896 resultados para 0.044-0.04 µm
Resumo:
The level and distribution of some heavy metals viz Cadmium, Lead, Copper Zinc, and Cobalt in five commercially important fishes, water and sediments at three different locations in Kainj Lake were determined using standard methods. The results show that the ranges of heavy metals mu g/g in fishes in Dam site Laotian are: Cd (0.05~c0.01-20~c01), (Pb(ND-1.12 plus or minus )1), Cu (0.81~c25-2.93~c06), Zn (20.89 arrow right .15-36.78~c2.97), Co(0.08~c01-0.27~c02); in cover Dam, the ranges are Cd (0.04~c02-0.16~c0.2), Pb (nd-02~c01), Cu(0.75~c05-2.61~c13), Zn(15.70~c1.55-32.23~c2.70), Co(0.04~c02-0.25~c0.01) and in Yuna they are Cd (0.05~c01-0.14~c02), Pb (nd-0.32~c01), Cu (0.23~c07-2.70~c05), Zn(15.50 plus or minus `.35-25.62~c2.47), Co(0.07~c02-23~c0.01). The metals concentration (mg/l) in the water sample from Dam site, cover dam and Yuna respectively are Cd(0.007~c001,. 004~c001 and 0.005~001), Pb(013~c001, ND and ND), Cu(.055~c008.030~c007, 05 plus or minus .010), Zn(0.13~c01, 0.060 plus or minus .0055) and Co (.026 plus or minus .022 plus or minus .004, .024 plus or minus .004), while the metals concentration ( mu g/g) in sediments sample from Dam site, cover dam and Yuna are respectively Cd(.05 plus or minus .01, .02 plus or minus .01), Pb(16.00~c1.00, ND and 9.33~c1.01), Cu(24.00~c1.34, 4.26 plus or minus .91 and 11.08~c1.32), Zn(42.00~c1.00, 35~c10 and 38.00 plus or minus .45), Co(15.00~c1.17, 8.69~c1.21 and 10.91~c44). The concentrations of the tested heavy metals are within the acceptable standards of WHO (1987a)
Resumo:
This work is divided into two independent papers.
PAPER 1.
Spall velocities were measured for nine experimental impacts into San Marcos gabbro targets. Impact velocities ranged from 1 to 6.5 km/sec. Projectiles were iron, aluminum, lead, and basalt of varying sizes. The projectile masses ranged from a 4 g lead bullet to a 0.04 g aluminum sphere. The velocities of fragments were measured from high-speed films taken of the events. The maximum spall velocity observed was 30 m/sec, or 0.56 percent of the 5.4 km/sec impact velocity. The measured velocities were compared to the spall velocities predicted by the spallation model of Melosh (1984). The compatibility between the spallation model for large planetary impacts and the results of these small scale experiments are considered in detail.
The targets were also bisected to observe the pattern of internal fractures. A series of fractures were observed, whose location coincided with the boundary between rock subjected to the peak shock compression and a theoretical "near surface zone" predicted by the spallation model. Thus, between this boundary and the free surface, the target material should receive reduced levels of compressive stress as compared to the more highly shocked region below.
PAPER 2.
Carbonate samples from the nuclear explosion crater, OAK, and a terrestrial impact crater, Meteor Crater, were analyzed for shock damage using electron para- magnetic resonance, EPR. The first series of samples for OAK Crater were obtained from six boreholes within the crater, and the second series were ejecta samples recovered from the crater floor. The degree of shock damage in the carbonate material was assessed by comparing the sample spectra to spectra of Solenhofen limestone, which had been shocked to known pressures.
The results of the OAK borehole analysis have identified a thin zone of highly shocked carbonate material underneath the crater floor. This zone has a maximum depth of approximately 200 ft below sea floor at the ground zero borehole and decreases in depth towards the crater rim. A layer of highly shocked material is also found on the surface in the vicinity of the reference bolehole, located outside the crater. This material could represent a fallout layer. The ejecta samples have experienced a range of shock pressures.
It was also demonstrated that the EPR technique is feasible for the study of terrestrial impact craters formed in carbonate bedrock. The results for the Meteor Crater analysis suggest a slight degree of shock damage present in the β member of the Kaibab Formation exposed in the crater walls.
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A compulsão alimentar está associada a diversas doenças, entre elas, a obesidade.Com o intuito de pesquisar a diferença hormonal ligada ao controle da fome e da saciedade associada ao episódio de compulsão alimentar (ECA), avaliou-se a concentração sérica dos hormônios que regulam este processo em mulheres adultas. Métodos: O estudo experimental foi composto de 3 grupos (n=23), sendo: grupo Eutrófico (GE;n=8), grupo obeso sem ECA (GO;n=7) e obesas com ECA (ECA;n=8). Todas as mulheres que participaram do estudo freqüentavam os serviços de saúde da Policlínica Piquet Carneiro. Foram dosados os hormônios: Grelina Total, Glucagon, Adiponectina, Amilina, Peptídeo C, GLP-1, Insulina e Leptina séricos nos tempos: jejum, 15 e 60 minutos após a ingestão da refeição fornecida. As refeições ingeridas foram controladas em energia, 55% carboidratos, 15% proteínas, 30% lipídios. Os dados foram analisados como valores médios por grupo em software SAS, considerando p<0,05. Resultados: A idade das mulheres estudadas variou de 32 a 50 anos. A concentração de adiponectina encontrada, que é inversamente proporcional a adiposidade, foi significativamente menor no grupo ECA em relação aos demais grupos (p=0,01). Em relação à leptina, o grupo GO apresentou concentração maior em relação aos demais grupos (p<0,0001). Já, a concentração de grelina encontrada foi significativamente menor no grupo ECA em relação aos demais grupos (p=0,02). Foram encontradas concentrações significativamente maiores de insulina no grupo GO em relação aos demais grupos (p=0,04). A concentração de amilina encontrada foi significativamente maior no grupo GO em relação aos outros grupos (p=0,01). A concentração de GLP-1 encontrada no grupo GO foi maior em média, porém esta diferença não foi estatisticamente significativa entre os grupos (p=0,25). A concentração de Peptídeo C encontrada no grupo GO foi maior em relação aos outros grupos (p=0,003). Apesar da concentração de Glucagon no grupo ECA ser maior em relação aos demais grupos, estes valores não eram diferentes estatisticamente (p=0,13). Nossos achados mostraram que obesas ECA tem perfil hormonal diferente de obesas sem ECA. A baixa concentração de grelina do grupo de obesas ECA e a alta concentração de insulina, peptídeo C e amilina nas obesas com e sem ECA pode estar relacionado com o aumento da ingestão alimentar e com o desequilíbrio energético.
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The initial probabilities of activated, dissociative chemisorption of methane and ethane on Pt(110)-(1 x 2) have been measured. The surface temperature was varied from 450 to 900 K with the reactant gas temperature constant at 300 K. Under these conditions, we probe the kinetics of dissociation via trapping-mediated (as opposed to 'direct') mechanism. It was found that the probabilities of dissociation of both methane and ethane were strong functions of the surface temperature with an apparent activation energies of 14.4 kcal/mol for methane and 2.8 kcal/mol for ethane, which implys that the methane and ethane molecules have fully accommodated to the surface temperature. Kinetic isotope effects were observed for both reactions, indicating that the C-H bond cleavage was involved in the rate-limiting step. A mechanistic model based on the trapping-mediated mechanism is used to explain the observed kinetic behavior. The activation energies for C-H bond dissociation of the thermally accommodated methane and ethane on the surface extracted from the model are 18.4 and 10.3 kcal/mol, respectively.
The studies of the catalytic decomposition of formic acid on the Ru(001) surface with thermal desorption mass spectrometry following the adsorption of DCOOH and HCOOH on the surface at 130 and 310 K are described. Formic acid (DCOOH) chemisorbs dissociatively on the surface via both the cleavage of its O-H bond to form a formate and a hydrogen adatom, and the cleavage of its C-O bond to form a carbon monoxide, a deuterium adatom and an hydroxyl (OH). The former is the predominant reaction. The rate of desorption of carbon dioxide is a direct measure of the kinetics of decomposition of the surface formate. It is characterized by a kinetic isotope effect, an increasingly narrow FWHM, and an upward shift in peak temperature with Ɵ_T, the coverage of the dissociatively adsorbed formic acid. The FWHM and the peak temperature change from 18 K and 326 K at Ɵ_T = 0.04 to 8 K and 395 K at Ɵ_T = 0.89. The increase in the apparent activation energy of the C-D bond cleavage is largely a result of self-poisoning by the formate, the presence of which on the surface alters the electronic properties of the surface such that the activation energy of the decomposition of formate is increased. The variation of the activation energy for carbon dioxide formation with Ɵ_T accounts for the observed sharp carbon dioxide peak. The coverage of surface formate can be adjusted over a relatively wide range so that the activation energy for C-D bond cleavage in the case of DCOOH can be adjusted to be below, approximately equal to, or well above the activation energy for the recombinative desorption of the deuterium adatoms. Accordingly, the desorption of deuterium was observed to be governed completely by the desorption kinetics of the deuterium adatoms at low Ɵ_T, jointly by the kinetics of deuterium desorption and C-D bond cleavage at intermediate Ɵ_T, and solely by the kinetics of C-D bond cleavage at high Ɵ_T. The overall branching ratio of the formate to carbon dioxide and carbon monoxide is approximately unity, regardless the initial coverage Ɵ_T, even though the activation energy for the production of carbon dioxide varies with Ɵ_T. The desorption of water, which implies C-O bond cleavage of the formate, appears at approximately the same temperature as that of carbon dioxide. These observations suggest that the cleavage of the C-D bond and that of the C-O bond of two surface formates are coupled, possibly via the formation of a short-lived surface complex that is the precursor to to the decomposition.
The measurement of steady-state rate is demonstrated here to be valuable in determining kinetics associated with short-lived, molecularly adsorbed precursor to further reactions on the surface, by determining the kinetic parameters of the molecular precursor of formaldehyde to its dissociation on the Pt(110)-(1 x 2) surface.
Overlayers of nitrogen adatoms on Ru(001) have been characterized both by thermal desorption mass spectrometry and low-energy electron diffraction, as well as chemically via the postadsorption and desorption of ammonia and carbon monoxide.
The nitrogen-adatom overlayer was prepared by decomposing ammonia thermally on the surface at a pressure of 2.8 x 10^(-6) Torr and a temperature of 480 K. The saturated overlayer prepared under these conditions has associated with it a (√247/10 x √247/10)R22.7° LEED pattern, has two peaks in its thermal desorption spectrum, and has a fractional surface coverage of 0.40. Annealing the overlayer to approximately 535 K results in a rather sharp (√3 x √3)R30° LEED pattern with an associated fractional surface coverage of one-third. Annealing the overlayer further to 620 K results in the disappearance of the low-temperature thermal desorption peak and the appearance of a rather fuzzy p(2x2) LEED pattern with an associated fractional surface coverage of approximately one-fourth. In the low coverage limit, the presence of the (√3 x √3)R30° N overlayer alters the surface in such a way that the binding energy of ammonia is increased by 20% relative to the clean surface, whereas that of carbon monoxide is reduced by 15%.
A general methodology for the indirect relative determination of the absolute fractional surface coverages has been developed and was utilized to determine the saturation fractional coverage of hydrogen on Ru(001). Formaldehyde was employed as a bridge to lead us from the known reference point of the saturation fractional coverage of carbon monoxide to unknown reference point of the fractional coverage of hydrogen on Ru(001), which is then used to determine accurately the saturation fractional coverage of hydrogen. We find that ƟSAT/H = 1.02 (±0.05), i.e., the surface stoichiometry is Ru : H = 1 : 1. The relative nature of the method, which cancels systematic errors, together with the utilization of a glass envelope around the mass spectrometer, which reduces spurious contributions in the thermal desorption spectra, results in high accuracy in the determination of absolute fractional coverages.
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A excreção urinária de glicosaminoglicanos (GAG) está alterada em várias patologias do trato urinário; o padrão de excreção pode estar associado com o estado da doença. A excreção urinária de GAG em crianças com bexiga neurogênica (BN) secundária a mielomeningocele (MMC) pode também estar alterada, mas até a presente data não há detalhamento epidemiológico dos pacientes e não se correlacionou o padrão de excreção com grau de disfunção vesical. Analisamos a excreção urinária de um grupo bem definido de crianças com MMC e correlacionamos os resultados com escore cistométrico. As amostras de urina de 17 pacientes com MMC, 10 meninos e 7 meninas (média de idade DP de 4,6 2,9 anos) foram obtidas durante o exame cistométrico. As amostras do grupo controle foram obtidas de 18 crianças normais, 13 meninos e 5 meninas (6,9 2,2 anos). Todas as crianças não estavam com infecção urinária, tinham função renal normal e não estavam sob tratamento farmacológico. A quantificação do GAG urinário total foi expressa em μg de ácido hexurônico / mg de creatinina e a proporção dos diferentes tipos de GAGs sulfatados foi obtida por eletroforese em gel de agarose. A avaliação cistométrica foi realizada utilizando aparelho de urodinâmica Dynapack modelo MPX816 (Dynamed, São Paulo, Brasil), a partir da qual o escore cistométrico foi calculado de acordo com procedimento recente publicado. [14]. Não observamos diferença significativa na excreção urinária de GAG total entre meninos e meninas tanto no grupo com MMC ( 0,913 0,528 vs 0,867 0,434, p>0,05) como no grupo controle (0,546 0,240 vs 0,699 0,296, p>0,05). Os resultados mostraram também que a excreção de GAG urinário não se correlacionou com a idade tanto no grupo com MMC ( r = -0,28, p> 0,05) como no grupo controle (r = -0,40, p> 0,05). Entretanto, a comparação dos dois grupos mostrou que o grupo com MMC excretava 52% a mais de GAG total que o grupo controle (0,894 0,477 vs 0,588 0,257, p <0,04). Nesses pacientes a excreção de GAG total não se correlacionou com a complacência vesical isoladamente (r = -0,18, p> 0,05) mas foi significativa e negativamente correlacionada ao escore cistométrico (r= -0,56, p<0,05). Em média, os pacientes com piores escores (<9) excretaram 81% a mais de GAG que os pacientes com melhor escore (>9) (1,157 0,467 vs 0,639 0,133, p<0,04). O sulfato de condroitin foi o GAG sulfatado predominante nos grupos neurogênico e controles (92,5 7,6% vs 96,4 4,8%, respectivamente, p> 0,05), enquanto o sulfato do heparan estava presente em quantidades marcadamente menores; o dermatam sulfato não foi detectado. A excreção urinária de GAG em pacientes com MMC é significativamente maior que a excreção das crianças normais e os altos valores encontrados estão correlacionados a um maior compromentimento da função vesical. Evidências em modelos animais com MMC induzida sugerem que alterações no detrusor estão associadas a um elevado turnover da matriz extra celular (MEC) vesical, o que pode explicar a elevada excreção de GAG nos pacientes com MMC. Além disso, esses resultados indicam que a excreção urinária de GAG pode ser usada como fator adjuvante para a caracterização da disfunção vesical em pacientes com MMC.
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The influence upon the basic viscous flow about two axisymmetric bodies of (i) freestream turbulence level and (ii) the injection of small amounts of a drag-reducing polymer (Polyox WSR 301) into the test model boundary layer was investigated by the schlieren flow visualization technique. The changes in the type and occurrence of cavitation inception caused by the subsequent modifications in the viscous flow were studied. A nuclei counter using the holographic technique was built to monitor freestream nuclei populations and a few preliminary tests investigating the consequences of different populations on cavitation inception were carried out.
Both test models were observed to have a laminar separation over their respective test Reynolds number ranges. The separation on one test model was found to be insensitive to freestream turbulence levels of up to 3.75 percent. The second model was found to be very susceptible having its critical velocity reduced from 30 feet per second at a 0.04 percent turbulence level to 10 feet per second at a 3.75 percent turbulence level. Cavitation tests on both models at the lowest turbulence level showed the value of the incipient cavitation number and the type of cavitation were controlled by the presence of the laminar separation. Cavitation tests on the second model at 0.65 percent turbulence level showed no change in the inception index, but the appearance of the developed cavitation was altered.
The presence of Polyox in the boundary layer resulted in a cavitation suppression comparable to that found by other investigators. The elimination of the normally occurring laminar separation on these bodies by a polymer-induced instability in the laminar boundary layer was found to be responsible for the suppression of inception.
Freestream nuclei populations at test conditions were measured and it was found that if there were many freestream gas bubbles the normally present laminar separation was elminated and travelling bubble type cavitation occurred - the value of the inception index then depended upon the nuclei population. In cases where the laminar separation was present it was found that the value of the inception index was insensitive to the free stream nuclei populations.
Resumo:
O prolapso uterino tem sua incidência aumentada na pós-menopausa. O objetivo deste estudo é identificar as alterações na matriz extracelular do ligamento cardinal associadas à menopausa e ao prolapso uterino. Ligamento cardinal de três diferentes grupos de mulheres, pré-menopausa, prolapso uterino e pós-menopausa, foram identificados e biopsiados durante 57 histerectomias abdominais ou vaginais. As amostras foram processadas por métodos bioquímicos para caracterização e quantificação de glicosaminoglicanos sulfatados e colágeno. As concentrações relativas de glicosaminoglicanos foram obtidas por eletroforese. Procedimentos histológicos foram feitos para identificar fibras elásticas (Weigert), distribuição de colágeno (Picro Sirius) e decorin (imunohistoquímica). Nossos resultados mostraram aumento na concentração de GAG de 72,2%, redução na concentração de colágeno de 37% e diminuição de 22% de fibras elásticas no grupo de prolapso uterino quando comparado ao grupo da pós-menopausa (p<0,05, p<0,04 e p<0,05 respectivamente). As concentrações relativas de glicosaminoglicanos sulfatados para condroitin sulfato, heparan sulfato e dermatan sulfato não mostraram diferenças entre os três grupos. A organização do colágeno foi similar entre os três grupos e a marcação do decorin pareceu estar diminuída no grupo de prolapso uterino. Nossos resultados indicam alterações no metabolismo do tecido conjuntivo. O ligamento cardinal da mulher na pós-menopausa possui uma matriz extracelular mais densa. Esta alteração não ocorre na mulher com prolapso uterino.
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Red fluorescent proteins (RFPs) have attracted significant engineering focus because of the promise of near infrared fluorescent proteins, whose light penetrates biological tissue, and which would allow imaging inside of vertebrate animals. The RFP landscape, which numbers ~200 members, is mostly populated by engineered variants of four native RFPs, leaving the vast majority of native RFP biodiversity untouched. This is largely due to the fact that native RFPs are obligate tetramers, limiting their usefulness as fusion proteins. Monomerization has imposed critical costs on these evolved tetramers, however, as it has invariably led to loss of brightness, and often to many other adverse effects on the fluorescent properties of the derived monomeric variants. Here we have attempted to understand why monomerization has taken such a large toll on Anthozoa class RFPs, and to outline a clear strategy for their monomerization. We begin with a structural study of the far-red fluorescence of AQ143, one of the furthest red emitting RFPs. We then try to separate the problem of stable and bright fluorescence from the design of a soluble monomeric β-barrel surface by engineering a hybrid protein (DsRmCh) with an oligomeric parent that had been previously monomerized, DsRed, and a pre-stabilized monomeric core from mCherry. This allows us to use computational design to successfully design a stable, soluble, fluorescent monomer. Next we took HcRed, which is a previously unmonomerized RFP that has far-red fluorescence (λemission = 633 nm) and attempted to monomerize it making use of lessons learned from DsRmCh. We engineered two monomeric proteins by pre-stabilizing HcRed’s core, then monomerizing in stages, making use of computational design and directed evolution techniques such as error-prone mutagenesis and DNA shuffling. We call these proteins mGinger0.1 (λem = 637 nm / Φ = 0.02) and mGinger0.2 (λem = 631 nm Φ = 0.04). They are the furthest red first generation monomeric RFPs ever developed, are significantly thermostabilized, and add diversity to a small field of far-red monomeric FPs. We anticipate that the techniques we describe will be facilitate future RFP monomerization, and that further core optimization of the mGingers may allow significant improvements in brightness.
Resumo:
Part I
A study of the thermal reaction of water vapor and parts-per-million concentrations of nitrogen dioxide was carried out at ambient temperature and at atmospheric pressure. Nitric oxide and nitric acid vapor were the principal products. The initial rate of disappearance of nitrogen dioxide was first order with respect to water vapor and second order with respect to nitrogen dioxide. An initial third-order rate constant of 5.5 (± 0.29) x 104 liter2 mole-2 sec-1 was found at 25˚C. The rate of reaction decreased with increasing temperature. In the temperature range of 25˚C to 50˚C, an activation energy of -978 (± 20) calories was found.
The reaction did not go to completion. From measurements as the reaction approached equilibrium, the free energy of nitric acid vapor was calculated. This value was -18.58 (± 0.04) kilocalories at 25˚C.
The initial rate of reaction was unaffected by the presence of oxygen and was retarded by the presence of nitric oxide. There were no appreciable effects due to the surface of the reactor. Nitric oxide and nitrogen dioxide were monitored by gas chromatography during the reaction.
Part II
The air oxidation of nitric oxide, and the oxidation of nitric oxide in the presence of water vapor, were studied in a glass reactor at ambient temperatures and at atmospheric pressure. The concentration of nitric oxide was less than 100 parts-per-million. The concentration of nitrogen dioxide was monitored by gas chromatography during the reaction.
For the dry oxidation, the third-order rate constant was 1.46 (± 0.03) x 104 liter2 mole-2 sec-1 at 25˚C. The activation energy, obtained from measurements between 25˚C and 50˚C, was -1.197 (±0.02) kilocalories.
The presence of water vapor during the oxidation caused the formation of nitrous acid vapor when nitric oxide, nitrogen dioxide and water vapor combined. By measuring the difference between the concentrations of nitrogen dioxide during the wet and dry oxidations, the rate of formation of nitrous acid vapor was found. The third-order rate constant for the formation of nitrous acid vapor was equal to 1.5 (± 0.5) x 105 liter2 mole-2 sec-1 at 40˚C. The reaction rate did not change measurably when the temperature was increased to 50˚C. The formation of nitric acid vapor was prevented by keeping the concentration of nitrogen dioxide low.
Surface effects were appreciable for the wet tests. Below 35˚C, the rate of appearance of nitrogen dioxide increased with increasing surface. Above 40˚C, the effect of surface was small.
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An array of two spark chambers and six trays of plastic scintillation counters was used to search for unaccompanied fractionally charged particles in cosmic rays near sea level. No acceptable events were found with energy losses by ionization between 0.04 and 0.7 that of unit-charged minimum-ionizing particles. New 90%-confidence upper limits were thereby established for the fluxes of fractionally charged particles in cosmic rays, namely, (1.04 ± 0.07)x10-10 and (2.03 ± 0.16)x10-10 cm-2sr-1sec-1 for minimum-ionizing particles with charges 1/3 and 2/3, respectively.
In order to be certain that the spark chambers could have functioned for the low levels of ionization expected from particles with small fractional charges, tests were conducted to estimate the efficiency of the chambers as they had been used in this experiment. These tests showed that the spark-chamber system with the track-selection criteria used might have been over 99% efficient for the entire range of energy losses considered.
Lower limits were then obtained for the mass of a quark by considering the above flux limits and a particular model for the production of quarks in cosmic rays. In this model, which is one involving the multi-peripheral Regge hypothesis, the production cross section and a corresponding mass limit are critically dependent on the Regge trajectory assigned to a quark. If quarks are "elementary'' with a flat trajectory, the mass of a quark can be expected to be at least 6 ± 2 BeV/c2. If quarks have a trajectory with unit slope, just as the existing hadrons do, the mass of a quark might be as small as 1.3 ± 0.2 BeV/c2. For a trajectory with unit slope and a mass larger than a couple of BeV/c2, the production cross section may be so low that quarks might never be observed in nature.
Resumo:
The two lowest T = 3/2 levels in 21Na have been studied in the 19F(3He, n), 20Ne (p,p) and 20Ne (p,p’) reactions, and their excitation energies, spins, parities and widths have been determined. In a separate investigation, branching ratios were measured for the isospin-nonconserving particle decays of the lowest T = 3/2 levels in 17O and 17F to the ground state and first two excited states of 16O, by studying the 15N(3He,n) 17F*(p) 16O and 18O(3He, α)17O*(n) 16O reactions.
The 19F(3He,n) 21Na reaction was studied at incident energies between 4.2 and 5.9 MeV using a pulsed-beam neutron-time-of-flight spectrometer. Two T = 3/2 levels were identified at excitation energies of 8.99 ± 0.05 MeV (J > ½) and 9.22 ± 0.015 MeV (J π = ½+, Γ ˂ 40 keV). The spins and parities were determined by a comparison of the measured angular distributions with the results of DWBA calculations.
These two levels were also obsesrved as isospin-forbidden resonances in the 20Ne(p,p) and 20Ne(p,p’) reactions. Excitation energies were measured and spins, parities, and widths were determined from a single level dispersion theory analysis. The following results were obtained:
Ex = 8.973 ± 0.007 MeV, J π = 5/2 + or 3/2+, Γ ≤ 1.2 keV,
Γpo = 0.1 ± 0.05 keV; Ex = 9.217 ± 0.007 MeV, Jπ = ½ +,
Γ = 2.3 ± 0.5 keV, Γpo = 1.1 ± 0.3 keV.
Isospin assignments were made on the basis of excitation energies, spins, parities, and widths.
Branching ratios for the isospin-nonconserving proton decays of the 11.20 MeV, T = 3/2 level in 17F were measured by the 15N(3He,n) 17 F*(p) 16O reaction to be 0.088 ± 0.016 to the ground state of 16O and 0.22 ± 0.04 to the unresolved 6.05 and 6.13 MeV levels of 16O. Branching ratios for the neutron decays of the analogous T = 3/2 level, at 11.08 MeV in 17O, were measured by the 16O(3He, α)17O*(n)16O reaction to be 0.91 ± 0.15 to the ground state of 16O and 0.05 ± 0.02 to the unresolved 6.05 and 6.13 MeV states. By comparing the ratios of reduced widths for the mirror decays, the form of the isospin impurity in the T = 3/2 levels is shown to depend on Tz.
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This thesis is the culmination of field and laboratory studies aimed at assessing processes that affect the composition and distribution of atmospheric organic aerosol. An emphasis is placed on measurements conducted using compact and high-resolution Aerodyne Aerosol Mass Spectrometers (AMS). The first three chapters summarize results from aircraft campaigns designed to evaluate anthropogenic and biogenic impacts on marine aerosol and clouds off the coast of California. Subsequent chapters describe laboratory studies intended to evaluate gas and particle-phase mechanisms of organic aerosol oxidation.
The 2013 Nucleation in California Experiment (NiCE) was a campaign designed to study environments impacted by nucleated and/or freshly formed aerosol particles. Terrestrial biogenic aerosol with > 85% organic mass was observed to reside in the free troposphere above marine stratocumulus. This biogenic organic aerosol (BOA) originated from the Northwestern United States and was transported to the marine atmosphere during periodic cloud-clearing events. Spectra recorded by a cloud condensation nuclei counter demonstrated that BOA is CCN active. BOA enhancements at latitudes north of San Francisco, CA coincided with enhanced cloud water concentrations of organic species such as acetate and formate.
Airborne measurements conducted during the 2011 Eastern Pacific Emitted Aerosol Cloud Experiment (E-PEACE) were aimed at evaluating the contribution of ship emissions to the properties of marine aerosol and clouds off the coast of central California. In one study, analysis of organic aerosol mass spectra during periods of enhanced shipping activity yielded unique tracers indicative of cloud-processed ship emissions (m/z 42 and 99). The variation of their organic fraction (f42 and f99) was found to coincide with periods of heavy (f42 > 0.15; f99 > 0.04), moderate (0.05 < f42 < 0.15; 0.01 < f99 < 0.04), and negligible (f42 < 0.05; f99 < 0.01) ship influence. Application of these conditions to all measurements conducted during E-PEACE demonstrated that a large fraction of cloud droplet (72%) and dry aerosol mass (12%) sampled in the California coastal study region was heavily or moderately influenced by ship emissions. Another study investigated the chemical and physical evolution of a controlled organic plume emitted from the R/V Point Sur. Under sunny conditions, nucleated particles composed of oxidized organic compounds contributed nearly an order of magnitude more cloud condensation nuclei (CCN) than less oxidized particles formed under cloudy conditions. The processing time necessary for particles to become CCN active was short ( < 1 hr) compared to the time needed for particles to become hygroscopic at sub-saturated humidity ( > 4 hr).
Laboratory chamber experiments were also conducted to evaluate particle-phase processes influencing aerosol phase and composition. In one study, ammonium sulfate seed was coated with a layer of secondary organic aerosol (SOA) from toluene oxidation followed by a layer of SOA from α-pinene oxidation. The system exhibited different evaporative properties than ammonium sulfate seed initially coated with α-pinene SOA followed by a layer of toluene SOA. This behavior is consistent with a shell-and-core model and suggests limited mixing among different SOA types. Another study investigated the reactive uptake of isoprene epoxy diols (IEPOX) onto non-acidified aerosol. It was demonstrated that particle acidity has limited influence on organic aerosol formation onto ammonium sulfate seed, and that the chemical system is limited by the availability of nucleophiles such as sulfate.
Flow tube experiments were conducted to examine the role of iron in the reactive uptake and chemical oxidation of glycolaldehyde. Aerosol particles doped with iron and hydrogen peroxide were mixed with gas-phase glycolaldehyde and photochemically aged in a custom-built flow reactor. Compared to particles free of iron, iron-doped aerosols significantly enhanced the oxygen to carbon (O/C) ratio of accumulated organic mass. The primary oxidation mechanism is suggested to be a combination of Fenton and photo-Fenton reactions which enhance particle-phase OH radical concentrations.
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The Mössbauer technique has been used to study the nuclear hyperfine interactions and lifetimes in W182 (2+ state) and W183 (3/2- and 5/2- states) with the following results: g(5/2-)/g(2+) = 1.40 ± 0.04; g(3/2- = -0.07 ± 0.07; Q(5/2-)/Q(2+) = 0.94 ± 0.04; T1/2(3/2-) = 0.184 ± 0.005 nsec; T1/2(5/2-) >̰ 0.7 nsec. These quantities are discussed in terms of a rotation-particle interaction in W183 due to Coriolis coupling. From the measured quantities and additional information on γ-ray transition intensities magnetic single-particle matrix elements are derived. It is inferred from these that the two effective g-factors, resulting from the Nilsson-model calculation of the single-particle matrix elements for the spin operators ŝz and ŝ+, are not equal, consistent with a proposal of Bochnacki and Ogaza.
The internal magnetic fields at the tungsten nucleus were determined for substitutional solid solutions of tungsten in iron, cobalt, and nickel. With g(2+) = 0.24 the results are: |Heff(W-Fe)| = 715 ± 10 kG; |Heff(W-Co)| = 360 ± 10 kG; |Heff(W-Ni)| = 90 ± 25 kG. The electric field gradients at the tungsten nucleus were determined for WS2 and WO3. With Q(2+) = -1.81b the results are: for WS2, eq = -(1.86 ± 0.05) 1018 V/cm2; for WO3, eq = (1.54 ± 0.04) 1018 V/cm2 and ƞ = 0.63 ± 0.02.
The 5/2- state of Pt195 has also been studied with the Mössbauer technique, and the g-factor of this state has been determined to be -0.41 ± 0.03. The following magnetic fields at the Pt nucleus were found: in an Fe lattice, 1.19 ± 0.04 MG; in a Co lattice, 0.86 ± 0.03 MG; and in a Ni lattice, 0.36 ± 0.04 MG. Isomeric shifts have been detected in a number of compounds and alloys and have been interpreted to imply that the mean square radius of the Pt195 nucleus in the first-excited state is smaller than in the ground state.
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Os aminoácidos L-arginina e L-glutamina foram analisados como protetores dos tecidos erétil do pênis contra os danos induzidos pela radiação. Grupos de ratos Wistar foram tratadas com: nenhuma intervenção, radiação pélvica e sacrifício 7 (RAD7) ou 15 (RAD15) dias; e radiação pélvica, a suplementação diária com L-arginina (A) ou L-glutamina (G), e sacrifício 7 (RAD7 + A, RAD7 + G) ou 15 (RAD15 + A, RAD15 + G) dias após irradiação. componentes estruturais do corpo cavernoso (CC), túnica albugínea do corpo esponjoso (TAC), e urotélio do pênis foram analisados através de métodos estereológicos e imuno-histoquímico. Os resultados mostraram que, no CC, o tecido conjuntivo foi maior nos RAD15 (p <0,04), mas essa mudança foi parcialmente revertido em RAD15 + G (p <0,05) e RAD15 + A (p <0,04). A matriz fibrosa das trabéculas CC estava manchada de colágeno tipo I. Nos RAD15, a intensidade da marcação foi aumentada, enquanto que em RAD15 + G + A e RAD15 a coloração era semelhante à dos controles. Nenhuma alteração de coloração foram observadas nos grupos que foram sacrificados sete dias após a radiação. Cavernosa teor de fibras elásticas na RAD15 foi aumentada (p <0,004), e este foi impedido de RAD15 + A (p <0,004), mas não em RAD15 + G. No TAC, os aminoácidos protegidos (p <0,02) contra o aumento da radiação induzida em fibras elásticas, mas apenas em RAD15. Densidade das células do urotélio e espessura urothellial, foram reduzidos em RAD15 (p <0,004), mas houve efeitos protetores dos dois aminoácidos. Em conclusão, a radiação induzida por alterações nas estruturas penianas tendem a ser mais pronunciado 15 dias após a sessão de radiação. Tanto A e G têm efeitos protetores contra estas alterações, sendo o primeiro um pouco mais eficaz.
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O objetivo deste estudo foi verificar se o tratamento periodontal não cirúrgico exercia alguma influência sobre o perfil lipídico, os elementos celulares das séries banca e vermelha do sangue, plaquetas e VHS de pacientes portadores de periodontite crônica generalizada. Dezoito pacientes, com média de idade de 50,6 anos ( 7,6), foram submetidos, previamente ao tratamento periodontal e 30 dias após o mesmo, à coleta de 10ml de sangue periférico, através do qual foram analisados o perfil lipídico, os elementos celulares das séries branca e vermelha, o número de plaquetas e VHS. Destes 18 pacientes, 7, com média de idade de 47,4 anos ( 5,9) também foram reavaliados 90 dias após o término do tratamento. Os parâmetros clínicos utilizados, previamente ao tratamento e nas reavaliações, foram o Índice de Placa (IP), de Silness e Löe (1964), o Índice Gengival (IG), de Löe (1967), Sangramento na Sondagem (SS), Profundidade de Bolsa à Sondagem (PBS) e Nível de Inserção (NI). Foram ainda registrados e classificados os sítios com envolvimento de furca. O tratamento periodontal consistiu de terapia básica não cirúrgica. Após 30 dias do término do tratamento periodontal todos os pacientes foram reavaliados sendo verificada melhora significativa (P<0,05) dos valores de IP, IG, SS e PBS e de NI ≥ 6mm (P=0,05). Sítios com envolvimento de furca classes II e III apresentaram também diminuição significativa (P=0,01). Os 7 pacientes submetidos às reavaliações de 30 e 90 dias pós-tratamento também mostraram melhora significativa (P<0,05) dos valores de IP, IG, SS e PBS entre estas fases. Já o NI entre 4-5mm aumentou de forma significativa (P=0,04) entre o pré-tratamento e 90 dias após o mesmo, enquanto que o NI ≥ 6mm diminui significativamente entre as reavaliações de 30 e 90 dias (P=0,01 e P=0,02, respectivamente). Quando comparados os valores de 30 com os de 90 dias resultados semelhantes aos supracitados foram observados, inclusive o aumento do NI entre 4-5mm (P=0,02). É verificado também entre estas fases um IG aumentado (P=0,07). Quanto aos valores hematológicos ocorreu uma diminuição significativa dos níveis de bastões (P=0,05) e de monócitos (P=0,03) após o tratamento periodontal (30 dias), enquanto que o colesterol total e o LDL apresentaram uma tendência ao aumento (P=0,09 para ambos). Já nos sete pacientes submetidos às duas reavaliações o colesterol total apresentou aumento significativo entre as fases pré-tratamento, 30 (P=0,04) e 90 dias (P=0,02) após terapia, assim como o LDL (P=0,04 e P=0,03, respectivamente). Quando comparados os valores plaquetários entre as fases 30 e 90 dias pós-tratamento, verifica-se uma tendência a sua diminuição (P=0,09). O Índice de Castelli II (relação colesterol/HDL) apresenta entre as fases pré e 30 dias pós-tratamento tendência a aumento (P=0,09). Através desses resultados é possível concluir que o tratamento periodontal exerceu influência sobre bastões e monócitos do sangue, caracterizada pela diminuição dessas células, e sobre o colesterol total e o LDL, representada pelo aumento de seus valores.