Determination and Evaluation of Alternative Methods for Managing and Controlling Highway-Related Dust Phase II—Demonstration Project, June 2005

The State of Iowa currently has approximately 69,000 miles of unpaved secondary roads. Due to the low traffic count on these unpaved o nts as ng e two dust ed d roads, paving with asphalt or Portland cement concrete is not economical. Therefore to reduce dust production, the use of dust suppressants has been utilized for decades. This study was conducted to evaluate the effectiveness of several widely used dust suppressants through quantitative field testing on two of Iowa’s most widely used secondary road surface treatments: crushed limestone rock and alluvial sand/gravel. These commercially available dust suppressants included: lignin sulfonate, calcium chloride, and soybean oil soapstock. These suppressants were applied to 1000 ft test sections on four unpaved roads in Story County, Iowa. Tduplicate field conditions, the suppressants were applied as a surface spray once in early June and again in late August or early September. The four unpaved roads included two with crushed limestone rock and two with alluvial sand/gravel surface treatmewell as high and low traffic counts. The effectiveness of the dust suppressants was evaluated by comparing the dust produced on treated and untreated test sections. Dust collection was scheduled for 1, 2, 4, 6, and 8 weeks after each application, for a total testiperiod of 16 weeks. Results of a cost analysis between annual dust suppressant application and biennial aggregate replacement indicated that the cost of the dust suppressant, its transportation, and application were relatively high when compared to that of thaggregate types. Therefore, the biennial aggregate replacement is considered more economical than annual dust suppressant application, although the application of annual dust suppressant reduced the cost of road maintenance by 75 %. Results of thecollection indicated that the lignin sulfonate suppressant outperformed calcium chloride and soybean oil soapstock on all four unpavroads, the effect of the suppressants on the alluvial sand/gravel surface treatment was less than that on the crushed limestone rock, the residual effects of all the products seem reasonably well after blading, and the combination of alluvial sand/gravel surface treatment anhigh traffic count caused dust reduction to decrease dramatically.

Grain size distribution and bulk chemistry of eolian dust

Atmospheric dust samples collected along a transect off the West African coast have been investigated for their physical (grain-size distribution), mineralogical, and chemical (major elements) composition. On the basis of these data the samples were grouped into sets of samples that most likely originated from the same source area. In addition, shipboard-collected atmospheric meteorological data, modeled 4-day back trajectories for each sampling day and location, and Total Ozone Mapping Spectrometer aerosol index data for the time period of dust collection (February-March 1998) were combined and used to reconstruct the sources of the groups of dust samples. On the basis of these data we were able to determine the provenance of the various dust samples. It appears that the bulk of the wind-blown sediments that are deposited in the proximal equatorial Atlantic Ocean are transported in the lower level (>~900 hPa) NE trade wind layer, which is a very dominant feature north of the Intertropical Convergence Zone (ITCZ). However, south of the surface expression of the ITCZ, down to 5°S, where surface winds are southwesterly, we still collected sediments that originated from the north and east, carried there by the NE trade wind layer, as well as by easterly winds from higher altitudes. The fact that the size of the wind-blown dust depends not only on the wind strength of the transporting agent but also on the distance to the source hampers a direct comparison of the dust's size distributions and measured wind strengths. However, a comparison between eolian dust and terrigenous sediments collected in three submarine sediment traps off the west coast of NW Africa shows that knowledge of the composition of eolian dust is a prerequisite for the interpretation of paleorecords obtained from sediment cores in the equatorial Atlantic.

Análise quantitativa das partículas de óxido de alumínio geradas na abrasão a ar em consultório odontológico

Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)

Os isotope ratios of Late Eocene sediments from the tropical Pacific

High resolution records (ca. 100 kyr) of Os isotope composition (187Os/188Os) in bulk sediments from two tropical Pacific sites (ODP Sites 1218 and 1219) capture the complete Late Eocene 187Os/188Os excursion and confirm that the Late Eocene 187Os/ 188Os minimum, earlier reported by Ravizza and Peucker-Ehrenbrink (2003, doi:10.1016/S0012-821X(03)00137-7), is a global feature. Using the astronomically tuned age models available for these sites, it is suggested that the Late Eocene 187Os/188Os minimum can be placed at 34.5 +/- 0.1 Ma in the marine records. In addition, two other distinct features of the 187Os/188Os excursion that are correlatable among sections are proposed as chemostratigraphic markers which can serve as age control points with a precision of ca. +/-0.1 Myr. We propose a speculative hypothesis that higher cosmic dust flux in the Late Eocene may have contributed to global cooling and Early Oligocene glaciation (Oi-1) by supplying bio-essential trace elements to the oceans and thereby resulting in higher ocean productivity, enhanced burial of organic carbon and draw down of atmospheric CO2. To determine if the hypothesis that enhanced cosmic dust flux in the Late Eocene was a cause for the 187Os/188Os excursion can be tested by using the paired bulk sediment and leachate Os isotope composition; 187Os/188Os were also measured in sediment leachates. Results of analyses of leachates are inconsistent between the south Atlantic and the Pacific sites, and therefore do not yield a robust test of this hypothesis. Comparison of 187Os/188Os records with high resolution benthic foraminiferal delta18O records across the Eocene-Oligocene transition suggests that 187Os flux to the oceans decreased during cooling and ice growth leading to the Oi-1 glaciation, whereas subsequent decay of ice-sheets and deglacial weathering drove seawater 187Os/188Os to higher values. Although the precise timing and magnitude of these changes in weathering fluxes and their effects on the marine 187Os/188Os records are obscured by recovery from the Late Eocene 187Os/188Os excursion, evidence of the global influence of glaciation on supply of Os to the ocean is robust as it has now been documented in both Pacific and Atlantic records.

Évaluation de la biomasse fongique dans les systèmes de ventilation

Le nettoyage des systèmes de Chauffage, Ventilation et Climatisation de l’Air est important pour assurer une bonne qualité d’air intérieur. Le déclenchement de leur nettoyage est basé sur une inspection visuelle qui ne tient pas compte du contenu en moisissures, lesquelles ont des effets sur le système respiratoire. Cette recherche vise à proposer une méthode d’évaluation du contenu en moisissures afin d’aider les gestionnaires d’immeuble. Cinq générations de poussières ont été effectuées pour simuler un conduit de ventilation. Une cassette modifiée 37 mm et un filtre CPV pré-pesés ont utilisés pour collecter les poussières déposées avec une pompe calibrée à 15L/min. Les pourcentages de collecte des cassettes et des filtres ont été calculés pour 54 échantillons. Dix générations supplémentaires de poussières ont été effectuées concomitamment avec la génération de spores. Soixante échantillons ont été analysés selon quatre méthodes : culture, comptage direct des spores par microscopie (CDSM), dosage de β-N-acétylhexosaminidase (NAHA), 18S-q-PCR. La limite de détection (LD), la réplicabilité, la répétabilité, le nombre de spores et le coefficient de corrélation (r) ont été déterminés. Les récupérations de poussières étaient supérieures à 84%. Selon la méthode analytique, les concentrations médianes de spores/100 cm² allaient de 10 000 à 815 000. Les LD variaient dépendamment de la méthode de 120 à 218 000 spores/100 cm² et r de -0,08 à 0,83. La réplicabilité et la répétabilité étaient de 1% et 1% pour PCR; 5% et 10% pour CDSM; 6% et 15% pour NAHA; 12% et 11% pour culture. La méthode de collecte a démontré une excellente efficacité de récupération. La PCR est la méthode analytique recommandée pour l’évaluation fongique des systèmes de ventilation. Une validation terrain est en cours.

Évaluation de la biomasse fongique dans les systèmes de ventilation

Le nettoyage des systèmes de Chauffage, Ventilation et Climatisation de l’Air est important pour assurer une bonne qualité d’air intérieur. Le déclenchement de leur nettoyage est basé sur une inspection visuelle qui ne tient pas compte du contenu en moisissures, lesquelles ont des effets sur le système respiratoire. Cette recherche vise à proposer une méthode d’évaluation du contenu en moisissures afin d’aider les gestionnaires d’immeuble. Cinq générations de poussières ont été effectuées pour simuler un conduit de ventilation. Une cassette modifiée 37 mm et un filtre CPV pré-pesés ont utilisés pour collecter les poussières déposées avec une pompe calibrée à 15L/min. Les pourcentages de collecte des cassettes et des filtres ont été calculés pour 54 échantillons. Dix générations supplémentaires de poussières ont été effectuées concomitamment avec la génération de spores. Soixante échantillons ont été analysés selon quatre méthodes : culture, comptage direct des spores par microscopie (CDSM), dosage de β-N-acétylhexosaminidase (NAHA), 18S-q-PCR. La limite de détection (LD), la réplicabilité, la répétabilité, le nombre de spores et le coefficient de corrélation (r) ont été déterminés. Les récupérations de poussières étaient supérieures à 84%. Selon la méthode analytique, les concentrations médianes de spores/100 cm² allaient de 10 000 à 815 000. Les LD variaient dépendamment de la méthode de 120 à 218 000 spores/100 cm² et r de -0,08 à 0,83. La réplicabilité et la répétabilité étaient de 1% et 1% pour PCR; 5% et 10% pour CDSM; 6% et 15% pour NAHA; 12% et 11% pour culture. La méthode de collecte a démontré une excellente efficacité de récupération. La PCR est la méthode analytique recommandée pour l’évaluation fongique des systèmes de ventilation. Une validation terrain est en cours.

Can quantum mechanics fool the cosmic censor?

We revisit the mechanism for violating the weak cosmic-censorship conjecture (WCCC) by overspinning a nearly-extreme charged black hole. The mechanism consists of an incoming massless neutral scalar particle, with low energy and large angular momentum, tunneling into the hole. We investigate the effect of the large angular momentum of the incoming particle on the background geometry and address recent claims that such a backreaction would invalidate the mechanism. We show that the large angular momentum of the incident particle does not constitute an obvious impediment to the success of the overspinning quantum mechanism, although the induced backreaction turns out to be essential to restoring the validity of the WCCC in the classical regime. These results seem to endorse the view that the ""cosmic censor"" may be oblivious to processes involving quantum effects.

First-order formalism for dark energy and dust

This work deals with a first-order formalism for dark energy and dust in standard cosmology, for models described by a real scalar field in the presence of dust in spatially flat space. The field dynamics may be standard or tachyonic, and we show how the equations of motion can be solved by first-order differential equations. We investigate a model to illustrate how the dustlike matter may affect the cosmic evolution using this framework.

Cosmogenic production rates and recoil loss effects in micrometeorites and interplanetary dust particles

We present a purely physical model to determine cosmogenic production rates for noble gases and radionuclides in micrometeorites (MMs) and interplanetary dust particles (IDPs) by solar cosmic-rays (SCR) and galactic cosmic-rays (GCR) fully considering recoil loss effects. Our model is based on various nuclear model codes to calculate recoil cross sections, recoil ranges, and finally the percentages of the cosmogenic nuclides that are lost as a function of grain size, chemical composition of the grain, and the spectral distribution of the projectiles. The main advantage of our new model compared with earlier approaches is that we consider the entire SCR particle spectrum up to 240 MeV and not only single energy points. Recoil losses for GCR-produced nuclides are assumed to be equal to recoil losses for SCR-produced nuclides. Combining the model predictions with Poynting-Robertson orbital lifetimes, we calculate cosmic-ray exposure ages for recently studied MMs, cosmic spherules, and IDPs. The ages for MMs and the cosmic-spherule are in the range <2.2–233 Ma, which corresponds, according to the Poynting-Robertson drag, to orbital distances in the range 4.0–34 AU. For two IDPs, we determine exposure ages of longer than 900 Ma, which corresponds to orbital distances larger than 150 AU. The orbital distance in the range 4–6 AU for one MM and the cosmic spherule indicate an origin either in the asteroid belt or release from comets coming either from the Kuiper Belt or the Oort Cloud. Three of the studied MMs have orbital distances in the range 23–34 AU, clearly indicating a cometary origin, either from short-period comets from the Kuiper Belt or from the Oort Cloud. The two IDPs have orbital distances of more than 150 AU, indicating an origin from Oort Cloud comets.