PubMed Health⌕ Search

SEARCH · PubMed Health

Results for “ATMOSPHERE”

Explore indexed PubMed citations for clinical trials, systematic reviews and public health research. Read source abstracts and follow each citation to its original PubMed record.

Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.

At least 1,081 records · Page 60Linked to original sources

On living in an arsenical atmosphere (Part 2). Clinical observations, animal experiments and ecological problems.

Humans and other animals living in an arsenic polluted atmosphere appear to absorb very little through their lungs, but absorb a varying quantity through the gut. A measure of human absorbtion is reflected in that excreted in the urine, but the amount excreted correlates poorly with clinical toxicity. Symptoms of toxicity my exist at as low a level as 0.25 ppm, with clearing of the problems when the patient is treated with BAL. On the other hand, people excreting well over 1 ppm may be free of any symptoms or signs. There is an indication that arsenic does not pass from the human mother for foetus or infant, either through the placenta or through the milk. Experimental animals living in an arsenical atmosphere thrive if fed uncontaminated food, but die rapidly if fed herbage gleaned from the contaminated area. The countryside subtended by atmospheric arsenical pollution becomes seriously ecologically down graded, with high arsenic levels in soil and on foliage. Most of the flora fail to thrive, while there is virtual disappearance of the natural fauna. Once the pollution has ceased, it would appear that the arsenic is rapidly leached away, with a return to ecological normality this recovery was surprisingly rapid and complete. There is statutory provision for closure of polluting industry. Indecision, unwillingness to cut off a source of national wealth, the question of employment, and an apparent lack of serious human toxicity allowed the continuation of the mining and roasting operation until the exhaustion of a payable orebody.

Adult↗

[Atmospheric radiations. Effects of potassium-inhibitory and potassium-retentive hormones on two types of infective agent].

The glucocorticoids and the estrogens facilitate the loss of potassium from the cells (iK+ hormones). The thyroid hormones, the androgens, the growth hormone and the insulin facilitate the penetration of potassium into the cells (rK+ hormones). The incretion of iK+ hormones follows the course of the intensity of the atmospheric radiations (atmospheric electric field, terrestrial magnetic field), that is it grows or diminishes according to the increase or decrease of the intensity of said radiations, while the incretion of rK+ hormones has an opposite course in comparison with the variations of said intensity. The iK+ hormones cause loss of iodine, decrease of eosinophils, of RNA and antibodies, while the rK+ hormones cause opposite effects. High temperatures produce an increase of iK+ hormones and low temperatures an increase of rK+ hormones. The study of the effects of atmospheric radiations on infectious diseases has shown the existence of two kind of infectious agents: the iK+ agents and the rK+ agents on which the hormones iK+ and rK+ have an effect. The hormones iK+ work jointly with iK+ agents (virus RNA, bacteria Gram-negative) and counteract the rK+ agents (virus DNA, bacteria Gram-positive, protozoa). The rK+ hormones have opposite effects in comparison to those of iK+ hormones, that is they counteract the iK+ agents and work jointly with the rK+ agents.

Background Radiation↗

[Nursery-acquired diseases and quality of the atmosphere ].

A comparative study of the diseases and the physicochemical and bacteriological properties of the atmosphere was performed in 4 nurseries in Paris between September 1976 and June 1977. The importance of nursery-acquired diseases was estimated in each child from the average of the days of non attendance because of illness. They were classified in 3 groups: upper and lower respiratory tract, gastro-intestinal, infection-eruption whose respective rates (80%, 10% and 10%) are not significantly different either from one nursery to another or with age. The children under 2 years of age are ill twice more frequently than the older ones (p less than 0.001). The duration of the absences for illness differs from one nursery to another (p less than 0.001). In the 2 nurseries where the thermohygrometric comfort is satisfying in 30% or more controls (temperature between 19 and 22 degrees C with hygrometry between 40 and 60% of relative humidity), the average of non attendance for ill;ness is 6.0 days; in the 2 nurseries where the comfort is satisfying in 20% of the cases or less, this average becomes 12.6 days in dry and globally contaminated atmosphere and 18.5 days in super-heated atmosphere where pathogen staphylococci predominate.

Air Microbiology↗

[Behaviour of gram-positive and gram-negative bacteria in dry and moist atmosphere (author's transl)].

The results of bacteriologic environmental studies show the frequently appearance of Staphylococci in dry and of Pseudomonas in moist atmosphere. There is a small frequency of Enterobacteriaceae in both cases. Therefore experiments are done about the behaviour in dry atmosphere of 5 different strains of Staph. aureus, Strept. faecalis, E. coli, Kl. pneumoniae, S. marcescens and P. aeruginosa. The bacterial suspensions are scored on aluminium foil and exposed at room temperature and constant air-moisture. The results show Enterobacteriaceae more sensitive for drying as Staph. aureus and Strept. faecalis. In dry atmosphere Pseudomonas is nearly not able to survive. In contrary to the other examined bacteria only Staphylococcus can be transfered by air or dust. The behaviour in moist environment is examined at room temperature in aqua bidest. and sterile tap-water. In both liquids only S. marcescens is able to grow. It is conspicous that P. aeruginosa dies off in aqua bidest, within 4 d while it is able to grow in tap-water. In tap-water the initial colony count of E. coli keeps constant, but in aqua bidest. E. coli is no more present after 24 d. In both liquids, Staph. aureus and Strept. faecalis have limited surviving rates: Staph. aureus can't be cultured in aqua bidest, after 5 d, in tap-water after 7 d, Strept. faecalis survive 11 and 10 d respectively. Additional the behaviour in tap-water is examined at 30 degrees C and 40 degrees C. These temperatures are characteristic for ultrasonic nebulizers and humidifiers respectively. At both temperatures only P. aeruginosa is able to grow. The other bacteria--including S. marcesens--die off at 30 degrees C and even faster at 40 degrees C. Furthermore mixed cultures are made with 5 strains each of Staph. aureus (= St), Strept. faecalis (= Sf), E. coli (= Ec), S. marcescens (= Se) and P. aeruginosa (= Pa) which formed the following groups: St/Sf, St/Ec, St/Se, St/Pa, Sf/Ec, Sf/Se, Sf/Pa, Ec/Se, Ec/Pa, Se/Pa. The examinations are done in aqua bidest. and tap-water at room temperature. Additional the behaviour in tap-water at 30 degrees C and 40 degrees C was tested. A mutual influence cannot be found. It is the conclusion to use the humidifiers and nebulizers with sterile aqua bidest. only and to prefer the humidifiers to the nebulizers.

Air Microbiology↗

Effects of atmospheric ammonia on young pigs experimentally infected with Ascaris suum.

Effects of atmospheric ammonia at 69.4 mg/m3 (100 ppm) on productive performance and respiratory tract health of young pigs (starting body weight averaged 7.5 kg) experimentally infected with Ascaris suum (50,000 embryonated ova administered by gavage when pigs were 5 weeks of age) were studied in 5 trials of 4 weeks each (when pigs were 5 to 9 weeks of age). Effects of atmospheric-ammonia exposure and ascarid infection on growth were additive. Compared with controls, percentage reductions in average daily gain were 32%, 28%, and 61% for ammonia-exposed, ascarid-infected, and combined ammonia plus ascarid groups, respectively. Ammonia exposure or ascarid infection alone depressed feed disappearance by 18%. Effects of the 2 factors were additive, resulting in a 35% reduction in feed disappearance. Pigs exposed to the combined factors had an average gain/feed ratio of 0.518, which was less than that of control pigs (0.546), but was greater than that of pigs exposed to atmospheric ammonia (0.489) or pigs infected with ascarids (0.501) alone. Liver scarring, due to larval migration, was not affected by ammonia exposure. Larval migration through the respiratory tract was not confirmed histopathologically in pigs killed 4 weeks after inoculation. A supplementary experiment was conducted which demonstrated that residual evidence of previous pulmonary larval migration was present 2 weeks after inoculation.

Air Pollutants↗

Relationships between mean lead levels in the atmosphere and in blood from data published since 1977.

The authors attempted to confirm the reliability of the linear log-log model presented by Goldsmith and Hexter in 1967. The data used were from seven reports published since 1977, including that of the authors. The age of the subjects in these reports ranged from three to over 65 years. Various methods of air sampling and pre-treatment of collected particulate matter were employed. Lead was determined by atomic absorption spectrophotometry. The mean value of lead in the atmosphere ranged from 0.11 to 19 micrograms/m3. A regression line obtained from 13 pairs of averaged lead in the atmosphere and in blood was log(Pb-B) = 0.259 x log(Pb-A) + .243, and the Pearson's moment correlation coefficient between the logarithm of Pb-A and the logarithm of Pb-B was 0.839. These results were roughly the same as those of Goldsmith. This finding confirms the consistency of the association between Pb-A and Pb-B, which may be used to monitor atmospheric and blood lead quantitatively in those countries conducting a lead reduction program in gasoline.

Air Pollutants↗

Annual, daily and diurnal variations in pollen from Olea europaea L. in the atmosphere of Granada (Spain).

The allergenic capacity of Olea europaea L. pollen is very important in several cities of the southern Iberian Peninsula, producing most pollinoses diagnosed in these cities. We have carried out a study on the annual, daily and diurnal variations in pollen from O. europaea in the atmosphere of Granada (Spain) during 4 consecutive years. Samplings were carried out with the aid of a Burkard spore trap. Very low levels of Olea pollen grains were first detected in the atmosphere from the end of April. Pollen levels peaked in May and June, and started to decrease from the last days of June and in July. Pollen in the atmosphere is related to meteorological parameters: temperature has a positive influence on pollinization and rainfall produces a negative effect. The diurnal variation pattern of pollen grain concentrations was quite homogeneous throughout the study, featuring an important increase around midday and a moderate decrease in the first hours of the morning and in the late evening.

Air Pollution↗

[Susceptible populations and urban atmospheric pollution. Development of a policy of protection].

The short term vulnerability of sections of the population to the harmful effects of chemical pollutants in the urban atmosphere represents an important unresolved problem of public health. These groups include young children, the elderly, asthmatic patients, and patients with chronic bronchitis and cardio-respiratory insufficiency. A recently ratified French law on air and rational energy use is aimed at resolving this problem in the context of recognizing that everybody has a right to breathe air which is not damaging to their health. In order to achieve this objective and direct the measures to be taken to reduce the emission of pollutants relating to industrial activity, to heating and to road traffic, the law provides for an extension to the chain of automatic registering stations which enable the recording of atmospheric data in large urban centers. It also defines the limits of substances allowed in the air over given periods and revises the critical levels of particulate and gaseous pollutants allowed according to current experimental and epidemiological data. Thresholds for information and for alerting the population will also be defined, with eventually restrictive measures for industry and for car traffic envisaged. These provisions are a major step for the protection of susceptible populations and should be enhanced in the near future by extension to cover other potentially noxious substances. This requires continued study on the short and long term effects of atmospheric pollution on people's health.

Air Pollution↗

[Exposure of inhabitants of Poznan to fluorides. I. Fluorides in atmospheric air, tap water and selected additional fluids].

The purpose of the study was to obtain information about fluoride pollution of the human environment. Fluoride concentrations were measured in atmospheric air, water and certain drinks. The measurements were done with a ion-selective electrode. In the atmospheric air of Poznań and its environs the concentrations ranged from 0.0006 mg/m3 to 0.0122 mg/m3. Tap water in Poznań contained 0.2 mg F3/dm3, on average. The selected drinks--mineral water and tea contained 0.3 and 1.5 mg F-/dm3 respectively. The acceptable values of fluoride concentrations were not exceeded, but fluoride concentration in atmospheric air was higher than that found usually in other regions of the country. In drinking water fluoride concentration in Murowana Goślina was within the acceptable range, and in Poznań it was twice lower.

Air Pollutants↗

Atmospheric pollution originating from the interaction of different gaseous effluents.

During the last few years, several episodes of atmospheric pollution have been reported in a limited area near Guidonia, Rome. The area contains a disposal plant, Inviolata, for the collection of municipal solid waste (MSW) and a famous thermal water resort, the Acque Albule spring, which is a source of water rich in H2S. We conducted a multiparametric study in the areas surrounding the solid waste disposal plant and the Acque Albule spring. The concentration of main gaseous effluent was continuously monitored over a period of 4 months and the data relating to the meteorologic conditions in the area during the last few decades were examined. Our results suggest that most of the atmospheric pollution is due to the interaction of different gaseous effluents. Specifically, the presence of relatively high levels of hydrogen sulfide in the atmosphere, constantly released in large amounts by the Acque Albule springs, and of biogases (mainly hydrocarbons) from the organic matter present in the solid waste continuously unloaded and stored at the disposal plant, lead to mixing and photochemical interactions between these chemical compounds, which in turn are responsible for most of the polluting effects. Such interactions are promoted by the strong solar irradiation in the area that is enhanced by the peculiar local meteorological features that do not allow the pollutants to disperse.

Air Pollutants↗

Response of vehicular lead to the presence of street dust in the atmospheric environment of major roads.

Size fractionated particulate samples were collected from the roadside atmosphere of three major roads within the Brisbane Metropolitan area, using a high volume sampler fitted with an Anderson impactor. Street dusts were also sampled at these sites. Deposition samples were collected simultaneously with those of atmospheric particulates from periods with and without rainfall. All types of samples were quantitatively analysed for lead and various anions and cations. The pH and electrical conductivity for street dusts and deposition samples together with total solids content of deposition samples were also determined. Results showed that at sites where the process of street dust resuspension was at a minimum, the bromide-to-lead ratios were comparable to the reported ratio in uncombusted petrol. However, the relatively higher bromide-to-lead ratios observed at sites with active street dust resuspension indicate the existence of a process by which fine lead particulates are removed from the atmosphere by resuspended coarse dust particles.

Air Pollution↗

Calculation of radiation fields in the atmosphere and comparison to experimental data.

In this paper the spectra of secondary hadrons are determined in the atmosphere at various depths down to sea level. The calculations are performed using the Monte Carlo code FLUKA together with cosmic-ray environmental models which describe the spectra of primary cosmic-ray particles. We discuss the details of the calculations and the dependence of the results on the primary cosmic-ray spectrum, the atmospheric depth and the geographical location. Special emphasis is put on comparisons of calculated and measured hadron spectra including an experiment which was recently performed at the mountain Zugspitze (47.4 degrees N, 11.0 degrees E, 2963 m), Germany. It is shown that FLUKA may serve as an important tool for the estimation of the radiation environment in the atmosphere.

Cosmic Radiation↗

[Morphological features of the nasal mucosa in healthy children exposed to different concentrations of atmospheric pollution].

OBJECTIVE: During the last decades the impact of pollution in big cities on the upper respiratory tract of children has become an issue of interest. The purpose of the present study was to determine if exposure of healthy children to different concentrations of atmospheric pollution alters morphologically the nasal respiratory epithelium. MATERIAL AND METHODS: In this randomised, prospective, open clinical trial we included 71 healthy children matched for age and sex and divided them into 3 groups: Group I, 31 children from Mexico City. Group II, 21 children from Tula, Hidalgo a moderate polluted area, and Group III, 19 children from Contepec, Michoacán, a rural non-polluted area. We took a nasal biopsy from the lower turbinate and performed nasal cytology in all children. The samples were examined twice by a pathologist with a double-blind technique. Ozone measurements were taken during 1992. RESULTS: Nasal symptoms (nasal obstruction, pruritus and dryness) were present in 96.8%, 71.4% and 52.6% of patients in groups I, II and III respectively (p = 0.001). We also found bilateral hypertrophy turbinates in 100% of children in group I versus 81% and 73% in groups II and III (p = 0.009). Citologic examination disclosed no significant differences among the study groups, although p values were 0.06 respecting inflammation and abnormal goblet cells when we compared group I versus group II and III. Respecting histological examination we found significant differences when comparing group I versus II and III in squamous metaplasia (p = 0.02) and pseudoepitheliomatous hyperplasia (p = 0.003), with not significant differences among keratinization (p = 0.06) and dysplasia (p = 0.06). CONCLUSIONS: The results of this study indicate that exposure to a polluted atmosphere is followed by severe changes in the histology and cytology of the nasal mucosa in healthy children, with these changes being more frequent and severe in the more polluted areas. These findings implicate that we must put more attention on the long term effects of atmospheric pollution in order to establish stronger control measures.

Adolescent↗

[The mutagenicity of the gas component of the atmosphere as an index of its quality].

Using an Ames proximate method with a metabolic activation, the authors could investigate the capacity of chemical substances complex extracted from the samples of the atmospheric air gas components of some industrial Ukrainian cities to induce genes' mutation at TA 98 and TA 100. It was shown that air samples extracted in the cities with predominantly developed metallurgical industry had induced the mutagenic effect of "medium" power; the atmospheric air of the cities with predominantly developed chemical industry had induced both "medium" and "weak" mutagenic effects; the atmospheric air of relatively "clean" cities either had not induced mutagenic effects or had induced "weak" effects. State of the system of metabolic activation was mainly uneffective.

Air↗

Incidence of Alternaria spores in the atmosphere of Murcia (SE Spain). Seasonal, monthly and intradiurnal variations.

Variation in Alternaria spores in the atmosphere of Murcia (SE Spain) were studied for 2 years. Using a Burkard volumetric sampler located about 19 m above ground level, spores were collected and counted hourly by light microscopy. The results suggest that species of Alternaria are present in the atmosphere of Murcia every day throughout the year. Mean daily concentration of Alternaria was 25 spores/m3. Seasonal variations showed the lowest concentrations during winter and the highest in autumn. In the monthly pattern two peaks were observed every year: the first in about May-June and the second occurring in October. In the intradiurnal variations, maximum concentrations were observed between 5:00-6:00 p.m. (Spanish official time). The variation of Alternaria spores in the atmosphere in Murcia seems to be related to different factors throughout the year.

Air Microbiology↗

Thermal structure of Uranus' atmosphere.

Application of a radiative-convective equilibrium model to the thermal structure of Uranus' atmosphere evaluates the role of hazes in the planet's stratospheric energy budget and places a lower limit on the internal energy flux. The model is constrained by Voyager and post-Voyager observations of the vertical aerosol and radiative active gas profiles. Our baseline model generally reproduces the observed tropospheric and stratospheric temperature profile. However, as in past studies, the model stratosphere from about 10(-3) to 10(-1) bar is too cold. We find that the observed stratospheric hazes do not warm this region appreciably and that any postulated hazes capable of warming the stratosphere sufficiently are inconsistent with Voyager and ground-based constraints. We explore the roles played by the stratospheric methane abundance, the H2 pressure-induced opacity, photochemical hazes, and C2H2, and C2H6 in controlling the temperature structure in this region. Assuming a vertical methane abundance profile consistent with that found by the Voyager UVS occultation observations, the model upper stratosphere, from 10 to 100 microbar, is also too cold. Radiation in the 7.8-micrometers band from a small abundance of hot methane in the lower thermosphere absorbed in this region can warm the atmosphere and bring models into closer agreement with observations. Finally, we find that internal heat fluxes < or approximately 60 erg cm-2 sec-1 are inconsistent with the observed tropospheric temperature profile.

Acetylene↗

Solid organic matter in the atmosphere and on the surface of outer Solar System bodies.

Many bodies in the outer Solar System display the presence of low albedo materials. These materials, evident on the surface of asteroids, comets, Kuiper Belt objects and their intermediate evolutionary step, Centaurs, are related to macromolecular carbon bearing materials such as polycyclic aromatic hydrocarbons and organic materials such as methanol and related light hydrocarbons, embedded in a dark, refractory, photoprocessed matrix. Many planetary rings and satellites around the outer gaseous planets display such component materials. One example, Saturn's largest satellite, Titan, whose atmosphere is comprised of around 90% molecular nitrogen N2 and less than 10% methane CH4, displays this kind of low reflectivity material in its atmospheric haze. These materials were first recorded during the Voyager 1 and 2 flybys of Titan and showed up as an optically thick pinkish orange haze layer. These materials are broadly classified into a chemical group whose laboratory analogs are termed "tholins", after the Greek word for "muddy". Their analogs are produced in the laboratory via the irradiation of gas mixtures and ice mixtures by radiation simulating Solar ultraviolet (UV) photons or keV charged particles simulating particles trapped in Saturn's magnetosphere. Fair analogs of Titan tholin are produced by bombarding a 9:1 mixture of N2:CH4 with charged particles and its match to observations of both the spectrum and scattering properties of the Titan haze is very good over a wide range of wavelengths. In this paper, we describe the historical background of laboratory research on this kind of organic matter and how our laboratory investigations of Titan tholin compare. We comment on the probable existence of polycyclic aromatic hydrocarbons in the Titan Haze and how biological and nonbiological racemic amino acids produced from the acid hydrolysis of Titan tholins make these complex organic compounds prime candidates in the evolution of terrestrial life and extraterrestrial life in our own Solar System and beyond. Finally, we also compare the spectrum and scattering properties of our resulting tholin mixtures with those observed on Centaur 5145 Pholus and the dark hemisphere of Saturn's satellite Iapetus in order to demonstrate the widespread distribution of similar organics throughout the Solar System.

Ammonia↗

Germination and growth of lettuce (Lactuca sativa) at low atmospheric pressure.

The response of lettuce (Lactuca sativa L. cv. Waldmann's Green) to low atmospheric pressure was examined during the initial 5 days of germination and emergence, and also during subsequent growth to vegetative maturity at 30 days. Growth took place inside a 66-l-volume low pressure chamber maintained at 70 kPa, and plant response was compared to that of plants in a second, matching chamber that was at ambient pressure (approximately 101 kPa) as a control. In other experiments, to determine short-term effects of low pressure transients, plants were grown at ambient pressure until maturity and then subjected to alternating periods of 24 h of low and ambient atmospheric pressures. In all treatments the partial pressure of O2 was maintained at 21 kPa (approximately the partial pressure in air at normal pressure), and the partial pressure of CO2 was in the range 66.5-73.5 Pa (about twice that in normal air) in both chambers, with the addition of CO2 during the light phase. With continuous exposure to low pressure, shoot and root growth was at least as rapid as at ambient pressure, with an overall trend towards slightly greater performance at the lower pressure. Dark respiration rates were greater at low pressure. Transient periods at low pressure decreased transpiration and increased dark respiration but only during the period of exposure to low pressure. We conclude that long-term or short-term exposure to subambient pressure (70 kPa) was without detectable detriment to vegetative growth and development.

Atmosphere Exposure Chambers↗