Correlation of the EPR properties of perchlorotriphenylmethyl radical and their efficiency as DNP polarizers

Water soluble perchlorinated trityl (PTM) radicals were found to be effective 95 GHz DNP (dynamic nuclear polarization) polarizers in ex situ (dissolution) 13C DNP (Gabellieri et al., Angew Chem., Int. Ed. 2010, 49, 3360). The degree of the nuclear polarization obtained was reported to be dependent on the position of the chlorine substituents on the trityl skeleton. In addition, on the basis of the DNP frequency sweeps it was suggested that the 13C NMR signal enhancement is mediated by the Cl nuclei. To understand the DNP mechanism of the PTM radicals we have explored the 95 GHz EPR characteristics of these radicals that are relevant to their performance as DNP polarizers. The EPR spectra of the radicals revealed axially symmetric g-tensors. A comparison of the spectra with the 13C DNP frequency sweeps showed that although the solid effect mechanism is operational the DNP frequency sweeps reveal some extra width suggesting that contributions from EPR forbidden transitions involving 35,37Cl nuclear flips are likely. This was substantiated experimentally by ELDOR (electron-electron double resonance) detected NMR measurements, which map the EPR forbidden transitions, and ELDOR experiments that follow the depolarization of the electron spin upon irradiation of the forbidden EPR transitions. DFT (density functional theory) calculations helped to assign the observed transitions and provided the relevant spin Hamiltonian parameters. These results show that the 35,37Cl hyperfine and nuclear quadrupolar interactions cause a considerable nuclear state mixing at 95 GHz thus facilitating the polarization of the Cl nuclei upon microwave irradiation. Overlap of Cl nuclear frequencies and the 13C Larmor frequency further facilitates the polarization of the 13C nuclei by spin diffusion. Calculation of the 13C DNP frequency sweep based on the Cl nuclear polarization showed that it does lead to an increase in the width of the spectra, improving the agreement with the experimental sweeps, thus supporting the existence of a new heteronuclear assisted DNP mechanism.

Kalibrointimenetelmä planaaristen siirtojohtojen mittaamiseen

Tässä diplomityössä tutkittiin TRL-kalibroinnin käyttämistä tasomaisten siirtojohtojen sähköisten parametrien määrittämisessä taajuusalueella 0,3 – 12 GHz. Työssä perehdyttiin TRL-kalibroinnin käyttämiseen piirianalysaattorilla toteutettujen mittauksien mittauskalibrointiin sekä kalibrointiin tarvittavien kalibrointistandardien mitoittamiseen. Kalibrointistandardit suunniteltiin ja toteutettiin sekä mikroliuska- että liuskajohdoille, joiden toiminnallisuutta tarkasteltiin sekä taajuustason että aikatason mittausten avulla. Työssä perehdyttiin myös kalibrointistandardien liityntärajapinnan suunniteluun ja toteuttamiseen. Saatujen tulosten perusteella voitiin osoittaa mikroliuskajohtokitin soveltuvan hyvin mittauskalibroinnin toteuttamiseen tarkoissa mittaussovelluksissa.

Johdinhäviöiden määrittäminen mikroliuskarakenteessa

Tässä diplomityössä on käsitelty mikroliuskarakenteen johdinhäviöiden määrittämistä kokeellisin ja analyyttisin menetelmin. Työssä on käyty läpi mikroliuskarakenteen ominaisuudet sekä esitetty tärkeimmät kirjallisuudessa esitellyt menetelmät johdinhäviöiden laskemiseksi. Mikroliuskarakenteen häviöitä mallinnettiin modernilla momenttimenetelmään perustuvalla kenttälaskentasimulaattorilla. Simulaattorin toimintaperiaate on esitelty ja sen soveltaminen mikroliuskarakenteen simuloimiseen on käyty läpi. Eräs mikroliuskarakenne mallinnettiin taajuusalueella 1-10 GHz ja simuloituja johdinhäviöitä verrattiin analyyttisesti määritettyihin. Mikroliuskarakenteen vaste mitattiin ja sitä verrattiin mallinnetun mikroliuskarakenteen vasteeseen. Tulosten perusteella on pohdittu simulaattorin soveltuvuutta mikroliuskarakenteen johdinhäviöiden mallintamiseen. Mikroliuskarakenteen johdinhäviöiden määrittämiseen mittausten avulla on esitetty ideoita jatkotutkimusta varten.

Antennimittausjärjestelmän toteutus ja ominaisuuksien määrittäminen

Diplomityössä tarkasteltiin antennien säteilykuviomittauksiin käytettävien antennimittaratojen ominaisuuksia. Sovelletun elektroniikan laboratorion antennimittaradasta kehitettiin toimiva säteilykuvion mittausjärjestelmä, johon kuuluvat radiokaiuton kammio, suuntauskoneisto ja antennikannakkeet, HP 8720D -piirianalysaattori ja RF-kaapelointi sekä valmistutetut mitta-antennitorvet. Työssä vertailtiin koaksiaalikaapeleita ja valittiin antennimittaukseen soveltuvat. 1,70–2,60 GHz:n taajuusalueen mittastandardiksi suunniteltiin torviantenni, jonka kaksi prototyyppiä valmistutettiin konetekniikan osastolla. Torviantennien ominaisuudet mitattiin. Antennimittaradan ominaisuudet ja soveltuvuus erilaisiin antennimittauksiin selvitettiin sekä teoreettisesti että mittauksin.

The 2010 May Flaring Episode of Cygnus X-3 in Radio, X-rays, and γ-rays

In 2009, Cygnus X-3 (Cyg X-3) became the first microquasar to be detected in the GeV γ-ray regime, via the satellites Fermi and AGILE. The addition of this new band to the observational toolbox holds promise for building a more detailed understanding of the relativistic jets of this and other systems. We present a rich data set of radio, hard and soft X-ray, and γ-ray observations of Cyg X-3 made during a flaring episode in 2010 May. We detect a ~3 day softening and recovery of the X-ray emission, followed almost immediately by a ~1 Jy radio flare at 15 GHz, followed by a 4.3σ γ-ray flare (E > 100 MeV) ~1.5 days later. The radio sampling is sparse, but we use archival data to argue that it is unlikely the γ-ray flare was followed by any significant unobserved radio flares. In this case, the sequencing of the observed events is difficult to explain in a model in which the γ-ray emission is due to inverse Compton scattering of the companion star's radiation field. Our observations suggest that other mechanisms may also be responsible for γ-ray emission from Cyg X-3.

Deep GMRT radio observations and a multi-wavelength study of the region around HESS J1858+020

Context. There are a number of very high energy sources in the Galaxy that remain unidentified. Multi-wavelength and variability studies, and catalogue searches, are powerful tools to identify the physical counterpart, given the uncertainty in the source location and extension. Aims. This work carries out a thorough multi-wavelength study of the unidentified, very high energy source HESS J1858+020 and its environs. Methods. We have performed Giant Metrewave Radio Telescope observations at 610 MHz and 1.4 GHz to obtain a deep, low-frequency radio image of the region surrounding HESS J1858+020. We analysed archival radio, infrared, and X-ray data as well. This observational information, combined with molecular data, catalogue sources, and a nearby Fermi gamma-ray detection of unidentified origin, are combined to explore possible counterparts to the very high energy source. Results. We provide with a deep radio image of a supernova remnant that might be related to the GeV and TeV emission in the region. We confirm the presence of an H ii region next to the supernova remnant and coincident with molecular emission. A potential region of star formation is also identified. We identify several radio and X-ray sources in the surroundings. Some of these sources are known planetary nebulae, whereas others may be non-thermal extended emitters and embedded young stellar objects. Three old, background Galactic pulsars also neighbour HESS J1858+020 along the line of sight. Conclusions. The region surrounding HESS J1858+020 is rich in molecular structures and non-thermal objects that may potentially be linked to this unidentified very high energy source. In particular, a supernova remnant interacting with nearby molecular clouds may be a good candidate, but a star forming region, or a non-thermal radio source of yet unclear nature, may also be behind the gamma-ray source. The neighbouring pulsars, despite being old and distant, cannot be discarded as candidates. Further observational studies are needed, however, to narrow the search for a counterpart to the HESS source.

Gas-phase photocatalytic oxidation of volatile organic compounds

Substances emitted into the atmosphere by human activities in urban and industrial areas cause environmental problems such as air quality degradation, respiratory diseases, climate change, global warming, and stratospheric ozone depletion. Volatile organic compounds (VOCs) are major air pollutants, emitted largely by industry, transportation and households. Many VOCs are toxic, and some are considered to be carcinogenic, mutagenic, or teratogenic. A wide spectrum of VOCs is readily oxidized photocatalytically. Photocatalytic oxidation (PCO) over titanium dioxide may present a potential alternative to air treatment strategies currently in use, such as adsorption and thermal treatment, due to its advantageous activity under ambient conditions, although higher but still mild temperatures may also be applied. The objective of the present research was to disclose routes of chemical reactions, estimate the kinetics and the sensitivity of gas-phase PCO to reaction conditions in respect of air pollutants containing heteroatoms in their molecules. Deactivation of the photocatalyst and restoration of its activity was also taken under consideration to assess the practical possibility of the application of PCO to the treatment of air polluted with VOCs. UV-irradiated titanium dioxide was selected as a photocatalyst for its chemical inertness, non-toxic character and low cost. In the present work Degussa P25 TiO2 photocatalyst was mostly used. In transient studies platinized TiO2 was also studied. The experimental research into PCO of following VOCs was undertaken: - methyl tert-butyl ether (MTBE) as the basic oxygenated motor fuel additive and, thus, a major non-biodegradable pollutant of groundwater; - tert-butyl alcohol (TBA) as the primary product of MTBE hydrolysis and PCO; - ethyl mercaptan (ethanethiol) as one of the reduced sulphur pungent air pollutants in the pulp-and-paper industry; - methylamine (MA) and dimethylamine (DMA) as the amino compounds often emitted by various industries. The PCO of VOCs was studied using a continuous-flow mode. The PCO of MTBE and TBA was also studied by transient mode, in which carbon dioxide, water, and acetone were identified as the main gas-phase products. The volatile products of thermal catalytic oxidation (TCO) of MTBE included 2-methyl-1-propene (2-MP), carbon monoxide, carbon dioxide and water; TBA decomposed to 2-MP and water. Continuous PCO of 4 TBA proceeded faster in humid air than dry air. MTBE oxidation, however, was less sensitive to humidity. The TiO2 catalyst was stable during continuous PCO of MTBE and TBA above 373 K, but gradually lost activity below 373 K; the catalyst could be regenerated by UV irradiation in the absence of gas-phase VOCs. Sulphur dioxide, carbon monoxide, carbon dioxide and water were identified as ultimate products of PCO of ethanethiol. Acetic acid was identified as a photocatalytic oxidation by-product. The limits of ethanethiol concentration and temperature, at which the reactor performance was stable for indefinite time, were established. The apparent reaction kinetics appeared to be independent of the reaction temperature within the studied limits, 373 to 453 K. The catalyst was completely and irreversibly deactivated with ethanethiol TCO. Volatile PCO products of MA included ammonia, nitrogen dioxide, nitrous oxide, carbon dioxide and water. Formamide was observed among DMA PCO products together with others similar to the ones of MA. TCO for both substances resulted in the formation of ammonia, hydrogen cyanide, carbon monoxide, carbon dioxide and water. No deactivation of the photocatalyst during the multiple long-run experiments was observed at the concentrations and temperatures used in the study. PCO of MA was also studied in the aqueous phase. Maximum efficiency was achieved in an alkaline media, where MA exhibited high fugitivity. Two mechanisms of aqueous PCO – decomposition to formate and ammonia, and oxidation of organic nitrogen directly to nitrite - lead ultimately to carbon dioxide, water, ammonia and nitrate: formate and nitrite were observed as intermediates. A part of the ammonia formed in the reaction was oxidized to nitrite and nitrate. This finding helped in better understanding of the gasphase PCO pathways. The PCO kinetic data for VOCs fitted well to the monomolecular Langmuir- Hinshelwood (L-H) model, whereas TCO kinetic behaviour matched the first order process for volatile amines and the L-H model for others. It should be noted that both LH and the first order equations were only the data fit, not the real description of the reaction kinetics. The dependence of the kinetic constants on temperature was established in the form of an Arrhenius equation.

Microwave spectrometry for the Evaluation of the structural integrity of metallic stents

Purpose: To assess the feasibility of a method based on microwave spectrometry to detect structural distortions of metallic stents in open air conditions and envisage the prospects of this approach toward possible medical applicability for the evaluation of implanted stents. Methods: Microwave absorbance spectra between 2.0 and 18.0 GHz were acquired in open air for the characterization of a set of commercial stents using a specifically design setup. Rotating each sample over 360º, 2D absorbance diagrams were generated as a function of frequency and rotation angle. To check our approach for detecting changes in stent length (fracture) and diameter (recoil), two specific tests were performed in open air. Finally, with a few adjustments, this same system provides 2D absorbance diagrams of stents immersed in a water-based phantom, this time over a bandwidth ranging from 0.2 to 1.8 GHz. Results: The authors show that metallic stents exhibit characteristic resonant frequencies in their microwave absorbance spectra in open air which depend on their length and, as a result, may reflect the occurrence of structural distortions. These resonances can be understood considering that such devices behave like dipole antennas in terms of microwave scattering. From fracture tests, the authors infer that microwave spectrometry provides signs of presence of Type I to Type IV stent fractures and allows in particular a quantitative evaluation of Type III and Type IV fractures. Recoil tests show that microwave spectrometry seems able to provide some quantitative assessment of diametrical shrinkage, but only if it involves longitudinal shortening. Finally, the authors observe that the resonant frequencies of stents placed inside the phantom shift down with respect to the corresponding open air frequencies, as it should be expected considering the increase of dielectric permittivity from air to water. Conclusions: The evaluation of stent resonant frequencies provided by microwave spectrometry allows detection and some quantitative assessment of stent fracture and recoil in open air conditions. Resonances of stents immersed in water can be also detected and their characteristic frequencies are in good agreement with theoretical estimates. Although these are promising results, further verifica tion in a more relevant phantom is required in order to foresee the real potential of this approach.

EVN+MERLIN observations of microquasar candidates at low galactic latitudes

In an attempt to increase the number of known microquasars, Paredes et al. (2002) have presented a long-term project focused on the search for new objects of this type. They performed a cross-identification between X-ray and radio catalogs under very restrictive selection criteria for sources with |b|<5 degrees, and obtained a sample of 13 radio-emitting X-ray sources. Follow-up observations of 6 of these sources with the VLA provided accurate coordinates, which were used to discover optical counterparts for all of them. We have observed these six sources with the EVN and MERLIN at 5 GHz. Five of the six objects have been detected and imaged, presenting different morphologies: one source has a two-sided jet, three sources have one-sided jets, and one source is compact. With all the presently available information, we conclude that two of the sources are promising microquasar candidates in our Galaxy.

The Electronic Structure of Co-Sputtered Zinc Indium Tin Oxide Thin Films

Zinc indium tin oxide (ZITO) transparent conductive oxide layers were deposited via radio frequency (RF) magnetron co-sputtering at room temperature. A series of samples with gradually varying zinc content was investigated. The samples were characterized with x-ray and ultraviolet photoemission spectroscopy (XPS, UPS) to determine the electronic structure of the surface. Valence and conduction bands maxima (VBM, CBM), and work function were determined. The experiments indicate that increasing Zn content results in films with a higher defect rate at the surface leading to the formation of a degenerately doped surface layer if the Zn content surpasses 50%. Furthermore, the experiments demonstrate that ZITO is susceptible to ultraviolet light induced work function reduction, similar to what was earlier observed on ITO and TiO2 films.

Photocatalytic Activity of Nanostructured Anatase Coatings Obtained by Cold Gas Spray

This article describes a photocatalytic nanostructured anatase coating deposited by cold gas spray (CGS)supported on titanium sub-oxide (TiO22x) coatings obtained by atmospheric plasma spray (APS) onto stainless steel cylinders. The photocatalytic coating was homogeneous and preserved the composition and nanostructure of the starting powder. The inner titanium sub-oxide coating favored the deposition of anatase particles in the solid state. Agglomerated nano-TiO2 particles fragmented when impacting onto the hard surface of the APS TiO22x bond coat. The rough surface provided by APS provided an ideal scenario for entrapping the nanostructured particles, which may be adhered onto the bond coat due to chemical bonding; a possible bonding mechanism is described. Photocatalytic experiments showed that CGS nano-TiO2 coating was active for photodegrading phenol and formic acid under aqueous conditions. The results were similar to the performance obtained by competitor technologies and materials such as dip-coating P25 photocatalysts. Disparity in the final performance of the photoactive materials may have been caused by differences in grain size and the crystalline composition of titanium dioxide.

A study of electromagnetic shielding properties of Ni79Fe16Mo5/copper films

The plane wave electromagnetic interference (EMI) shielding properties of DC sputtered Ni79Fe16Mo5 and copper layers were studied according to ASTM D 4935-89 on frequency range of 50 MHz – 2.5 GHz and RF magnetic shielding effectiveness by shielded magnetic loop probes. Results show that Ni79Fe16Mo5 provides better RF magnetic shielding above the layer thickness of approximately 120 nm. Copper provides better plane wave shielding effectiveness. The effect of shield internal interfaces was studied by depositing thin multilayer structures with and without a dielectric spacer layer.

Dustiness and deagglomeration testing: interlaboratory comparison of systems for nanoparticle powders

Different types of aerosolization and deagglomeration testing systems exist for studying the properties of nanomaterial powders and their aerosols. However, results are dependent on the specific methods used. In order to have well-characterized aerosols, we require a better understanding of how system parameters and testing conditions influence the properties of the aerosols generated. In the present study, four experimental setups delivering different aerosolization energies were used to test the resultant aerosols of two distinct nanomaterials (hydrophobic and hydrophilic TiO2). The reproducibility of results within each system was good. However, the number concentrations and size distributions of the aerosols created varied across the four systems; for number concentrations, e.g., from 10(3) to 10(6) #/cm(3). Moreover, distinct differences were also observed between the two materials with different surface coatings. The article discusses how system characteristics and other pertinent conditions modify the test results. We propose using air velocity as a suitable proxy for estimating energy input levels in aerosolization systems. The information derived from this work will be especially useful for establishing standard operating procedures for testing nanopowders, as well as for estimating their release rates under different energy input conditions, which is relevant for occupational exposure.

The Coordinated Radio and Infrared Survey for High-mass Star Formation. II. Source Catalog

The CORNISH project is the highest resolution radio continuum survey of the Galactic plane to date. It is the 5 GHz radio continuum part of a series of multi-wavelength surveys that focus on the northern GLIMPSE region (10° < l < 65°), observed by the Spitzer satellite in the mid-infrared. Observations with the Very Large Array in B and BnA configurations have yielded a 1.''5 resolution Stokes I map with a root mean square noise level better than 0.4 mJy beam 1. Here we describe the data-processing methods and data characteristics, and present a new, uniform catalog of compact radio emission. This includes an implementation of automatic deconvolution that provides much more reliable imaging than standard CLEANing. A rigorous investigation of the noise characteristics and reliability of source detection has been carried out. We show that the survey is optimized to detect emission on size scales up to 14'' and for unresolved sources the catalog is more than 90% complete at a flux density of 3.9 mJy. We have detected 3062 sources above a 7σ detection limit and present their ensemble properties. The catalog is highly reliable away from regions containing poorly sampled extended emission, which comprise less than 2% of the survey area. Imaging problems have been mitigated by down-weighting the shortest spacings and potential artifacts flagged via a rigorous manual inspection with reference to the Spitzer infrared data. We present images of the most common source types found: H II regions, planetary nebulae, and radio galaxies. The CORNISH data and catalog are available online at http://cornish.leeds.ac.uk.

Stability of nanoparticle agglomerates under mechanical stress and its effects on their release into the air

L'exposition professionnelle aux nanomatériaux manufacturés dans l'air présente des risques potentiels pour la santé des travailleurs dans les secteurs de la nanotechnologie. Il est important de comprendre les scénarios de libération des aérosols de nanoparticules dans les processus et les activités associées à l'exposition humaine. Les mécanismes de libération, y compris les taux de libération et les propriétés physico-chimiques des nanoparticules, déterminent leurs comportements de transport ainsi que les effets biologiques néfastes. La distribution de taille des particules d'aérosols est l'un des paramètres les plus importants dans ces processus. La stabilité mécanique d'agglomérats de nanoparticules affecte leurs distributions de tailles. Les potentiels de désagglomération de ces agglomérats déterminent les possibilités de leur déformation sous énergies externes. Cela rend les changements possibles dans leur distribution de taille et de la concentration en nombre qui vont finalement modifier leurs risques d'exposition. Les conditions environnementales, telles que l'humidité relative, peuvent influencer les processus de désagglomération par l'adhérence de condensation capillaire de l'humidité. L'objectif général de cette thèse était d'évaluer les scénarios de libération des nanomatériaux manufacturés des processus et activités sur le lieu de travail. Les sous-objectifs étaient les suivants: 1. Etudier les potentiels de désagglomération des nanoparticules dans des conditions environnementales variées. 2. Etudier la libération des nano-objets à partir de nanocomposites polymères; 3. Evaluer la libération de nanoparticules sur le lieu de travail dans des situations concrètes. Nous avons comparé différents systèmes de laboratoire qui présentaient différents niveau d'énergie dans l'aérosolisation des poudres. Des nanopoudres de TiO2 avec des hydrophilicités de surface distinctes ont été testées. Un spectromètre à mobilité électrique (SMPS), un spectromètre à mobilité aérodynamique (APS) et un spectromètre optique (OPC) ont été utilisés pour mesurer la concentration de particules et la distribution de taille des particules. La microscopie électronique à transmission (TEM) a été utilisée pour l'analyse morphologique d'échantillons de particules dans l'air. Les propriétés des aérosols (distribution de taille et concentration en nombre) étaient différentes suivant la méthode employée. Les vitesses des flux d'air d'aérosolisation ont été utilisées pour estimer le niveau d'énergie dans ces systèmes, et il a été montré que les tailles modales des particules étaient inversement proportionnelles à la vitesse appliquée. En général, les particules hydrophiles ont des diamètres plus grands et des nombres inférieurs à ceux des particules hydrophobes. Toutefois, cela dépend aussi des méthodes utilisées. La vitesse de l'air peut donc être un paramètre efficace pour le classement de l'énergie des procédés pour des systèmes d'aérosolisation similaires. Nous avons développé un système laboratoire pour tester les potentiels de désagglomération des nanoparticules dans l'air en utilisant des orifices critiques et un humidificateur. Sa performance a été comparée à un système similaire dans un institut partenaire. Une variété de nanopoudres différentes a été testée. Le niveau d'énergie appliquée et l'humidité ont été modifiés. Le SMPS et l'OPC ont été utilisés pour mesurer la concentration de particules et la distribution de la taille. Un TEM a été utilisé pour l'analyse morphologique d'échantillons de particules dans l'air. Le diamètre moyen des particules a diminué et la concentration en nombre s'est accrue lorsque des énergies externes ont été appliquées. Le nombre de particules inférieures à 100 nm a été augmenté, et celui au-dessus de 350 nm réduits. Les conditions humides ont faits exactement le contraire, en particulier pour les petites particules. En outre, ils ont réduits les effets de la différence de pression due à l'orifice. Les résultats suggèrent que la désagglomération d'agglomérats de nanoparticules dans l'air est possible dans la gamme d'énergie appliquée. Cependant, l'atmosphère humide peut favoriser leur agglomération et améliorer leurs stabilités en réduisant la libération de nanoparticules dans l'environnement. Nous proposons d'utiliser notre système pour le test de routine des potentiels de désagglomération des nanomatériaux manufacturés et de les classer. Un tel classement faciliterait la priorisation de l'exposition et du risque encouru en fonction du niveau d'ENM. Un système de perçage automatique et un système de sciage manuel ont été développés pour étudier la libération de nanoparticules à partir de différents types de nanocomposites. La vitesse de perçage et taille de la mèche ont été modifiées dans les expériences. La distribution de taille des particules et leur concentration en nombre ont été mesurées par un SMPS et un miniature diffusion size classifier (DISCmini). Les distributions de nanoparticules dans les composites et les particules libérées ont été analysés par un TEM et un microscope électronique à balayage (SEM). Les tests de perçage ont libérés un plus grand nombre de particules que le sciage. Des vitesses de perçage plus rapide et les mèches plus grandes ont augmentés la génération de particules. Les charges de nanoparticules manufacturées dans les composites ne modifient pas leurs comportements de libération dans les expériences de perçage. Toutefois, le sciage différencie les niveaux de libération entre les composites et les échantillons blancs. De plus, les vapeurs de polymères ont été générées par la chaleur de sciage. La plupart des particules libérées sont des polymères contenant des nanoparticules ou sur leurs surface. Les résultats ont souligné l'importance du type de processus et paramètres pour déterminer la libération de nanoparticules de composites. Les émissions secondaires telles que les fumées polymères appellent à la nécessité d'évaluations de l'exposition et de risque pour de tels scénarios. Une revue systématique de la littérature sur le sujet de libérations de nanoparticules dans l'air dans les secteurs industriels et laboratoires de recherche a été effectuée. Des stratégies de recherche des informations pertinentes et de stockage ont été développées. Les mécanismes de libération, tels que la taille de particules d'aérosol et de leur concentration en nombre, ont été comparés pour différentes activités. La disponibilité de l'information contextuelle qui est pertinente pour l'estimation de l'exposition humaine a été évaluée. Il a été constaté que les données relatives à l'exposition ne sont pas toujours disponibles dans la littérature actuelle. Les propriétés des aérosols libérés semblent dépendre de la nature des activités. Des procédés à haute énergie ont tendance à générer des plus hauts niveaux de concentrations de particules dans les gammes de plus petite taille. Les résultats peuvent être utiles pour déterminer la priorité des procédés industriels pour l'évaluation les risques associés dans une approche à plusieurs niveaux. Pour l'évaluation de l'exposition, la disponibilité de l'information peut être améliorée par le développement d'une meilleure méthode de communication des données.