Selection of operational parameters for the production of instant soy protein isolate by pulsed fluid bed agglomeration

The objective of this study was to select the optimal operational conditions for the production of instant soy protein isolate (SPI) by pulsed fluid bed agglomeration. The spray-dried SPI was characterized as being a cohesive powder, presenting cracks and channeling formation during its fluidization (Geldart type A). The process was carried out in a pulsed fluid bed, and aqueous maltodextrin solution was used as liquid binder. Air pulsation, at a frequency of 600 rpm, was used to fluidize the cohesive SPI particles and to allow agglomeration to occur. Seventeen tests were performed according to a central composite design. Independent variables were (i) feed flow rate (0.5-3.5 g/min), (ii) atomizing air pressure (0.5-1.5 bar) and (iii) binder concentration (10-50%). Mean particle diameter, process yield and product moisture were analyzed as responses. Surface response analysis led to the selection of optimal operational parameters, following which larger granules with low moisture content and high process yield were produced. Product transformations were also evaluated by the analysis of size distribution, flowability, cohesiveness and wettability. When compared to raw material, agglomerated particles were more porous and had a more irregular shape, presenting a wetting time decrease, free-flow improvement and cohesiveness reduction. (C) 2010 Elsevier B.V. All rights reserved.

Meiotic nucleolar cycle and chromatoid body formation during the rat (Rattus novergicus) and mouse (Mus musculus) spermiogenesis

The aims of the present study were to follow the nucleolar cycle in spermiogenesis of the laboratory rodents Rattus novergicus and Mus musculus, to verify the relationship between the nucleolar component and chromatoid body (CB) formation and to investigate the function of this cytoplasmic supramolecular structure in spermatogenic haploid cells. Histological sections of adult seminiferous tubules were analyzed cytochemically by light microscopy and ultrastructural procedures by transmission electron microscopy. The results reveal that in early spermatids, the CB was visualized in association with the Golgi cisterns indicating that this structure may participate in the acrosome formation process. In late spermatids, the CB was observed near the axonema, a fact suggesting that this structure may support the formation of the spermatozoon tail. In conclusion, our data showed that there is disintegration of spermatid nucleoli at the beginning of spermatogenesis and a fraction of this nucleolar material migrates to the cytoplasm, where a specific structure is formed, known as the "chromatoid body", which, apparently, participates in some parts of the rodent spermiogenesis process. (c) 2007 Elsevier Ltd. All rights reserved.

Relationship between the nucleolar cycle and chromatoid body formation in the spermatogenesis of Phrynops geoffroanus (Reptilia Testudines)

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Estudo da distribuição de tamanho e composição iônica de aerossóis e seus efeitos na capacidade de nuclear gotas de nuvens

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

THE ROLE OF TURBULENT MAGNETIC RECONNECTION IN THE FORMATION OF ROTATIONALLY SUPPORTED PROTOSTELLAR DISKS

The formation of protostellar disks out of molecular cloud cores is still not fully understood. Under ideal MHD conditions, the removal of angular momentum from the disk progenitor by the typically embedded magnetic field may prevent the formation of a rotationally supported disk during the main protostellar accretion phase of low-mass stars. This has been known as the magnetic braking problem and the most investigated mechanism to alleviate this problem and help remove the excess of magnetic flux during the star formation process, the so-called ambipolar diffusion (AD), has been shown to be not sufficient to weaken the magnetic braking at least at this stage of the disk formation. In this work, motivated by recent progress in the understanding of magnetic reconnection in turbulent environments, we appeal to the diffusion of magnetic field mediated by magnetic reconnection as an alternative mechanism for removing magnetic flux. We investigate numerically this mechanism during the later phases of the protostellar disk formation and show its high efficiency. By means of fully three-dimensional MHD simulations, we show that the diffusivity arising from turbulent magnetic reconnection is able to transport magnetic flux to the outskirts of the disk progenitor at timescales compatible with the collapse, allowing the formation of a rotationally supported disk around the protostar of dimensions similar to 100 AU, with a nearly Keplerian profile in the early accretion phase. Since MHD turbulence is expected to be present in protostellar disks, this is a natural mechanism for removing magnetic flux excess and allowing the formation of these disks. This mechanism dismisses the necessity of postulating a hypothetical increase of the ohmic resistivity as discussed in the literature. Together with our earlier work which showed that magnetic flux removal from molecular cloud cores is very efficient, this work calls for reconsidering the relative role of AD in the processes of star and planet formation.

Statistical properties of Radio Halos and the re-acceleration model

Galaxy clusters occupy a special position in the cosmic hierarchy as they are the largest bound structures in the Universe. There is now general agreement on a hierarchical picture for the formation of cosmic structures, in which galaxy clusters are supposed to form by accretion of matter and merging between smaller units. During merger events, shocks are driven by the gravity of the dark matter in the diffuse barionic component, which is heated up to the observed temperature. Radio and hard-X ray observations have discovered non-thermal components mixed with the thermal Intra Cluster Medium (ICM) and this is of great importance as it calls for a “revision” of the physics of the ICM. The bulk of present information comes from the radio observations which discovered an increasing number of Mpcsized emissions from the ICM, Radio Halos (at the cluster center) and Radio Relics (at the cluster periphery). These sources are due to synchrotron emission from ultra relativistic electrons diffusing through µG turbulent magnetic fields. Radio Halos are the most spectacular evidence of non-thermal components in the ICM and understanding the origin and evolution of these sources represents one of the most challenging goal of the theory of the ICM. Cluster mergers are the most energetic events in the Universe and a fraction of the energy dissipated during these mergers could be channelled into the amplification of the magnetic fields and into the acceleration of high energy particles via shocks and turbulence driven by these mergers. Present observations of Radio Halos (and possibly of hard X-rays) can be best interpreted in terms of the reacceleration scenario in which MHD turbulence injected during these cluster mergers re-accelerates high energy particles in the ICM. The physics involved in this scenario is very complex and model details are difficult to test, however this model clearly predicts some simple properties of Radio Halos (and resulting IC emission in the hard X-ray band) which are almost independent of the details of the adopted physics. In particular in the re-acceleration scenario MHD turbulence is injected and dissipated during cluster mergers and thus Radio Halos (and also the resulting hard X-ray IC emission) should be transient phenomena (with a typical lifetime <» 1 Gyr) associated with dynamically disturbed clusters. The physics of the re-acceleration scenario should produce an unavoidable cut-off in the spectrum of the re-accelerated electrons, which is due to the balance between turbulent acceleration and radiative losses. The energy at which this cut-off occurs, and thus the maximum frequency at which synchrotron radiation is produced, depends essentially on the efficiency of the acceleration mechanism so that observations at high frequencies are expected to catch only the most efficient phenomena while, in principle, low frequency radio surveys may found these phenomena much common in the Universe. These basic properties should leave an important imprint in the statistical properties of Radio Halos (and of non-thermal phenomena in general) which, however, have not been addressed yet by present modellings. The main focus of this PhD thesis is to calculate, for the first time, the expected statistics of Radio Halos in the context of the re-acceleration scenario. In particular, we shall address the following main questions: • Is it possible to model “self-consistently” the evolution of these sources together with that of the parent clusters? • How the occurrence of Radio Halos is expected to change with cluster mass and to evolve with redshift? How the efficiency to catch Radio Halos in galaxy clusters changes with the observing radio frequency? • How many Radio Halos are expected to form in the Universe? At which redshift is expected the bulk of these sources? • Is it possible to reproduce in the re-acceleration scenario the observed occurrence and number of Radio Halos in the Universe and the observed correlations between thermal and non-thermal properties of galaxy clusters? • Is it possible to constrain the magnetic field intensity and profile in galaxy clusters and the energetic of turbulence in the ICM from the comparison between model expectations and observations? Several astrophysical ingredients are necessary to model the evolution and statistical properties of Radio Halos in the context of re-acceleration model and to address the points given above. For these reason we deserve some space in this PhD thesis to review the important aspects of the physics of the ICM which are of interest to catch our goals. In Chapt. 1 we discuss the physics of galaxy clusters, and in particular, the clusters formation process; in Chapt. 2 we review the main observational properties of non-thermal components in the ICM; and in Chapt. 3 we focus on the physics of magnetic field and of particle acceleration in galaxy clusters. As a relevant application, the theory of Alfv´enic particle acceleration is applied in Chapt. 4 where we report the most important results from calculations we have done in the framework of the re-acceleration scenario. In this Chapter we show that a fraction of the energy of fluid turbulence driven in the ICM by the cluster mergers can be channelled into the injection of Alfv´en waves at small scales and that these waves can efficiently re-accelerate particles and trigger Radio Halos and hard X-ray emission. The main part of this PhD work, the calculation of the statistical properties of Radio Halos and non-thermal phenomena as expected in the context of the re-acceleration model and their comparison with observations, is presented in Chapts.5, 6, 7 and 8. In Chapt.5 we present a first approach to semi-analytical calculations of statistical properties of giant Radio Halos. The main goal of this Chapter is to model cluster formation, the injection of turbulence in the ICM and the resulting particle acceleration process. We adopt the semi–analytic extended Press & Schechter (PS) theory to follow the formation of a large synthetic population of galaxy clusters and assume that during a merger a fraction of the PdV work done by the infalling subclusters in passing through the most massive one is injected in the form of magnetosonic waves. Then the processes of stochastic acceleration of the relativistic electrons by these waves and the properties of the ensuing synchrotron (Radio Halos) and inverse Compton (IC, hard X-ray) emission of merging clusters are computed under the assumption of a constant rms average magnetic field strength in emitting volume. The main finding of these calculations is that giant Radio Halos are naturally expected only in the more massive clusters, and that the expected fraction of clusters with Radio Halos is consistent with the observed one. In Chapt. 6 we extend the previous calculations by including a scaling of the magnetic field strength with cluster mass. The inclusion of this scaling allows us to derive the expected correlations between the synchrotron radio power of Radio Halos and the X-ray properties (T, LX) and mass of the hosting clusters. For the first time, we show that these correlations, calculated in the context of the re-acceleration model, are consistent with the observed ones for typical µG strengths of the average B intensity in massive clusters. The calculations presented in this Chapter allow us to derive the evolution of the probability to form Radio Halos as a function of the cluster mass and redshift. The most relevant finding presented in this Chapter is that the luminosity functions of giant Radio Halos at 1.4 GHz are expected to peak around a radio power » 1024 W/Hz and to flatten (or cut-off) at lower radio powers because of the decrease of the electron re-acceleration efficiency in smaller galaxy clusters. In Chapt. 6 we also derive the expected number counts of Radio Halos and compare them with available observations: we claim that » 100 Radio Halos in the Universe can be observed at 1.4 GHz with deep surveys, while more than 1000 Radio Halos are expected to be discovered in the next future by LOFAR at 150 MHz. This is the first (and so far unique) model expectation for the number counts of Radio Halos at lower frequency and allows to design future radio surveys. Based on the results of Chapt. 6, in Chapt.7 we present a work in progress on a “revision” of the occurrence of Radio Halos. We combine past results from the NVSS radio survey (z » 0.05 − 0.2) with our ongoing GMRT Radio Halos Pointed Observations of 50 X-ray luminous galaxy clusters (at z » 0.2−0.4) and discuss the possibility to test our model expectations with the number counts of Radio Halos at z » 0.05 − 0.4. The most relevant limitation in the calculations presented in Chapt. 5 and 6 is the assumption of an “averaged” size of Radio Halos independently of their radio luminosity and of the mass of the parent clusters. This assumption cannot be released in the context of the PS formalism used to describe the formation process of clusters, while a more detailed analysis of the physics of cluster mergers and of the injection process of turbulence in the ICM would require an approach based on numerical (possible MHD) simulations of a very large volume of the Universe which is however well beyond the aim of this PhD thesis. On the other hand, in Chapt.8 we report our discovery of novel correlations between the size (RH) of Radio Halos and their radio power and between RH and the cluster mass within the Radio Halo region, MH. In particular this last “geometrical” MH − RH correlation allows us to “observationally” overcome the limitation of the “average” size of Radio Halos. Thus in this Chapter, by making use of this “geometrical” correlation and of a simplified form of the re-acceleration model based on the results of Chapt. 5 and 6 we are able to discuss expected correlations between the synchrotron power and the thermal cluster quantities relative to the radio emitting region. This is a new powerful tool of investigation and we show that all the observed correlations (PR − RH, PR − MH, PR − T, PR − LX, . . . ) now become well understood in the context of the re-acceleration model. In addition, we find that observationally the size of Radio Halos scales non-linearly with the virial radius of the parent cluster, and this immediately means that the fraction of the cluster volume which is radio emitting increases with cluster mass and thus that the non-thermal component in clusters is not self-similar.

Development of analytical methodologies for iodine species in gaseous and particulate phases of the coastal atmosphere

It has been demonstrated that iodine does have an important influence on atmospheric chemistry, especially the formation of new particles and the enrichment of iodine in marine aerosols. It was pointed out that the most probable chemical species involved in the production or growth of these particles are iodine oxides, produced photochemically from biogenic halocarbon emissions and/or iodine emission from the sea surface. However, the iodine chemistry from gaseous to particulate phase in the coastal atmosphere and the chemical nature of the condensing iodine species are still not understood. A Tenax / Carbotrap adsorption sampling technique and a thermo-desorption / cryo-trap / GC-MS system has been further developed and improved for the volatile organic iodine species in the gas phase. Several iodo-hydrocarbons such as CH3I, C2H5I, CH2ICl, CH2IBr and CH2I2 etc., have been measured in samples from a calibration test gas source (standards), real air samples and samples from seaweeds / macro-algae emission experiments. A denuder sampling technique has been developed to characterise potential precursor compounds of coastal particle formation processes, such as molecular iodine in the gas phase. Starch, TMAH (TetraMethylAmmonium Hydroxide) and TBAH (TetraButylAmmonium Hydroxide) coated denuders were tested for their efficiencies to collect I2 at the inner surface, followed by a TMAH extraction and ICP/MS determination, adding tellurium as an internal standard. The developed method has been proved to be an effective, accurate and suitable process for I2 measurement in the field, with the estimated detection limit of ~0.10 ng∙L-1 for a sampling volume of 15 L. An H2O/TMAH-Extraction-ICP/MS method has been developed for the accurate and sensitive determination of iodine species in tropospheric aerosol particles. The particle samples were collected on cellulose-nitrate filters using conventional filter holders or on cellulose nitrate/tedlar-foils using a 5-stage Berner impactor for size-segregated particle analysis. The water soluble species as IO3- and I- were separated by anion exchanging process after water extraction. Non-water soluble species including iodine oxide and organic iodine were digested and extracted by TMAH. Afterwards the triple samples were analysed by ICP/MS. The detection limit for particulate iodine was determined to be 0.10~0.20 ng•m-3 for sampling volumes of 40~100 m3. The developed methods have been used in two field measurements in May 2002 and September 2003, at and around the Mace Head Atmospheric Research Station (MHARS) located at the west coast of Ireland. Elemental iodine as a precursor of the iodine chemistry in the coastal atmosphere, was determined in the gas phase at a seaweed hot-spot around the MHARS, showing I2 concentrations were in the range of 0~1.6 ng∙L-1 and indicating a positive correlation with the ozone concentration. A seaweed-chamber experiment performed at the field measurement station showed that the I2 emission rate from macro-algae was in the range of 0.019~0.022 ng•min-1•kg-1. During these experiments, nanometer-particle concentrations were obtained from the Scanning Mobility Particle Sizer (SMPS) measurements. Particle number concentrations were found to have a linear correlation with elemental iodine in the gas phase of the seaweeds chamber, showing that gaseous I2 is one of the important precursors of the new particle formation in the coastal atmosphere. Iodine contents in the particle phase were measured in both field campaigns at and around the field measurement station. Total iodine concentrations were found to be in the range of 1.0 ~ 21.0 ng∙m-3 in the PM2.5 samples. A significant correlation between the total iodine concentrations and the nanometer-particle number concentrations was observed. The particulate iodine species analysis indicated that iodide contents are usually higher than those of iodate in all samples, with ratios in the range of 2~5:1. It is possible that those water soluble iodine species are transferred through the sea-air interface into the particle phase. The ratio of water soluble (iodate + iodide) and non-water soluble species (probably iodine oxide and organic iodine compounds) was observed to be in the range of 1:1 to 1:2. It appears that higher concentrated non-water soluble species, as the products of the photolysis from the gas phase into the particle phase, can be obtained in those samples while the nucleation events occur. That supports the idea that iodine chemistry in the coastal boundary layer is linked with new particle formation events. Furthermore, artificial aerosol particles were formed from gaseous iodine sources (e.g. CH2I2) using a laboratory reaction-chamber experiment, in which the reaction constant of the CH2I2 photolysis was calculated to be based upon the first order reaction kinetic. The end products of iodine chemistry in the particle phase were identified and quantified.

Kontrollierte Fällung von amorphem Calciumcarbonat durch homogene Carbonatfreisetzung

In der Vergangenheit haben Untersuchung an biologischen und Modell-Systemen gezeigt, dass amorphes Calciumcarbonat als instabiles Zwischenprodukt bei der Bildung kristalliner Strukturen aus CaCO3 auftritt. Über dessen Rolle im Fällungsprozess von CaCO3 ist nicht viel bekannt und es wird davon ausgegangen, dass es als CaCO3-Speicher für die nachfolgenden kristallinen Produkte dient. Der genaue Reaktionsablauf, der zur Bildung von amorphem Calciumcarbonat (ACC) führt, ist nicht bekannt. Ziel dieser Arbeit war die Entwicklung einer Fällungstechnik, die die Beobachtung der Bildungskinetik von ACC durch Lichtstreuung ermöglicht. In Fällungsexperimenten wird gezeigt, dass die Fällung unter nicht-turbulenten Bedingungen zur Bildung von amorphem Calciumcarbonat führt. Hinsichtlich der Basen- und Alkylcarbonatmenge, die äquivalent oder im Überschuss zur Calciumionenkonzentration eingesetzt wird, entstehen zwei verschiedene Fällungsprodukte. In Bezug auf ihre chemische Zusammensetzung, thermische und mechanische Eigenschaften werden diese charakterisiert. In beiden Fällen wird ein amorphes CaCO3 mit einem Wassergehalt von 0,5 mol/L pro Mol CaCO3 erhalten. Die in situ Generierung von Carbonat führt zur Bildung von sphärischem amorphem Calciumcarbonat, das eine gewisse Tendenz zur Koazervation zeigt. Die bei gleichem Reaktionsumsatz beobachtete Temperaturabhängigkeit des Partikelradius konnten wir unter Annahme einer Mischungslücke mit unterer kritischer Mischungstemperatur interpretieren. Für die Bildung von amorphem Calciumcarbonat schlagen wir daher einen Mechanismus via binodaler flüssig-flüssig Entmischung vor. Nach einer kurzen Keimbildungsperiode können flüssige Tröpfchen aus wasserhaltigem CaCO3 wachsen und dann infolge von stetigem Wasserverlust glasartig erstarren und so amorphes Calciumcarbonat bilden. Bekräftigt wird dieses Modell durch die Wachstumskinetik, die mittels Lichtstreuung und SAXS verfolgt worden ist. In den Fällungsversuchen sind je nach Reaktionsbedingungen, zwei verschiedene Zeitgesetze des Teilchenwachstums erkennbar: Bei schneller Freisetzung von Carbonat liegt ein parabolischer Verlauf des Radienwachstums vor; hingegen führt eine langsame Freisetzung von Carbonat zu einem linearen Wachstum der Radien. Diese Abhängigkeiten lassen sich im Rahmen der bekannten Kinetik einer flüssig-flüssig Entmischung deuten. Ferner wird der Einfluss von doppelthydrophilen Blockcopolymeren (PEO-PMAA) auf die Teilchengröße und die Kinetik der Bildung von amorphem Calciumcarbonat untersucht. Zum Einsatz kommen zwei verschiedene Blockcopolymere, die sich in der Länge des PEO-Blocks unterscheiden. Im Fällungsexperiment führt das in sehr kleinen Konzentrationen vorliegende Blockcopolymere zur Stabilisierung von kleineren Partikeln. Das Blockcopolymer mit der längeren PEO-Einheit weist eine größere Effizienz auf. Die Ergebnisse lassen sich durch Annahme von Adsorption des Polymers an der Oberfläche interpretieren. Der Einfluss der doppelthydrophilen Blockcopolymere auf die Bildung von ACC deutet darauf, dass amorphes Calciumcarbonat eine komplexere Rolle als lediglich die eines Calciumcarbonatspeichers für das spätere Wachstum kristalliner Produkte einnimmt. Für die Wirkung von Polymerzusätzen muss somit nicht nur die Wechselwirkung mit den gegen Ende gebildeten Kristalle betrachtet werden, sondern auch der Einfluss, den das Polymer auf die Bildung des amorphen Calciumcarbonats hat. Die hier neu entwickelte Methode bietet die Möglichkeit, auch für komplexere Polymere, wie z.B. extrahierte Proteine, den Einfluss auf die Bildung der amorphen Vorstufe zu untersuchen.

Massenspektrometrische Untersuchungen und Nachweise von organischen Hydroperoxiden und höhermolekularen Verbindungen im biogenen sekundären organischen Aerosol

Atmosphärische Aerosole beeinflussen den Strahlungshaushalt und damit das Klima der Erde. Dies geschieht sowohl direkt (Streuung und Absorption), als auch indirekt (Wolkenkondensationskeime). Das sekundäre organische Aerosol (SOA) bildet einen wichtigen Bestandteil des atmosphärischen Aerosols. Seine Bildung erfolgt durch Reaktionen von Kohlenwasserstoffen mit atmosphärischen Oxidationsmitteln (z.B. Ozon, OH-Radikalen). Eine Klasse dieser Kohlenwasserstoffe sind die Terpene. Sie werden in großen Mengen durch die Vegetation emittiert und gelten als wichtige Vorläufersubstanzen des biogenen SOAs. In den Reaktionen von Monoterpenen und Sesquiterpenen mit atmosphärischen Reaktionspartnern wird eine große Vielfalt an multifunktionellen Reaktionsprodukten gebildet, von denen bis heute nur ein Bruchteil identifiziert werden konnte. In der vorliegenden Arbeit soll im Speziellen die Bildung von organischen Peroxiden und oligomeren Verbindungen im biogenen SOA untersucht und Nachweise einzelner Moleküle erbracht werden.rnFür eine Identifizierung von organischen Peroxiden aus der Oxidation einzelner Monoterpene und Sesquiterpene mit Ozon wurden die Reaktionsprodukte direkt in eine bei Atmosphärendruck arbeitende chemische Ionisationsquelle überführt und massenspektrometrisch untersucht (online-APCI-MS). Hierdurch konnten organische Hydroperoxide in der Partikelphase nachgewiesen werden, welche sich durch eine signifikante Abspaltung von H2O2 im Tandem-Massenspektrum (MS/MS) auszeichneten. Des Weiteren sollte die Bildung von höhermolekularen Verbindungen („Dimere“) im SOA des α-Pinens untersucht werden. Hierfür wurden zunächst die Reaktionsprodukte des Cyclohexens, das als einfache Modellverbindung des α-Pinens dient, mittels online-APCI-MS und offline durch Flüssigkeitschromatographie und Elektrospray-Ionenfallenmassenspektrometrie (HPLC/ESI-MS) untersucht. Verschiedene Produkte der Cyclohexen-Ozonolyse konnten hierbei als Esterverbindungen identifiziert werden, wobei eigens synthetisierte Referenzsubstanzen für die Identifizierung verwendet wurden. In einem weiteren Experiment, indem gleichzeitig Cyclohexen und α-Pinen mit Ozon umgesetzt wurden, konnten ebenfalls eine Bildung von höhermolekularen Estern nachgewiesen werden. Es handelte sich hierbei um „Mischester“, deren Struktur aus Reaktionsprodukten der beiden VOC-Vorläufermoleküle aufgebaut war. Durch diese neuen Erkenntnisse, über die Bildung von Estern im SOA des Cyclohexens, wurden die Dimer-Bildung einer reinen α-Pinen/Ozon-Reaktion online und offline massenspektrometrisch untersucht. Hier stellten sich als Hauptprodukte die Verbindungen mit m/z 357 und m/z 367 ([M-H]--Ionen) heraus, welche zudem erstmals auf einem Filter einer Realprobe aus Hyytiälä, Finnland nachgewiesen werden konnten. Aufgrund ihrer Fragmentierung in MS/MS-Untersuchungen sowie den exakten Summenformeln aus FT-MS Messungen konnte für die Struktur der höhermolekularen Verbindung mit m/z 367 ebenfalls ein Ester und für m/z 357 ein Peroxyhemiacetal vorgeschlagen werden. Die vorgeschlagene Struktur der Verbindung m/z 367 konnte im Anschluss über eine Reaktion aus Hydroxypinonsäure mit Pinsäure bestätigt werden. Die Identifizierung der Esterverbindung des α-Pinen-SOA erfolgte ebenfalls mit Hilfe von LC-MSn-Messungen.rnDie bisher diskutierten Ergebnisse, sowie die meisten in der Literatur beschriebenen Studien befassen sich jedoch mit einzelnen Vorläuferverbindungen, im Gegensatz zu den komplexen SOA-Proben aus den Emissionen der Vegetation. Im Rahmen einer Messkampagne am Forschungszentrum Jülich erfolgte eine massenspektrometrische Charakterisierung (online-APCI-MS) des SOAs aus direkten VOC-Emissionen von Pflanzen. Durch einen Vergleich der Produktverteilung dieser erhalten online-Massenspektren mit denen aus den Reaktionen einzelner VOCs, konnten Aussagen über die in den Reaktionen umgesetzten VOCs gemacht werden. Es konnte gezeigt werden, dass in stressbedingten Situationen die untersuchten Exemplare der Betula pendula (Birke) hauptsächlich Sesquiterpene, Picea abies (Fichte) eher Monoterpene und Eucalyptus (Eukalyptus) sowohl Sesquiterpene als auch Monoterpene emittieren. Um die atmosphärischen Prozesse, die zur Bildung der Produkte im SOA führen vollständig zu verstehen, müssen jedoch noch weitere Anstrengungen unternommen werden.rn

Integrated analysis and design of optimization and up-scaling of inductively coupled plasma synthesis of nanoparticles

This study is focused on radio-frequency inductively coupled thermal plasma (ICP) synthesis of nanoparticles, combining experimental and modelling approaches towards process optimization and industrial scale-up, in the framework of the FP7-NMP SIMBA European project (Scaling-up of ICP technology for continuous production of Metallic nanopowders for Battery Applications). First the state of the art of nanoparticle production through conventional and plasma routes is summarized, then results for the characterization of the plasma source and on the investigation of the nanoparticle synthesis phenomenon, aiming at highlighting fundamental process parameters while adopting a design oriented modelling approach, are presented. In particular, an energy balance of the torch and of the reaction chamber, employing a calorimetric method, is presented, while results for three- and two-dimensional modelling of an ICP system are compared with calorimetric and enthalpy probe measurements to validate the temperature field predicted by the model and used to characterize the ICP system under powder-free conditions. Moreover, results from the modeling of critical phases of ICP synthesis process, such as precursor evaporation, vapour conversion in nanoparticles and nanoparticle growth, are presented, with the aim of providing useful insights both for the design and optimization of the process and on the underlying physical phenomena. Indeed, precursor evaporation, one of the phases holding the highest impact on industrial feasibility of the process, is discussed; by employing models to describe particle trajectories and thermal histories, adapted from the ones originally developed for other plasma technologies or applications, such as DC non-transferred arc torches and powder spherodization, the evaporation of micro-sized Si solid precursor in a laboratory scale ICP system is investigated. Finally, a discussion on the role of thermo-fluid dynamic fields on nano-particle formation is presented, as well as a study on the effect of the reaction chamber geometry on produced nanoparticle characteristics and process yield.

Aggregation of hybrid molecules and film formation of colloidal monolayers

A unique characteristic of soft matter is its ability to self-assemble into larger structures. Characterizing these structures is crucial for their applications. In the first part of this work, I investigated DNA-organic hybrid material by means of Fluorescence Correlation Spectroscopy (FCS) and Fluorescence Cross-Correlation Spectroscopy (FCCS). DNA-organic hybrid materials, a novel class of hybrid materials composed of synthetic macromolecules and oligodeoxynucleotide segmenta, are mostly amphiphilic and can self-assemble into supramolecular structures in aqueous solution. A hybrid material of a fluorophore, perylenediimide (PDI), and a DNA segment (DNA-PDI) has been developed in Prof. A. Hermann’s group (University of Groningen). This novel material has the ability to form aggregates through pi-pi stacking between planar PDIs and can be traced in solution due to the fluorescence of PDI. I have determined the diffusion coefficient of DNA-PDI conjugates in aqueous solution by means of FCS. In addition, I investigated whether such DNA-PDIs form aggregates with certain structure, for instance dimers. rnOnce the DNA hybrid material self-assemble into supermolecular structures for instance into micelles, the single molecules do not necessarily stay in one specific micelle. Actually, a single molecule may enter and leave micelles constantly. The average residence time of a single molecule in a certain micelle depends on the nature of the molecule. I have chosen DNA-b-polypropylene oxide (PPO) as model molecules and investigated the residence time of DNA-b-PPO molecules in their according micelles by means of FCCS.rnBesides the DNA hybrid materials, polymeric colloids can also form ordered structures once they are brought to an air/water interface. Here, hexagonally densely packed monolayers can be generated. These monolayers can be deposited onto different surfaces as coating layers. In the second part of this work, I investigated the mechanical properties of such colloidal monolayers using micromechanical cantilevers. When a coating layer is deposited on a cantilever, it can modify the elasticity of the cantilever. This variation can be reflected either by a deflection or by a resonance frequency shift of the cantilever. In turn, detecting these changes provides information about the mechanical properties of the coating layer. rnIn the second part of this work, polymeric colloidal monolayers were coated on a cantilever and homogenous polymer films of a few hundred nanometers in thickness were generated from these colloidal monolayers by thermal annealing or organic vapor annealing. Both the film formation process and the mechanical properties of these resulting homogenous films were investigated by means of cantilever. rnElastic property changes of the coating film, for example upon absorption of organic vapors, induce a deflection of the cantilever. This effect enables a cantilever to detect target molecules, when the cantilever is coated with an active layer with specific affinity to target molecules. In the last part of this thesis, I investigated the applicability of suitably functionalized micromechanical cantilevers as sensors. In particular, glucose sensitive polymer brushes were grafted on a cantilever and the deflection of this cantilever was measured during exposure to glucose solution. rn

Formation and surface exchange of nitrous acid

Die salpetrige Säure (HONO) ist eine der reaktiven Stickstoffkomponenten der Atmosphäre und Pedosphäre. Die genauen Bildungswege von HONO, sowie der gegenseitige Austausch von HONO zwischen Atmosphäre und Pedosphäre sind noch nicht vollständig aufgedeckt. Bei der HONO-Photolyse entsteht das Hydroxylradikal (OH) und Stickstoffmonooxid (NO), was die Bedeutsamkeit von HONO für die atmosphärische Photochemie widerspiegelt.rnUm die genannte Bildung von HONO im Boden und dessen anschließenden Austausch mit der Atmosphäre zu untersuchen, wurden Messungen von Bodenproben mit dynamischen Kammern durchgeführt. Im Labor gemessene Emissionsflüsse von Wasser, NO und HONO zeigen, dass die Emission von HONO in vergleichbarem Umfang und im gleichen Bodenfeuchtebereich wie die für NO (von 6.5 bis 56.0 % WHC) stattfindet. Die Höhe der HONO-Emissionsflüsse bei neutralen bis basischen pH-Werten und die Aktivierungsenergie der HONO-Emissionsflüsse führen zu der Annahme, dass die mikrobielle Nitrifikation die Hauptquelle für die HONO-Emission darstellt. Inhibierungsexperimente mit einer Bodenprobe und die Messung einer Reinkultur von Nitrosomonas europaea bestärkten diese Theorie. Als Schlussfolgerung wurde das konzeptionelle Model der Bodenemission verschiedener Stickstoffkomponenten in Abhängigkeit von dem Wasserhaushalt des Bodens für HONO erweitert.rnIn einem weiteren Versuch wurde zum Spülen der dynamischen Kammer Luft mit erhöhtem Mischungsverhältnis von HONO verwendet. Die Messung einer hervorragend charakterisierten Bodenprobe zeigte bidirektionale Flüsse von HONO. Somit können Böden nicht nur als HONO-Quelle, sondern auch je nach Bedingungen als effektive Senke dienen. rnAußerdem konnte gezeigt werden, dass das Verhältnis von HONO- zu NO-Emissionen mit dem pH-Wert des Bodens korreliert. Grund könnte die erhöhte Reaktivität von HONO bei niedrigem pH-Wert und die längere Aufenthaltsdauer von HONO verursacht durch reduzierte Gasdiffusion im Bodenporenraum sein, da ein niedriger pH-Wert mit erhöhter Bodenfeuchte am Maximum der Emission einhergeht. Es konnte gezeigt werden, dass die effektive Diffusion von Gasen im Bodenporenraum und die effektive Diffusion von Ionen in der Bodenlösung die HONO-Produktion und den Austausch von HONO mit der Atmosphäre begrenzen. rnErgänzend zu den Messungen im Labor wurde HONO während der Messkampagne HUMPPA-COPEC 2010 im borealen Nadelwald simultan in der Höhe von 1 m über dem Boden und 2 bis 3 m über dem Blätterdach gemessen. Die Budgetberechnungen für HONO zeigen, dass für HONO sämtliche bekannte Quellen und Senken in Bezug auf die übermächtige HONO-Photolyserate tagsüber vernachlässigbar sind (< 20%). Weder Bodenemissionen von HONO, noch die Photolyse von an Oberflächen adsorbierter Salpetersäure können die fehlende Quelle erklären. Die lichtinduzierte Reduktion von Stickstoffdioxid (NO2) an Oberflächen konnte nicht ausgeschlossen werden. Es zeigte sich jedoch, dass die fehlende Quelle stärker mit der HONO-Photolyserate korreliert als mit der entsprechenden Photolysefrequenz, die proportional zur Photolysefrequenz von NO2 ist. Somit lässt sich schlussfolgern, dass entweder die Photolyserate von HONO überschätzt wird oder dass immer noch eine unbekannte, HONO-Quelle existiert, die mit der Photolyserate sehr stark korreliert. rn rn

Analyse der intrazellulären Freisetzung von Wirkstoffmodellen via konfokaler Laser-Raster-Mikroskopie

In der vorliegenden Arbeit wurde gezeigt, wie man das Potential nanopartikulärer Systeme, die vorwiegend via Miniemulsion hergestellt wurden, im Hinblick auf „Drug Delivery“ ausnutzen könnte, indem ein Wirkstoffmodell auf unterschiedliche Art und Weise intrazellulär freigesetzt wurde. Dies wurde hauptsächlich mittels konfokaler Laser-Raster-Mikrokopie (CLSM) in Kombination mit dem Bildbearbeitungsprogramm Volocity® analysiert.rnPBCA-Nanokapseln eigneten sich besonders, um hydrophile Substanzen wie etwa Oligonukleotide zu verkapseln und sie so auf ihrem Transportweg in die Zellen vor einem etwaigen Abbau zu schützen. Es konnte eine Freisetzung der Oligonukleotide in den Zellen aufgrund der elektrostatischen Anziehung des mitochondrialen Membranpotentials nachgewiesen werden. Dabei war die Kombination aus Oligonukleotid und angebundenem Cyanin-Farbstoff (Cy5) an der 5‘-Position der Oligonukleotid-Sequenz ausschlaggebend. Durch quantitative Analysen mittels Volocity® konnte die vollständige Kolokalisation der freigesetzten Oligonukleotide an Mitochondrien bewiesen werden, was anhand der Kolokalisationskoeffizienten „Manders‘ Coefficients“ M1 und M2 diskutiert wurde. Es konnte ebenfalls aufgrund von FRET-Studien doppelt markierter Oligos gezeigt werden, dass die Oligonukleotide weder beim Transport noch bei der Freisetzung abgebaut wurden. Außerdem wurde aufgeklärt, dass nur der Inhalt der Nanokapseln, d. h. die Oligonukleotide, an Mitochondrien akkumulierte, das Kapselmaterial selbst jedoch in anderen intrazellulären Bereichen aufzufinden war. Eine Kombination aus Cyanin-Farbstoffen wie Cy5 mit einer Nukleotidsequenz oder einem Wirkstoff könnte also die Basis für einen gezielten Wirkstofftransport zu Mitochondrien liefern bzw. die Grundlage schaffen, eine Freisetzung aus Kapseln ins Zytoplasma zu gewährleisten.rnDer vielseitige Einsatz der Miniemulsion gestattete es, nicht nur Kapseln sondern auch Nanopartikel herzustellen, in welchen hydrophobe Substanzen im Partikelkern eingeschlossen werden konnten. Diese auf hydrophobe Wechselwirkungen beruhende „Verkapselung“ eines Wirkstoffmodells, in diesem Fall PMI, wurde bei PDLLA- bzw. PS-Nanopartikeln ausgenutzt, welche durch ein HPMA-basiertes Block-Copolymer stabilisiert wurden. Dabei konnte gezeigt werden, dass das hydrophobe Wirkstoffmodell PMI innerhalb kürzester Zeit in die Zellen freigesetzt wurde und sich in sogenannte „Lipid Droplets“ einlagerte, ohne dass die Nanopartikel selbst aufgenommen werden mussten. Daneben war ein intrazelluläres Ablösen des stabilisierenden Block-Copolymers zu verzeichnen, welches rn8 h nach Partikelaufnahme erfolgte und ebenfalls durch Analysen mittels Volocity® untermauert wurde. Dies hatte jedoch keinen Einfluss auf die eigentliche Partikelaufnahme oder die Freisetzung des Wirkstoffmodells. Ein großer Vorteil in der Verwendung des HPMA-basierten Block-Copolymers liegt darin begründet, dass auf zeitaufwendige Waschschritte wie etwa Dialyse nach der Partikelherstellung verzichtet werden konnte, da P(HPMA) ein biokompatibles Polymer ist. Auf der anderen Seite hat man aufgrund der Syntheseroute dieses Block-Copolymers vielfältige Möglichkeiten, Funktionalitäten wie etwa Fluoreszenzmarker einzubringen. Eine kovalente Anbindung eines Wirkstoffs ist ebenfalls denkbar, welcher intrazellulär z. B. aufgrund von enzymatischen Abbauprozessen langsam freigesetzt werden könnte. Somit bietet sich die Möglichkeit mit Nanopartikeln, die durch HPMA-basierte Block-Copolymere stabilisiert wurden, gleichzeitig zwei unterschiedliche Wirkstoffe in die Zellen zu bringen, wobei der eine schnell und der zweite über einen längeren Zeitraum hinweg (kontrolliert) freigesetzt werden könnte.rnNeben Nanokapseln sowie –partikeln, die durch inverse bzw. direkte Miniemulsion dargestellt wurden, sind auch Nanohydrogelpartikel untersucht worden, die sich aufgrund von Selbstorganisation eines amphiphilen Bock-Copolymers bildeten. Diese Nanohydrogelpartikel dienten der Komplexierung von siRNA und wurden hinsichtlich ihrer Anreicherung in Lysosomen untersucht. Aufgrund der Knockdown-Studien von Lutz Nuhn konnte ein Unterschied in der Knockdown-Effizienz festgestellt werden, je nach dem, ob 100 nm oder 40 nm große Nanohydrogelpartikel verwendet wurden. Es sollte festgestellt werden, ob eine größenbedingte, unterschiedlich schnelle Anreicherung dieser beiden Partikel in Lysosomen erfolgte, was die unterschiedliche Knockdown-Effizienz erklären könnte. CLSM-Studien und quantitative Kolokalisationsstudien gaben einen ersten Hinweis auf diese Größenabhängigkeit. rnBei allen verwendeten nanopartikulären Systemen konnte eine Freisetzung ihres Inhalts gezeigt werden. Somit bieten sie ein großes Potential als Wirkstoffträger für biomedizinische Anwendungen.rn

Aerosol-cloud interactions studied with a chemistry-climate model

This study aims at a comprehensive understanding of the effects of aerosol-cloud interactions and their effects on cloud properties and climate using the chemistry-climate model EMAC. In this study, CCN activation is regarded as the dominant driver in aerosol-cloud feedback loops in warm clouds. The CCN activation is calculated prognostically using two different cloud droplet nucleation parameterizations, the STN and HYB CDN schemes. Both CDN schemes account for size and chemistry effects on the droplet formation based on the same aerosol properties. The calculation of the solute effect (hygroscopicity) is the main difference between the CDN schemes. The kappa-method is for the first time incorporated into Abdul-Razzak and Ghan activation scheme (ARG) to calculate hygroscopicity and critical supersaturation of aerosols (HYB), and the performance of the modied scheme is compared with the osmotic coefficient model (STN), which is the standard in the ARG scheme. Reference simulations (REF) with the prescribed cloud droplet number concentration have also been carried out in order to understand the effects of aerosol-cloud feedbacks. In addition, since the calculated cloud coverage is an important determinant of cloud radiative effects and is influencing the nucleation process two cloud cover parameterizations (i.e., a relative humidity threshold; RH-CLC and a statistical cloud cover scheme; ST-CLC) have been examined together with the CDN schemes, and their effects on the simulated cloud properties and relevant climate parameters have been investigated. The distinct cloud droplet spectra show strong sensitivity to aerosol composition effects on cloud droplet formation in all particle sizes, especially for the Aitken mode. As Aitken particles are the major component of the total aerosol number concentration and CCN, and are most sensitive to aerosol chemical composition effect (solute effect) on droplet formation, the activation of Aitken particles strongly contribute to total cloud droplet formation and thereby providing different cloud droplet spectra. These different spectra influence cloud structure, cloud properties, and climate, and show regionally varying sensitivity to meteorological and geographical condition as well as the spatiotemporal aerosol properties (i.e., particle size, number, and composition). The changes responding to different CDN schemes are more pronounced at lower altitudes than higher altitudes. Among regions, the subarctic regions show the strongest changes, as the lower surface temperature amplifies the effects of the activated aerosols; in contrast, the Sahara desert, where is an extremely dry area, is less influenced by changes in CCN number concentration. The aerosol-cloud coupling effects have been examined by comparing the prognostic CDN simulations (STN, HYB) with the reference simulation (REF). Most pronounced effects are found in the cloud droplet number concentration, cloud water distribution, and cloud radiative effect. The aerosol-cloud coupling generally increases cloud droplet number concentration; this decreases the efficiency of the formation of weak stratiform precipitation, and increases the cloud water loading. These large-scale changes lead to larger cloud cover and longer cloud lifetime, and contribute to high optical thickness and strong cloud cooling effects. This cools the Earth's surface, increases atmospheric stability, and reduces convective activity. These changes corresponding to aerosol-cloud feedbacks are also differently simulated depending on the cloud cover scheme. The ST-CLC scheme is more sensitive to aerosol-cloud coupling, since this scheme uses a tighter linkage of local dynamics and cloud water distributions in cloud formation process than the RH-CLC scheme. For the calculated total cloud cover, the RH-CLC scheme simulates relatively similar pattern to observations than the ST-CLC scheme does, but the overall properties (e.g., total cloud cover, cloud water content) in the RH simulations are overestimated, particularly over ocean. This is mainly originated from the difference in simulated skewness in each scheme: the RH simulations calculate negatively skewed distributions of cloud cover and relevant cloud water, which is similar to that of the observations, while the ST simulations yield positively skewed distributions resulting in lower mean values than the RH-CLC scheme does. The underestimation of total cloud cover over ocean, particularly over the intertropical convergence zone (ITCZ) relates to systematic defficiency of the prognostic calculation of skewness in the current set-ups of the ST-CLC scheme.rnOverall, the current EMAC model set-ups perform better over continents for all combinations of the cloud droplet nucleation and cloud cover schemes. To consider aerosol-cloud feedbacks, the HYB scheme is a better method for predicting cloud and climate parameters for both cloud cover schemes than the STN scheme. The RH-CLC scheme offers a better simulation of total cloud cover and the relevant parameters with the HYB scheme and single-moment microphysics (REF) than the ST-CLC does, but is not very sensitive to aerosol-cloud interactions.

The Investigation of Uniform, Monodisperse Crystalline Particles via the Evaporation of Small Droplets

Many industrial solids processes require the production of disperse particles. In industries such as food, personal care, and pharmaceuticals, particle formation is widely used to produce solid products or to separate substances in intermediate process steps. The most important characteristics known to impact the effectiveness of a solid product are purity, size, internal structure, and morphology. These characteristics are essential to maintain optimal operation of subsequent process steps and for obtaining the desired high quality product. This thesis aims to aid in the advancement of particle production technology by (1) investigating the use of a vibrating orifice aerosol generator (VOAG) for collecting data to predict particle attributes including morphology, size, and internal structure as a function of processing parameters such as solvent, solution concentration, air flow rate, and initial droplet size, as well as to (2) determine the extent to which uniform droplet evaporation can be a tool to achieve novel particle morphologies, controlled sizes, or internal structures (crystallinity and crystal form). Experimental results for succinic acid, L-serine, and L-glutamic acid suggest that particles of controlled characteristics can indeed be produced by this method. Analysis by scanning electron microscopy (SEM), nanoindentation, and X-ray diffraction (XRD) shows that various sizes, internal structures, and morphologies can be obtained using the VOAG. Furthermore, unique morphologies and unexpected internal structures were able to be achieved for succinic acid, providing an added benefit to particle formation by this method.