-ray irradiation on intrinsic growth rate in populations ofDrosophila pseudoobscura

An experiment was designed using populations ofDrosophila pseudoobscura with different gene arrangements on the third chromosome, to study the effects of various temperatures and different dosages of radiation on the innate capacity for increase.The innate capacity for increase was found to increase with temperature and decrease with higher in radiation dosages. The mean generation length showed a decline with both treatments with a greater decrease in the former treatments.Net reproductive rate showed a decrease in both cases while the finite rate of increase () showed an increase in the temperature experiment and a decrease in the radiation experiment.Percentage contribution of each age group to the rate of muliplication per generation depends on temperature and dosages of radiation as well as the genetic background of the population.     

Effect of γ radiation on physiological parameters of the ethanolic fermentation

This work examines the efficacy of radiation in reducing the viability of certain contaminating bacteria of sugar-cane must and the consequential beneficial effect of lethal doses of radiation on some physiological parameters of the yeast-based ethanolic fermentation. The must from sugar-cane juice was inoculated with different bacteria that usually contaminate the must in the production facilities: Bacillus and Lactobacillus. The contaminated must was irradiated at 2.0, 4.0, 6.0, 8.0 and 10.0 kGy of gamma radiation. The population density of the bacteria in the irradiated must was recorded. Ethanolic fermentation by yeast (Saccharomyces cerevisiae) was carried out and the total acidity, the volatile acidity and the organic acids (lactic and acetic) produced during the fermentation were determined. The ethanol yield was also recorded. The treatment with radiation reduced the population of the contaminating microorganisms of the sugar-cane must. The acidity and the organic acids (lactic and acetic) produced during the fermentation decreased as the dose of radiation applied to the must increased. It is concluded that irradiation was efficient in decontaminating the sugar-cane must and improved the biochemical parameters of the ethanolic fermentation, including the ethanol yield by 2%.     

Ultraviolet radiation,ozone depletion,and marine photosynthesis

Concerns about stratospheric ozone depletion have stimulated interest in the effects of UVB radiation (280–320 nm) on marine phytoplankton. Research has shown that phytoplankton photosynthesis can be severely inhibited by surface irradiance and that much of the effect is due to UV radiation. Quantitative generalization of these results requires a biological weighting function (BWF) to quantify UV exposure appropriately. Different methods have been employed to infer the general shape of the BWF for photoinhibition in natural phytoplankton, and recently, detailed BWFs have been determined for phytoplankton cultures and natural samples. Results show that although UVB photons are more damaging than UVA (320–400 nm), the greater fluxes of UVA in the ocean cause more UV inhibition. Models can be used to analyze the sensitivity of water column productivity to UVB and ozone depletion. Assumptions about linearity and time-dependence strongly influence the extrapolation of results. Laboratory measurements suggest that UV inhibition can reach a steady-state consistent with a balance between damage and recovery processes, leading to a non-linear relationship between weighted fluence rate and inhibition. More testing for natural phytoplankton is required, however. The relationship between photoinhibition of photosynthesis and decreases in growth rate is poorly understood, so long-term effects of ozone depletion are hard to predict. However, the wide variety of sensitivities between species suggests that some changes in species composition are likely. Predicted effects of ozone depletion on marine photosynthesis cannot be equated to changes in carbon flux between the atmosphere and ocean. Nonetheless, properly designed studies on the effects of UVB can help identify which physiological and ecological processes are most likely to dominate the responses of marine ecosystems to ozone depletion.Abbreviations BWF biological weighting function - BWF/P-I photosynthesis versus photosynthetically available irradiance as influenced by biologically-weighted UV - Chl chlorophyll a - DOM dissolved organic matter - E _PAR irradiance in energy units (PAR) - E _s saturation parameter for PAR in the BWF/P-I model - E _inh ^* biologically-weighted dimensionless fluence rate for photoinhibition of photosynthesis by UV and PAR - biological weighting coefficient - % MathType!MTEF!2!1!+-% feaafiart1ev1aaatCvAUfeBSjuyZL2yd9gzLbvyNv2CaerbuLwBLn% hiov2DGi1BTfMBaeXatLxBI9gBaerbd9wDYLwzYbItLDharqqtubsr% 4rNCHbGeaGqiVu0Je9sqqrpepC0xbbL8F4rqqrFfpeea0xe9Lq-Jc9% vqaqpepm0xbba9pwe9Q8fs0-yqaqpepae9pg0FirpepeKkFr0xfr-x% fr-xb9adbaqaaeGaciGaaiaabeqaamaabaabaaGcbaGafqyTduMbae% baaaa!37AC!\[\bar \varepsilon \]_PAR biological weighting coefficient for damage to photosynthesis by E _PAR - k() diffuse attenuation coefficient for wavelength - MAAs mycosporine-like amino acids - PAR photosynthetically available radiation - P ^B rate of photosynthesis normalized to Chl - P _s ^B maximum attainable rate of photosynthesis in the absence of photoinhibition - UVA ultraviolet A (320–400 nm) - UVB ultraviolet B (280–320 nm)     

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.     

The effect of sulfide on the blue-green algae of hot springs II. Yellowstone National Park

In the Mammoth Springs (Yellowstone National Park) waters with near neutral pH and soluble sulfide (H₂S, HS^–, S^2–) of over 1–2 mg/liter (30–60M) are characterized by substrate covers of phototrophic bacteria (Chloroflexus and aChlorobium-like unicell) above 50C and by a blue-green alga (Spirulina labyrinthiformis) below this temperature.Synechococcus. Mastigocladus, and other blue-green algae typical of most hot springs of western North America are excluded, apparently by sulfide. The sulfide-adaptedSpirulina photosynthesized at maximum rates at 45C and at approximately 300 to 700Ein/m²/sec of visible radiation. Sulfide (0.6–1.2 mM) severely poisoned photosynthesis of nonadapted populations, but those continuously exposed to over 30M tolerated at least 1 mM without inhibition. A normal¹⁴C-HCO₃ photoincorporation rate was sustained with 0.6–1 mM sulfide in the presence of DCMU (7M) or NH₂OH (0.2 mM), although both of these photosystem II inhibitors prevented photoincorporation without sulfide. Other sulfur-containing compounds (S₂O₃ ^2– SO₃ ^2–, S₂O₄ ^2– thioglycolic acid cysteine) were unable to relieve DCMU inhibition. The lowering of the photoincorporation rate by preferentially irradiating photosystem I was also relieved by sulfide. The most tenable explanation of these results is that sulfide is used as a photo-reductant of CO₂, at least when photosystem II is inhibited. It is suggested that in some blue-green algae photosystem II is poisoned by a low sulfide concentration, thus making these algae sulfidedependent if they are to continue photosynthesizing in a sulfide environment. Presumably a sulfidecytochrome reductase enzyme system must be synthesized for sulfide to be used as a photo-reductant.     

Common misinterpretations of the “linear,no-threshold” relationship used in radiation protection

Summary Absorbed doseD is shown to be a composite variable, the product of the fraction of cells hit (I _H ) and the mean dose (hit size)z to those cells.D is suitable for use with high level exposure (HLE) to radiation and its resulting acute organ effects because, sinceI _H = 1.0, it approximates closely enough the mean energy density in the cell as well as in the organ. However, with low level exposure (LLE) to radiation and its consequent probability of cancer induction from a single cell, stochastic delivery of energy to cells results in a wide distribution of hit sizesz, and the expected mean value,z, is constant with exposure. Thus, with LLE, onlyI _H varies withD so that the apparent proportionality between dose and the fraction of cells transformed is misleading. This proportionality therefore does not mean that any (cell) dose, no matter how small, can be lethal. Rather, it means that, in the exposure of a population of individual organisms consisting of the constituent relevant cells, there is a small probability of particle-cell interactions which transfer energy. The probability of a cell transforming and initiating a cancer can only be greater than zero if the hit size (dose) to the cell is large enough. Otherwise stated, if the dose is defined at the proper level of biological organization, namely, the cell and not the organ, only a large dosez to that cell is effective.Dedicated to Prof. L.E. Feinendegen on the occasion of his 60th birthday     

Evaluation of radioprotective activities of Rhodiola imbricata Edgew – A high altitude plant

The present study reports the radioprotective properties of a hydro-alcoholic rhizome extract of Rhodiola imbricata (code named REC-7004), a plant native to the high-altitude Himalayas. The radioprotective effect, along with its relevant superoxide ion scavenging, metal chelation, antioxidant, anti-lipid peroxidation and anti-hemolytic activities was evaluated under both in vitro and in vivo conditions. Chemical analysis showed the presence of high content of polyphenolics (0.971 ± 0.01 mg% of quercetin). Absorption spectra analysis revealed constituents that absorb in the range of 220–290 nm, while high-performance liquid chromatography (HPLC) analysis confirmed the presence of four major peaks with retention times of 4.780, 5.767, 6.397 and 7.577 min. REC-7004 was found to lower lipid oxidation significantly (p < 0.05) at concentrations viz., 8 and 80 g/ml respectively as compared to reduced glutathione, although the optimally protective dose was 80 g/ml, which showed 59.5% inhibition of induction of linoleic acid degradation within first 24 h. The metal chelation activity of REC-7004 was found to increase concomitantly from 1 to 50 g/ml. REC-7004 (10–50 g/ml) exhibited significant metal chelation activity (p < 0.05), as compared to control, and maximum percentage inhibition (30%) of formation of iron-2,2-bi-pyridyl complex was observed at 50 g/ml, which correlated well with quercetin (34.9%), taken as standard. The reducing power of REC-7004 increased in a dose-dependent manner. The absorption unit value of REC-7004 was significantly lower (0.0183± 0.0033) as compared to butylated hydroxy toluene, a standard antioxidant (0.230± 0.091), confirming its high reducing ability. Superoxide ion scavenging ability of REC-7004 exhibited a dose-dependent increase (1–100 g/ml) and was significantly higher (p < 0.05) than that of quercetin at lower concentrations (1–10 g/ml), while at 100 g/ml, both quercetin and REC-7004 scavenged over 90% superoxide anions. MTT assay in U87 cell line revealed an increase in percent survival of cells at doses between 25 and 125 g/ml in case of drug + radiation group. In vivo evaluation of radio-protective efficacy in mice revealed that intraperitoneal administration of REC-7004 (maximally effective dose: 400 mg/kg b.w.) 30 min prior to lethal (10 Gy) total-body -irradiation rendered 83.3% survival. The ability of REC-7004 to inhibit lipid peroxidation induced by iron/ascorbate, radiation (250 Gy) and their combination [i.e., iron/ascorbate and radiation (250 Gy)], was also investigated and was found to decrease in a dose-dependent manner (0.05–2 mg/ml). The maximum percent inhibition of formation of MDA-TBA complex at 2 mg/ml in case of iron/ascorbate, radiation (250 Gy) and both i.e., iron/ascorbate with radiation (250 Gy) was 53.78, 63.07, and 51.76% respectively and were found to be comparable to that of quercetin. REC-7004 (1 g/ml) also exhibited significant anti-hemolytic capacity by preventing radiation-induced membrane degeneration of human erythrocytes. In conclusion, Rhodiola renders in vitro and in vivo radioprotection via multifarious mechanisms that act in a synergistic manner.     

Regulation of Photosynthesis by Radiation Quality in the Lichen Evernia prunastri

In Evernia prunastri, photosynthetic gas exchange was saturated with yellow radiation (SOX) at 400 mol m^–2s^–1, and then red (R), far-red (FR), or blue (B) radiations at irradiance of 15 mol m^–2s^–1 were added. Because of photosynthesis saturation, any stimulation or decay in CO₂ assimilation by any radiation quality could be attributed to the involvement of a non-photosynthetic photoreceptor. Thus CO₂ assimilation, effective quantum yield, and photochemical quenching were enhanced when R was included, and decreased with FR. Blue radiation completely abolished CO₂ fixation. Hence different spectral radiation qualities may activate non-photosynthetic photoreceptors such as phytochrome and blue photoreceptors, which are involved in regulating the photosynthetic activity in E. prunastri.     

The effect of grasses on the quality of transmitted radiation and its influence on the growth of white clover Trifolium repens

Summary Plants of white clover Trifolium repens were grown under the canopies of three grass species, Lolium perenne, Agrostis tenuis and Holcus lanatus, and under simulated canopies of black polythene and controls were exposed to unfiltered natural radiation. The canopies were adjusted so that they transmitted equal intensities of Photosynthetically Active Radiation (P.A.R.). The ratio of red to far red radiation () was unchanged under the black polythene canopies but was reduced under canopies of Lolium and Agrostis and even more so under Holcus. The effect of canopy filtered radiation on the growth of clover was greatly to reduced internode length, mean number of nodes, the number of branched nodes and the number of rooted nodes and greatly to increase petiole length. The effect of canopies of Holcus was greater than that of the other grass species both in its effect on and on the responses of the clover plant to its shade.