Sunscreen Protection Against Ultraviolet Radiation-induced Pyrimidine Dimers in Mouse Epidermal DNA

Pyrimidine dimers were measured in epidermal DNA of SKH:HRI mice following exposure to solar-simulated UV radiation (SSUV, 290–400 nm) or to UVA (320–400 nm). Mice were exposed to SSUV or UVA after topical application (2 mg/cm²) of vehicle, a UVB absorber (5% 2-ethylhexyl p-methoxycinnamate [2-EHMC]), or a broad-spectrum UVA absorber (5% Mexoryl®SX). The rates of induction of pyrimidine dimers in untreated animals were 5.4 ± 0.57 times 10^-4 (mean ± SEM) and 7.6 ± 0.95 times 10^-6 dimers per 10⁸ Da of epidermal DNA per J/m² of SSUV and UVA, respectively. Topical application of Mexoryl®SX reduced the rate of induction of pyrimidine dimers in SSUV-exposed animals to 4.7 ± 0.44 times 10^-5 dimers per 10⁸ Da per J/m² for a dimer induction protection factor (PF) of 11.5 (5.4 times 10 ⁴/4.7 times 10^-5). The rate of dimer induction in Mexoryl®SX-treated, UVA-ex-posed mice was 0.95 ± 0.2 times 10^-6 dimers per 10⁸ Da per J/m² (PF = 8.0). The 2-EHMC at a concentration of 5% (wt/wt) was significantly less effective than Mexoryl®SX in preventing the induction of pyrimidine dimers in animals exposed to either SSUV or UVA. The rates of dimer induction in 2-EHMC-treated mice were 8.2 ± 1.1 times 10^-5 and 3.8 ± 0.33 times 10^-6 dimers per Da per J/m² of SSUV (PF = 6.6) and UVA (PF = 2.0), respectively. Upon normalizing to the efficacy for edema induction, UVA induced approximately one-fourth the number of pyrimidine dimers per equivalent edematous response when compared to SSUV.     

Medical UV Exposures and HIV Activation

This paper presents the first attempt to evaluate the potential of clinical UV exposures to induce the human immunodeficiency (HIV) promoter and, thus, to upregulate HIV growth in those skin cells that are directly affected by the exposure. Using the data for HIV promoter activation in vitro, we computed UVB and psoralen plus UVA (PUVA) doses that produce 50% of the maximal promoter activation (AD₅₀). Then, using (a) literature data for UV transmittance in the human skin, (b) a composite action spectrum for HIV promoter and pyrimidine dimer induction by UVB and (c) an action spectrum for DNA synthesis inhibition by PUVA, we estimated the distribution of medical UVB and PUVA doses in the skin. This allowed us to estimate how deep into the skin the HIV-activating doses might penetrate in an initial and an advanced stage of UVB or PUVA therapy. Such analysis was done for normal type II skin and for single exposures. The results allow us to predict where in the skin the HIV promoter may be induced by selected small and large therapeutic UVB or PUVA doses. To accommodate changes in skin topography due to disease and UV therapy, our considerations would require further refinements. For UVB we found that, when the incident dose on the surface of the skin is 500 J/m² (290–320nm) (initial stage of the therapy), the dose producing 50% of the maximal HIV promoter activation (AD^UVB₅₀) is limited to the stratum corneum. However, with an incident dose of 5000 J/m² (an advanced stage of the therapy), AD^UVB₅₀ may be delivered as far as the living cells of the epidermis and even to some parts of the upper dermis. For PUVA we found that, when the incident UVA doses are 25 or 100 kJ/m² (320–400nm) (an initial and an advanced stage of therapy, respectively), and the 8-methoxypsoralen concentration in the blood is 0.1 μg/mL (the desired level), the combined doses to the mid epidermis (and some areas of the upper dermis) are well below the 50% HIV promoter-activating PUVA dose (AD^PUVA₅₀). Only under the worst scenario conditions, i. e. an exceptionally high drug concentration in the patient's tissues and localization of HIV in the nearest proximity to the skin surface, would the combined PUVA dose expected during photochemotherapy exceed AD^PUVA₅₀. These results suggest that the probability of HIV activation in the epidermis by direct mechanisms is higher for UVB than for PUVA treatment. However, complexities of the UV-inducible HIV activation and immunomodulatory phenomena are such that our results by themselves should not be taken as an indication that UVB therapy carries a higher risk than PUVA therapy when administered to HIV-infected patients.     

INDUCTION OF SKIN TUMORS IN THE RAT BY SINGLE EXPOSURE TO ULTRAVIOLET RADIATION

Abstract— The dose response for tumor induction in albino rat skin by single exposures of UV radiation has been characterized. The shaved dorsal skin of 202 animals was exposed to either of two sources: one emitting a broad spectrum of wavelengths from 275 to 375 nm, and the other emitting at 254 nm. Skin tumors began to appear within 10 weeks of exposure and continued to appear for 70 weeks. The highest tumor yield was 5.5 tumors per rat and occurred when the rats were exposed to 13.0 times 10⁴ J/m² of the 275–375 nm UV. The 275–375 nm UV was about eight times as effective as the 254 nm UV for the induction of tumors throughout the exposure range from 0.8 times 10⁴ to 26.0 times 10⁴J/m². Tissue destruction and hair follicle damage was found at the highest exposure to 275–375 nm UV but at none of the exposures to 254 nm UV. Repeated weekly exposures to 275–375 nm UV proved less effective than an equivalent single exposure for inducing tumors, even though the multiple exposures caused more severe skin damage. The transmission of the UV through excised samples of rat epidermis indicated that the exposure to the basal cell layer was about 3% of the surface exposure at 254 nm and about 15% of the surface exposure between 275 and 320 nm. The dependence of tumor yield on UV exposure was linear for 254 nm UV but was more complex for the 275–375 nm UV. For the latter more tumors were produced per unit exposure at lower exposures than at higher exposures.     

UV-induced free radicals in oriented DNA.

Abstract— Samples of oriented DNA containing 30% water were UV-irradiated at 77 K and investigated by electron paramagnetic resonance (EPR). The EPR spectra recorded in directions parallel and perpendicular to the DNA fibre direction showed that at low UV doses the induced free radicals are very similar to those induced by γ-irradiation at the same temperature. The γ-induced free radicals have previously been analysed and found to consist mainly of anionic free radicals on thymine and cationic free radicals on guanine. At higher UV doses or by suitable annealing of the samples given a low UV dose, significant amounts of hydrogen-addition radicals on thymine were observed. The quantum yield of free radical formation for irradiation at 300nm ± 10nm was estimated to 10^--⁴. We also made a quantitative determination of the UV-induced free radicals inside an optically effective volume of the sample. The following free radical induction frequencies at 77 K were estimated: γ-rays: 2 × 10^--¹² free radicals per rad per dalton and UV (300nm): 6 × 10^--¹² free radicals per J/m² per dalton.     

Ultraviolet Spectral Energy Differences Affect the Ability of Sunscreen Lotions to Prevent Ultraviolet-Radiation-Induced Immunosuppression*

Acute exposure to UV radiation causes immunosuppression of contact hypersensitivity (CH) responses. Past studies conducted with unfiltered sunlamps emitting nonsolar spectrum UV power (wavelengths below 295 nm) or using excessive UV doses have suggested sunscreens may not prevent UV-induced immunosuppression in mice. This study was thus designed to evaluate critically the effects of different UV energy spectra on the immune protection capacity of sunscreen lotions. Minimum immune suppression doses (MISD), i.e. the lowest UV dose to cause~50% suppression of the CH response to dinitrofluorobenzene in C3H mice, were established for three artificial UV sources. The MISD for each UV source was 0.25 kJ/m² for unfiltered FS20 sunlamps (FS), 0.90 kJ/m² for Kodacel-filtered FS20 sunlamps (KFS), which do not emit UV power at wavelengths <290 nm, and 1.35 kJ/m² for a 1000 W filtered xenon arc lamp solar simulator. Using MISD as baseline, sunscreens with labeled sun protection factors (SPF) of 4, 8, 15 and 30 were tested with each UV source to establish their relative immune protection factors. The immune protection factor of each sunscreen exceeded its labeled SPF in tests conducted with the solar simulator, which has a UV power spectrum (295–400 nm) similar to that of sunlight. Conversely, sunscreen immune protection factors were significantly less than the labeled SPF in tests conducted with FS and KFS. Comparison of the immunosuppression effectiveness spectra showed that relatively small amounts of nonsolar spectrum UV energy, i.e. UVC (200–290 nm) and/or shorter wavelength UVB (between 290 and 295 nm), produced by FS and KFS contributes significantly to the induction of immunosuppression. For example, 36.3% and 3.5% of the total immunosuppressive UV energy from FS and KFS, respectively, lies below 295 nm. Sunscreen absorption spectra showed that transmission of immunosuppressive UV energy below 295 nm for FS was at least eight-fold higher than that for KFS. Compared to the solar simulator UV spectrum the transmission of nonsolar immunosuppressive UV energy through sunscreens was >15-fold higher for FS and ≥1.5-fold higher for KFS. These data demonstrate that relevant evaluations of sunscreen immune protection can only be obtained when tests are conducted with UV sources that produce UV power spectra similar to that of sunlight and UV doses are employed that are based on established MISD.     

DNA polymerase I-mediated repair of 365 nm-induced single-strand breaks in the DNA of Escherichia coli.

Abstract. Irradiation of closed circular phage Λ DNA in vivo at 365 nm results in the induction of single-strand breaks and alkali-labile lesions at rates of 1.1 × 10^-14, and 0.2 × 10^-14/dalton/J/m², respectively. The sum of the induction rates is similar to the rate of induction of single-strand breaks plus alkali-labile lesions (1 × 10^-14/dalton/J/m²) observed in the E. coli genome. Postirradiation incubation of wild-type cells in buffer results in rapid repair of the breaks (up to 80% repaired in 10 min). No repair was observed in a DNA polymerase I-deficient mutant of E. coli.     

Induction of single-strand breaks (alkali-labile bonds) in bacterial and phage DNA by near UV (365 nm) radiation

Abstract —Irradiation at 365 nm results in the induction of approximately 2–4 times 10^-6 and 1-2times 10^-6 single-strand breaks (alkali-labile bonds) per 10⁸ daltons per J m^-2 in extracted phage T4 DNA and in Escherichia coli bacterial DNA, respectively. The rate of break induction in DNA of intact phage is approximately one-fourth that for extracted phage DNA. 2-aminoethylisothiouronium bromide-HBr protects against break induction in both phage systems. No breaks are induced in the DNA of bacteria irradiated under anaerobic conditions over the dose range tested. Possible induction mechanisms are suggested. Consideration is given to the relative importance of pyrimidine dimers and single-strand breaks in the bactericidal action of 365 nm radiation.     

Effect of ultraviolet irradiation on eggs and larvae on the northern anchovy, Engraulis mordax, and the Pacific mackerel, Scomber japonicus, during the embryonic stage.

Abstract— Anchovy and mackerel eggs and yolk-sac larvae were exposed to UV radiation in the bioactive band of wavelengths between 280 and 320 nm. the UV-B region of the spectrum. Irradiation levels were based upon predicted UV-B increases that would result from anthropogenic diminution of Earth's protective ozone shell. Dose-response relationships for mortality and histological and morphological effects were determined for two different spectral energy compositions, using FS-40 sunlamps and two filter combinations. Anchovy were more sensitive than mackerel to UV-B. Data for anchovy were analyzed in terms of DNA-effective doses, i.e. the integrated spectral thence (in J/m²/nm) with the energy at each nm weighted by its effectiveness relative to the Setlow generalized DNA action spectrum. Fifty per cent of anchovy survived a cumulative DNA effective dose of 1150J'm^-2 over a 4-day period. In the surviving larvae. irradiation induced lesions in the brain and eye. caused marked dispersion of pigment within melanophores and retarded growth and development. At the lowest dosage used. 760 (J. m^-2)_DNA, growth was retarded and brain lesions occurred in anchovy. Calculations of Smith and Baker (in this issue) indicate that in clear ocean water a significant incidence of lesions and retardation of growth in anchovy could occur at the surface at a 25%, reduction in ozone and down to 3.5 m at a 50% reduction. Eggs and larvae of anchovy occur at these depths.     

THE ACTION SPECTRUM AND DOSE RESPONSE STUDIES OF UNSCHEDULED DNA SYNTHESIS IN NORMAL HUMAN FIBROBLASTS

Abstract— Excision repair of DNA damage by UV has been assessed in normal human fibroblasts in culture by measuring unscheduled DNA synthesis. Dose response experiments indicated that the same chromophore was involved in UV-induced damage and excision repair at three different wavelengths between 260 and 300 nm. Action spectra for unscheduled DNA synthesis were determined at wavelengths between 260 and 320 nm 30 min after irradiation using 2 doses of UV, 100 J m^-2and 10Jm^-2. Experiments at the lower dose were carried out because it appeared that repair was saturated with the higher dose at 260 and 280 nm. To explore this part of the spectrum further, experiments were performed with different doses at 260 and 280 nm and unscheduled DNA synthesis assessed 30 min and 24 h after irradiation. At 24 hr after irradiation a significantly greater amount of unscheduled DNA synthesis occurred at 280 nm. It is suggested, therefore, that both DNA and protein are concerned in the absorption of UV which leads to DNA damage and excision repair.     

ULTRAVIOLET RADIATION-INDUCED PHOSPHOLIPASE A2 ACTIVATION OCCURS IN MAMMALIAN CELL MEMBRANE PREPARATIONS

Ultraviolet erythema in human skin is mediated in part by membrane derivatives of arachidonic acid (AA). UVA (320–400nm) and UVB (290–320nm) have been shown to induce release of AA from intact mammalian cells in culture. In order to investigate the mechanism of this release we examined the effect of UVA and UVB on release of [³H] AA from membrane preparations of murine fibroblasts. C3H 10T1/2 cells were prelabelled for 24 h with [³H] AA. The membrane fractions of the cells were separated after lysis by differential centrifugation. The membranes were irradiated in suspension and the [³H] AA released from the membranes was determined by scintillation spectroscopy of supernatants3–4 h after irradiation. Both UVA and UVB induced release of AA from the membrane preparations. The response to UVB was small but significant, reaching levels approximately 150% of control release at doses of 1,200-4,000 J/m². The response to UVA was larger; doses of 2.5-5.0 J/cm² induced release equal to twice control (200%) levels, while doses of10–20 J/cm² induced maximal release at levels approximately 400% of control. Time course studies with UVB and UVA showed maximal release at 4 h after irradiation. When the membrane preparations were incubated with a polyclonal anti-phospholipase A₂ antibody the UV induced release of [³H] AA was completely inhibited in both UVB (1200 J/m²) and UVA (10 J/cm²) treated cells. These data suggest that activation of phospholipase A₂ is responsible for the UV induced release of AA in mammalian cells and that the mechanism of this activation is due, in part at least, to direct photon-membrane interaction.     

Ultraviolet action spectrum (238-405 nm) for inhibition of glycine uptake in E. coli.

Abstract— Initial rate of uptake of ³H-glycine by Escherichia coli B/r was measured immediately after irradiation with monochromatic light. Uptake was proportional to time for at least 2 min in both control and irradiated samples. Inhibition of uptake is an exponential function of fluence to about 20% remaining activity, beyond which it is much more resistant to irradiation, suggesting two different uptake systems. The principal (sensitive) system shows an F₃₇ of 2.2 kJ/m² at 280 nm and 110 kJ/m² at 334 nm. The response is independent of cell killing and of presence of the rel gene. The chromophore remains unidentified, although an action spectrum suggests a protein chromophore in the far-UV (below 300 nm) region and a menaquinone chromophore in the near-ultraviolet (above 300 nm). A 10–20%, stimulation of uptake rate, which we cannot account for, is observed at low fluences (generally below 100 kJ/m²) at 313, 366 and 405 nm, but not at 334 nm.     

Measurement and Analysis of Broadband UVB Solar Radiation in Spain

Measurements of broadband UVB irradiance (290–315 nm) at 14 locations in Spain for the period 2000–2009 have been used to generate instantaneous, hourly and daily values of irradiance (W m^?2) and radiant exposure (kJ m^?2). These measurements, and its statistical indices, have been analyzed. For the UVB irradiance, the values corresponding to July (maximum) and December (minimum) have been analyzed as representative of the year during the whole period for all locations. For the UVB radiant exposure, the temporal evolution of daily values has been evaluated for all locations to estimate an average yearly behavior. The accumulated radiant exposure for an average year has also been studied for each location. Finally, to determine possible trends in the evolution of the UVB levels, the linear regressions for the mean daily values for all locations have been determined.     

Photometric titrations of mercury(II) based on UV-absorption of mercury(II)-complexes

Summary A method is described for the complexometric determination of traces of mercury(II) with EDTA, EGTA and DTPA, with photometric endpoint indication. Titrations with EDTA and EGTA appeared to be possible only if acetylacetone was added. The wavelength used in that case was 275 nm. With DTPA a direct titration is possible at 260 nm. At p_H 2 determinations of 2·10^–5 M mercury(II) are possible with good accuracy.

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Zusammenfassung Eine komplexometrische Bestimmung von Spuren Quecksilber(II) mit ÄDTA, ÄGTA und DTPA wurde beschrieben. Die Endpunktanzeige erfolgte photometrisch. Titrationen mit ÄDTA und ÄGTA waren nur möglich in Anwesenheit von Acetylaceton. In diesem Fall war die verwendete Wellenlänge 275 nm. Mit DTPA sind auch direkte Titrationen möglich bei 260 nm. Bei p_H 2 sind Analysen von 2·10^–5-m Lösungen mit guter Genauigkeit durchführbar.

     

SPECTRAL ALBEDO MEASUREMENTS IN THE UV and VISIBLE REGION OVER DIFFERENT TYPES OF SURFACES

Abstract— The spectral albedo of the earth's surface, i.e. the ratio between spectral irradiance reflected by the ground to all directions and global irradiance, was measured by a spectroradiometer in the UV and visible region from 290 nm to 800 nm with a spectral resolution of 1.5 nm at steps of 2 nm in the UV (290–400 nm) and 10 nm in the visible (400–800 nm) region. The measurements were performed over bare fertile soil, sand at the beach, concrete (autobahn) and snow as well as over different types of vegetation (grass, oats, rye, sugar-beet, stubble). As the albedo increases with increasing wavelengths for most types of surfaces considered, it is smaller in the UV than in the visible region. In the UVB region (λ < 315 nm) the measured albedo is as small as 0.016-0.017 over vegetation, 0.04-0.05 over bare fertile soil, 0.07-0.10 over concrete ("autobahn") and 0.62-0.76% over polluted snow with a small wavelength dependence. A somewhat higher albedo occurs in the UVA region (315 < λ < 400 nm) with values ranging from 0.02 over vegetation to 0.05 to 0.08 over bare soil. The albedo over dry bright sand, which is typically found at the beach, is significantly higher (0.14 at 300 nm to 0.24 at 400 nm) than over other snow-free surfaces, thus leading to an enhanced dose of biologically effective radiation at the beach.     

Photochemical properties of Ag ion clusters included within ZSM-5 zeolites prepared by an ion-exchange method

Photoluminescence investigations of the Ag ion-exchanged ZSM-5 (Ag⁺ /ZSM-5) zeolite revealed that a Ag ion cluster (Agⁿ _m ⁺) exists in the pore structure of ZSM-5 exhibiting photoluminesm cence at 380 nm upon excitation at 332 nm. UV irradiation ( = 285 nm) of Ag⁺ /ZSM-5 at 77 K leads to the transformation of Agⁿ _m ⁺ into a different Ag ion cluster (Ag_m ^(n-1)+) which exhibits photoluminescence at 465 nm upon excitation at 315 nm. This photo-transformation of the Ag ion clusters was found to be thermally reversible under vacuum. It was demonstrated that an electron transfer from the photo-excited Al³⁺ -O^2- to Agⁿ _m ⁺ plays a significant role in this process. In the presence of oxygen, UV irradiation of Ag⁺ /ZSM-5 leads to the formation of O₂- instead of an Ag ion cluster (Ag_m ^(n-1)+), suggesting that oxygen acts as an efficient electron scavenger, which interferes with the electron capture of Agⁿ _m ⁺ under UV irradiation at 285 nm.     

The Value of the Ratio of UVA to UVB in Sunlight

The objective of this communication is to present the calculated ratio between UVA and UVB irradiance from sunrise to sunset and under a number of weather conditions. UVA plays an important role in the sun spectrum and a lot of attention has been paid lately regarding the protection of people from UVA. Solar spectra were collected in Kuwait City located at 29.3^oNorth latitude (similar to that of Houston, TX) over a period of 8 months and under various weather conditions. Spectra were collected from 260 nm to 400 nm in 2 nm increments for solar elevation angles from 10^o to 90^o using a calibrated Optronics Laboratories OL‐742 Spectroradiometer. The measurements reported in this study the ratio of UVA (320–400 nm) to UVB (280–320 nm) in solar terrestrial radiation remains essentially constant and equal to 20 for the part of the day when the solar elevation is greater than 60^o. Consequently the value of the ratio of solar UVA/UVB should be considered as equal to 20 for studies in photobiology and photomedicine. When the wavelength limiting the range of UVA and UVB is 315 nm (i.e. UVB: 280–315 nm and UVA: 315–400 nm) the ratio of UVA to UVB becomes equal to 41.     

DIFFERENTIAL SENSITIVITY TO INACTIVATION OF NUR AND NUR+ STRAINS OF ESCHERICHIA COLI AT SIX SELECTED WAVELENGTHS IN THE UVA,UVB AND UVC RANGES*

The radiation response of stationary-phase cells of Escherichia coli strains RT4 (nur⁺) and RT2 (nur) was measured at 6 selected wavelengths between 254 and 405 ran. The relative response of the nur⁺. and nur strains was almost the same at 254 and 290 nm. However, the differential sensitivity of the RT4 and RT2 strains (ratio of the initial F₃₇ values of the nur⁺ to the nur strains) was 2.7 at 313 nm, 3.2 at 334 nm, 3.1 at 365 nm, and 2.3 at 405 nm. Thus, the fluence enhancing effect of the nur genotype extends over the wavelength range of approximately 300 to 420 nm. The substantial effect of nur at 313 nm strongly suggests that the increased sensitivity of the nur strain is the consequence of a repair deficiency that reduces the efficiency of mending DNA lesions produced by UVA (320–400 nm) and UVB (290–320 nm), but not UVC (200–290 nm) radiation.     

PHOTOREGULATION OF LOGARITHMIC FLUENCE-RESPONSE CURVES FOR PHYTOCHROME CONTROL OF CHLOROPHYLL FORMATION IN PISUM SATIVUM L*

Abstract— Logarithmic fluence-response curves for red (660 nm) and far red (730 nm) light induction of rapid chlorophyll a (Chi a) accumulation in pea seedlings (Pisum sativum L. cv. Early Alaska) indicate extreme light sensitivity in dark-grown seedlings. The energy requirement for onset of 660 nm light induction is less than 20 μJ m^-2 and for 730 nm is about 1 mJ m^-2. De-etiolation produced by a saturating exposure of red light (3–8 kJ m^-2) 24 h prior to the construction of the logarithmic fluence-response curves resulted in approximately a 3 fold increase in slope for 660 nm light, whereas the energy requirement for onset of induction shifted to about 100 mJ m^-2. In such de-etiolated plant material, far red applied at low incident energies almost completely lost its inductive capacity. The inductive capacity of far red applied as high irradiance over a long period of time (16h) appeared not to be affected by the de-etiolation treatment. Reciprocity failed for both dark-grown and de-etiolated seedlings upon exposures exceeding 1,000s. Nearly identical results were obtained for seedlings de-etiolated by red exposures immediately followed by far red (4.8 kJ m^-2), although this treatment did not lead to any significant decrease in spectrophotometrically measurable phytochrome. Therefore, no simple correlation was observed between the level of phytochrome present and the sensitivity of seedlings for induction of rapid Chl a accumulation. In order to explain this apparent phytochrome paradox the possibility was tested and ruled out for changes in the degree of synchronization of seedlings, or for induction of some sort of circadian rhythmicity in light sensitivity being involved. In addition, no correlation was observed between induction of morphogenic development and changing light sensitivity. These results formed, therefore, additional support for a model for phytochrome action involving its intracellular transport and local concentration during the process of seedling de-etiolation.     

SURVIVAL, SPORE FORMATION AND EXCISION REPAIR OF UV-IRRADIATED DEVELOPING CELLS OF DICTYOSTELIUM DISCOIDEUM NC-4

Abstract— The synchronously developing aggregates of the cellular slime mold, Dictyostelium discoideum NC-4, were disaggregated into individual cells and irradiated with 254 nm UV light at preaggregation (0h), late interphase (6h), late aggregation (12 h), and preculmination (18 h). When assayed for replica-tive ability (colony formation), the developing cells at 0, 6, 12, and 18h showed the same sensitivity as vegetative cells; the 10% survival dose (D₁₀) was 160 J/m². The spores were more sensitive, with D₁₀ of 70 J/m². Excision repair of the nuclear DNA of the developing cells was studied by alkaline sucrose gradients. UV-induced single-strand breakage and rejoining of the DNA occurred to the same final extent in the cells from the 0, 6, 12 and 18 h stages of development, but a longer time was required for the completion of rejoining at the later stages (for example, at 54 J/m², 6.6 h for preculmination cells, 3.3 h for preaggregation cells). When the cells irradiated at various stages were required to redevelop, as measured by the relative numbers of spores produced, their sensitivity for completing this development increased the later the stage from which they were taken. The D₁₀s for spore production were 200, 130, 100 and 70 J/m² for cells at the 0, 6, 12 and 18 h stages, respectively. The fractional viability among the spores that appeared after this treatment was the same independent of the stage at which the cells were irradiated; the D₁₀ for this viability was 160 J/m², the same as if the cells had been plated immediately with no intervening developmental sequence. We conclude that DNA excision repair as related to replicative ability is retained at all stages of development; however, development seems independent of replicative ability and depends upon DNA and/or non-DNA damage in a more complex way.     

Stepwise ionization of hydroquinone vapor by monochromatic radiation

Processes of stepwise ionization of hydroquinone vapor by radiation in the range 315–275 nm were studied using photoionization spectroscopy techniques. The two-step ionization process yielding molecular ions was found to prevail at a laser power density up to ∼10⁷ W/cm². As the radiation intensity increases, the progressively stronger and deeper degradation takes place via dissociation of the molecular and, probably, fragment ions due to absorption of at least one additional photon. The slow process of the formation of C₅H₆O⁰ ions at an effective rate constant of the order of 10⁶ s⁻¹ was observed.