Phytoplankton community composition and size-abundance spectra in areas of the Alborán sea with different hydrological characteristics

[EN] Size-abundance spectra (SAS) were analyzed in different phytoplankton assemblages of the Alborán Sea collected in areas with contrasting hydrological features (upwelling areas and anticyclonic gyre). Abundance of micro-plankton cells decreased following the hydrological gradient from the most productive stations towards offshore stations. This size-fraction of phytoplankton was dominated by diatoms. Pico-plankton followed an opposite gradient. Concordantly, the slope of the SAS trended to decrease from coastal areas (upwelling) towards the anticyclonic gyre. However, phytoplankton assemblages featuring similar SAS values presented a quite different taxonomical composition of their diatom communities. According to the previous available information about the taxonomical composition of the phytoplankton communities in the Alborán Sea, these differences in diatom composition are indicative of differences in productivity of the phytoplankton. Consequently, the utility of phytoplankton SAS as an indicator of changes in the phytoplankton communities of the Alborán Sea is discussed.

Development of the optimal estimation method for inversion of stratospheric emission spectra and validation of HNO3 profiles

This doctoral thesis focuses on ground-based measurements of stratospheric nitric acid (HNO3)concentrations obtained by means of the Ground-Based Millimeter-wave Spectrometer (GBMS). Pressure broadened HNO3 emission spectra are analyzed using a new inversion algorithm developed as part of this thesis work and the retrieved vertical profiles are extensively compared to satellite-based data. This comparison effort I carried out has a key role in establishing a long-term (1991-2010), global data record of stratospheric HNO3, with an expected impact on studies concerning ozone decline and recovery. The first part of this work is focused on the development of an ad hoc version of the Optimal Estimation Method (Rodgers, 2000) in order to retrieve HNO3 spectra observed by means of GBMS. I also performed a comparison between HNO3 vertical profiles retrieved with the OEM and those obtained with the old iterative Matrix Inversion method. Results show no significant differences in retrieved profiles and error estimates, with the OEM providing however additional information needed to better characterize the retrievals. A final section of this first part of the work is dedicated to a brief review on the application of the OEM to other trace gases observed by GBMS, namely O3 and N2O. The second part of this study deals with the validation of HNO3 profiles obtained with the new inversion method. The first step has been the validation of GBMS measurements of tropospheric opacity, which is a necessary tool in the calibration of any GBMS spectra. This was achieved by means of comparisons among correlative measurements of water vapor column content (or Precipitable Water Vapor, PWV) since, in the spectral region observed by GBMS, the tropospheric opacity is almost entirely due to water vapor absorption. In particular, I compared GBMS PWV measurements collected during the primary field campaign of the ECOWAR project (Bhawar et al., 2008) with simultaneous PWV observations obtained with Vaisala RS92k radiosondes, a Raman lidar, and an IR Fourier transform spectrometer. I found that GBMS PWV measurements are in good agreement with the other three data sets exhibiting a mean difference between observations of ~9%. After this initial validation, GBMS HNO3 retrievals have been compared to two sets of satellite data produced by the two NASA/JPL Microwave Limb Sounder (MLS) experiments (aboard the Upper Atmosphere Research Satellite (UARS) from 1991 to 1999, and on the Earth Observing System (EOS) Aura mission from 2004 to date). This part of my thesis is inserted in GOZCARDS (Global Ozone Chemistry and Related Trace gas Data Records for the Stratosphere), a multi-year project, aimed at developing a long-term data record of stratospheric constituents relevant to the issues of ozone decline and expected recovery. This data record will be based mainly on satellite-derived measurements but ground-based observations will be pivotal for assessing offsets between satellite data sets. Since the GBMS has been operated for more than 15 years, its nitric acid data record offers a unique opportunity for cross-calibrating HNO3 measurements from the two MLS experiments. I compare GBMS HNO3 measurements obtained from the Italian Alpine station of Testa Grigia (45.9° N, 7.7° E, elev. 3500 m), during the period February 2004 - March 2007, and from Thule Air Base, Greenland (76.5°N 68.8°W), during polar winter 2008/09, and Aura MLS observations. A similar intercomparison is made between UARS MLS HNO3 measurements with those carried out from the GBMS at South Pole, Antarctica (90°S), during the most part of 1993 and 1995. I assess systematic differences between GBMS and both UARS and Aura HNO3 data sets at seven potential temperature levels. Results show that, except for measurements carried out at Thule, ground based and satellite data sets are consistent within the errors, at all potential temperature levels.

Identified primary hadron spectra with the TOF detector of the ALICE experiment at LHC

In this thesis the analysis to reconstruct the transverse momentum p_{t} spectra for pions, kaons and protons identified with the TOF detector of the ALICE experiment in pp Minimum Bias collisions at $\sqrt{s}=7$ TeV was reported. After a detailed description of all the parameters which influence the TOF PID performance (time resolution, calibration, alignment, matching efficiency, time-zero of the event) the method used to identify the particles, the unfolding procedure, was discussed. With this method, thanks also to the excellent TOF performance, the pion and kaon spectra can be reconstructed in the 0.5

Ab-initio determination of x-ray absorption near edge structure (xanes) spectra in an ultrasoft and norm conserving pseudopotentials scheme

X-ray absorption spectroscopy (XAS) is a powerful means of investigation of structural and electronic properties in condensed -matter physics. Analysis of the near edge part of the XAS spectrum, the so – called X-ray Absorption Near Edge Structure (XANES), can typically provide the following information on the photoexcited atom: - Oxidation state and coordination environment. - Speciation of transition metal compounds. - Conduction band DOS projected on the excited atomic species (PDOS). Analysis of XANES spectra is greatly aided by simulations; in the most common scheme the multiple scattering framework is used with the muffin tin approximation for the scattering potential and the spectral simulation is based on a hypothetical, reference structure. This approach has the advantage of requiring relatively little computing power but in many cases the assumed structure is quite different from the actual system measured and the muffin tin approximation is not adequate for low symmetry structures or highly directional bonds. It is therefore very interesting and justified to develop alternative methods. In one approach, the spectral simulation is based on atomic coordinates obtained from a DFT (Density Functional Theory) optimized structure. In another approach, which is the object of this thesis, the XANES spectrum is calculated directly based on an ab – initio DFT calculation of the atomic and electronic structure. This method takes full advantage of the real many-electron final wavefunction that can be computed with DFT algorithms that include a core-hole in the absorbing atom to compute the final cross section. To calculate the many-electron final wavefunction the Projector Augmented Wave method (PAW) is used. In this scheme, the absorption cross section is written in function of several contributions as the many-electrons function of the finale state; it is calculated starting from pseudo-wavefunction and performing a reconstruction of the real-wavefunction by using a transform operator which contains some parameters, called partial waves and projector waves. The aim of my thesis is to apply and test the PAW methodology to the calculation of the XANES cross section. I have focused on iron and silicon structures and on some biological molecules target (myoglobin and cytochrome c). Finally other inorganic and biological systems could be taken into account for future applications of this methodology, which could become an important improvement with respect to the multiscattering approach.

Studies of pure rotational spectra of isolated molecules and molecular adducts using pulsed jet Fourier transform microwave (PJ-FTM) spectroscopy

This thesis focuses on studying molecular structure and internal dynamics by using pulsed jet Fourier transform microwave (PJ-FTMW) spectroscopy combined with theoretical calculations. Several kinds of interesting chemical problems are investigated by analyzing the MW spectra of the corresponding molecular systems. First, the general aspects of rotational spectroscopy are summarized, and then the basic theory on molecular rotation and experimental method are described briefly. ab initio and density function theory (DFT) calculations that used in this thesis to assist the assignment of rotational spectrum are also included. From chapter 3 to chapter 8, several molecular systems concerning different kind of general chemical problems are presented. In chapter 3, the conformation and internal motions of dimethyl sulfate are reported. The internal rotations of the two methyl groups split each rotational transition into several components line, allowing for the determination of accurate values of the V3 barrier height to internal rotation and of the orientation of the methyl groups with respect to the principal axis system. In chapter 4 and 5, the results concerning two kinds of carboxylic acid bi-molecules, formed via two strong hydrogen bonds, are presented. This kind of adduct is interesting also because a double proton transfer can easily take place, connecting either two equivalent or two non-equivalent molecular conformations. Chapter 6 concerns a medium strong hydrogen bonded molecular complex of alcohol with ether. The dimer of ethanol-dimethylether was chosen as the model system for this purpose. Chapter 7 focuses on weak halogen…H hydrogen bond interaction. The nature of O-H…F and C-H…Cl interaction has been discussed through analyzing the rotational spectra of CH3CHClF/H2O. In chapter 8, two molecular complexes concerning the halogen bond interaction are presented.

Generating vegetation-spectra as a basis for global monitoring of annual vegetation cycles using DOAS satellite observations

Vegetation-cycles are of general interest for many applications. Be it for harvest-predictions, global monitoring of climate-change or as input to atmospheric models.rnrnCommon Vegetation Indices use the fact that for vegetation the difference between Red and Near Infrared reflection is higher than in any other material on Earth’s surface. This gives a very high degree of confidence for vegetation-detection.rnrnThe spectrally resolving data from the GOME and SCIAMACHY satellite-instrumentsrnprovide the chance to analyse finer spectral features throughout the Red and Near Infrared spectrum using Differential Optical Absorption Spectroscopy (DOAS). Although originally developed to retrieve information on atmospheric trace gases, we use it to gain information on vegetation. Another advantage is that this method automatically corrects for changes in the atmosphere. This renders the vegetation-information easily comparable over long time-spans.rnThe first results using previously available reference spectra were encouraging, but also indicated substantial limitations of the available reflectance spectra of vegetation. This was the motivation to create new and more suitable vegetation reference spectra within this thesis.rnThe set of reference spectra obtained is unique in its extent and also with respect to its spectral resolution and the quality of the spectral calibration. For the first time, this allowed a comprehensive investigation of the high-frequency spectral structures of vegetation reflectance and of their dependence on the viewing geometry.rnrnThe results indicate that high-frequency reflectance from vegetation is very complex and highly variable. While this is an interesting finding in itself, it also complicates the application of the obtained reference spectra to the spectral analysis of satellite observations.rnrnThe new set of vegetation reference spectra created in this thesis opens new perspectives for research. Besides refined satellite analyses, these spectra might also be used for applications on other platforms such as aircraft. First promising studies have been presented in this thesis, but the full potential for the remote sensing of vegetation from satellite (or aircraft) could bernfurther exploited in future studies.

Synthese von Sialyl-Lewis-X-Mimetika durch stereoselektive ortho-C-Glycosylierung von Phenolen

Ziel der Arbeit war es, Sialyl-LewisX-Mimetika auf Basis ortho-C-glycosylierter Phenole als Inhibitoren für die Selektin-Ligand-Wechselwirkungen zu synthetisieren. Dazu wurde zunächst die Stereoselektivität der ortho-C-Mannosylierung untersucht. Dabei wurde gezeigt, dass bei der Umsetzung von Phenolen mit dem benzylgeschützten Mannosyl-trichloracetimidat in Gegenwart von TMSOTf selektiv das β-C-Mannosid erhalten wurde. Gleichzeitig konnte anhand der NMR-spektroskopischen Untersuchungen nachgewiesen werden, dass die in der Literatur beschriebenen α-C-Mannoside von Phenolen tatsächlich β-konfiguriert sind. Wenn Naphthole als Glycosylakzeptoren verwendet wurden, konnten durch Modifikation des Promotors auch die für die Synthese der Mimetika benötigten α-C-Mannoside erhalten werden, wobei ZnCl2 als Promotor die besten Ergebnisse lieferte. Allerdings zeigten die synthetisierten α-C-Mannoside und α-C-Galactoside eine Inversion des Pyranoseringes und lagen in der ungewöhnlichen 1C4-Konformation vor.rnAnschließend konnte auf diese Weise das durch Docking-Studien gefundene Mimetikum (2S)-3-Cyclohexyl-2-[7-hydroxy-8-(α-D-mannosyl)naphthalin-2-yloxy]propionsäure syntheti-siert werden. Es besaß jedoch in Zelladhäsionstests keine ausreichende Aktivität bei der Inhibierung der Selektin-Ligand-Wechselwirkung. Bei den ursprünglichen Dockingstudien war allerdings von der gewohnten 4C1-Konformation ausgegangen worden. Spätere NMR-Experimente und DFT-Berechnungen zeigten, dass das Mimetikum tatsächlich in der 1C4-Konformation vorlag und es deshalb nicht aktiv war. Die synthetisierten Stereo- und Regioisomere zeigten in Zelladhäsionstests ebenfalls keine Aktivität.rnVersuche, die α-1-C-Mannosylnaphthole zu den benötigten 1-C-2-O-Diglycosyl-naphthalinen umzusetzen waren nicht erfolgreich, da die phenolische OH-Gruppe sterisch zu sehr abgeschirmt war, um unter milden Reaktionsbedingungen glycosyliert zu werden, bzw. die α-1-C-Mannosylnaphthaline unter drastischeren Reaktionsbedingungen nicht stabil waren. Daher wurde 1-(2′,3′,4′,6′-Tetra-O-benzyl-β-D-galactopyranosyl)-2-naphthol mit 2,3,4,6-Tetra-O-acetyl-α-D-mannopyranosyl-trichloracetimidat in Gegenwart von TMSOTf zum ersten synthetischen 1-C-2-O-Diglycosyl-phenol umgesetzt. Nach Abspaltung der Schutzgruppen sollte das erhaltene 1-Galactosyl-2-O-mannosyl-naphthalin enzymatisch zum Sialyl-LewisX-Mimetikum verlängert werden. Es wurde vom Enzym jedoch nicht als Substrat erkannt. Versuche zur chemischen Anbindung des Säurebausteins stehen noch aus.rn

Pre-edge analysis of X-rays absorption spectra in TiO2 modified films

The thesis is mainly focused on the pre-edge analysis of XAS spectra of Ti HCF sample hexacyanocobaltate and hexacyanoferrate samples doped on a Indium Tin Oxide (ITO) thin film. The work is aimed at the determination of Ti oxidation state, as well as indication of various coordination number in the studied samples. The experiment have been conducted using XAFS (X-ray absorption fine structure)beamline at Elettra synchrotron, Trieste (Italy) under supervision of Professor Marco Giorgetti, Department of Industrial Chemistry, University of Bologna. The Master thesis accreditation to fullfill the ASC Master of Advanced Spectroscopy in Chemistry Degree requirement.

High precision radial velocities with giano spectra

Radial velocities measured from near-infrared (NIR) spectra are a potential tool to search for extrasolar planets around cool stars. High resolution infrared spectrographs now available reach the high precision of visible instruments, with a constant improvement over time. GIANO is an infrared echelle spectrograph and it is a powerful tool to provide high resolution spectra for accurate radial velocity measurements of exo-planets and for chemical and dynamical studies of stellar or extragalactic objects. No other IR instruments have the GIANO's capability to cover the entire NIR wavelength range. In this work we develop an ensemble of IDL procedures to measure high precision radial velocities on a few GIANO spectra acquired during the commissioning run, using the telluric lines as wevelength reference. In Section 1.1 various exoplanet search methods are described. They exploit different properties of the planetary system. In Section 1.2 we describe the exoplanet population discovered trough the different methods. In Section 1.3 we explain motivations for NIR radial velocities and the challenges related the main issue that has limited the pursuit of high-precision NIR radial velocity, that is, the lack of a suitable calibration method. We briefly describe calibration methods in the visible and the solutions for IR calibration, for instance, the use of telluric lines. The latter has advantages and problems, described in detail. In this work we use telluric lines as wavelength reference. In Section 1.4 the Cross Correlation Function (CCF) method is described. This method is widely used to measure the radial velocities.In Section 1.5 we describe GIANO and its main science targets. In Chapter 2 observational data obtained with GIANO spectrograph are presented and the choice criteria are reported. In Chapter 3 we describe the detail of the analysis and examine in depth the flow chart reported in Section 3.1. In Chapter 4 we give the radial velocities measured with our IDL procedure for all available targets. We obtain an rms scatter in radial velocities of about 7 m/s. Finally, we conclude that GIANO can be used to measure radial velocities of late type stars with an accuracy close to or better than 10 m/s, using telluric lines as wevelength reference. In 2014 September GIANO is being operative at TNG for Science Verification and more observational data will allow to further refine this analysis.

Searching for outflows signatures in sdss spectra of x-ray selected, obscured agn in the cosmos field

Partendo dal campione di AGN presente nella survey di XMM-COSMOS, abbiamo cercato la sua controparte ottica nel database DR10 della Sloan Digital Sky Survey (SDSS), ed il match ha portato ad una selezione di 200 oggetti, tra cui stelle, galassie e quasar. A partire da questo campione, abbiamo selezionato tutti gli oggetti con un redshift z<0.86 per limitare l’analisi agli AGN di tipo 2, quindi siamo giunti alla selezione finale di un campione di 30 sorgenti. L’analisi spettrale è stata fatta tramite il task SPECFIT, presente in IRAF. Abbiamo creato due tipi di modelli: nel primo abbiamo considerato un’unica componente per ogni riga di emissione, nel secondo invece è stata introdotta un’ulteriore com- ponente limitando la FWHM della prima ad un valore inferiore a 500 km\s. Le righe di emissione di cui abbiamo creato un modello sono le seguenti: Hβ, [NII]λλ 6548,6581, Hα, [SII]λλ 6716,6731 e [OIII]λλ 4959,5007. Nei modelli costruiti abbiamo tenuto conto della fisica atomica per quel che riguarda i rapporti dei flussi teorici dei doppietti dell’azoto e dell’ossigeno, fissandoli a 1:3 per entrambi; nel caso del modello ad una componente abbiamo fissato le FWHM delle righe di emissione; mentre nel caso a due componenti abbiamo fissato le FWHM delle componenti strette e larghe, separatamente. Tenendo conto del chi-quadro ottenuto da ogni fit e dei residui, è stato possibile scegliere tra i due modelli per ogni sorgente. Considerato che la nostra attenzione è focalizzata sulla cinematica dell’ossigeno, abbiamo preso in considerazione solo le sorgenti i cui spettri mostravano la riga suddetta, cioè 25 oggetti. Su questa riga è stata fatta un’analisi non parametrica in modo da utilizzare il metodo proposto da Harrison et al. (2014) per caratterizzare il profilo di riga. Sono state determinate quantità utili come il 2 e il 98 percentili, corrispondenti alle velocità massime proiettate del flusso di materia, e l’ampiezza di riga contenente l’80% dell’emissione. Per indagare sull’eventuale ruolo che ha l’AGN nel guidare questi flussi di materia verso l’esterno, abbiamo calcolato la massa del gas ionizzato presente nel flusso e il tasso di energia cinetica, tenendo conto solo delle componenti larghe della riga di [OIII] λ5007. Per la caratterizzazione energetica abbiamo considerato l’approccio di Cano-Diaz et al (2012) e di Heckman (1990) in modo da poter ottenere un limite inferiore e superiore della potenza cinetica, adottando una media geometrica tra questi due come valore indicativo dell’energetica coinvolta. Confrontando la potenza del flusso di gas con la luminosità bolometrica dell’AGN, si è trovato che l’energia cinetica del flusso di gas è circa lo 0.3-30% della luminosità dell’AGN, consistente con i modelli che considerano l’AGN come principale responsabile nel guidare questi flussi di gas.

COSMIC-LAB: Unexpected Results from High-resolution Spectra of AGB Stars in Globular Clusters

We have used high-resolution spectra, acquired with UVES@ESO-VLT, to determine the chemical abundances of different samples of AGB and RGB stars in 4 Galactic globular clusters, namely 47Tuc, NGC3201, M22 and M62. For almost all the analyzed AGB stars we found a clear discrepancy between the iron abundance measured from neutral lines and that obtained from single ionized lines, while this discrepancy is not obtained for the RGB samples observed in the same clusters and analyzed with the same procedure. Such a behavior exactly corresponds to what expected in the case of Non-Local Thermodynamical Equilibrium (NLTE) in the star atmosphere. These results have a huge impact on the proper determination of GC chemistry. In fact, one of the most intriguing consequences is that, at odds with previous claims, no iron spread is found in NGC3201 and M22 if the iron abundance is obtained from ionized lines only.

Data analysis and simulations of VIRTIS venus spectra

VIRTIS, a bordo di Venus Express, è uno spettrometro in grado di operare da 0.25 a 5 µm. Nel periodo 2006-2011 ha ricavato un'enorme mole di dati ma a tutt'oggi le osservazioni al lembo sono poco utilizzate per lo studio delle nubi e delle hazes, specialmente di notte. Gli spettri al lembo a quote mesosferiche sono dominati dalla radianza proveniente dalle nubi e scatterata in direzione dello strumento dalle hazes. L'interpretazione degli spettri al lembo non può quindi prescindere dalla caratterizzazione dell'intera colonna atmosferica. L'obiettivo della tesi è di effettuare un’analisi statistica sulle osservazioni al nadir e proporre una metodologia per ricavare una caratterizzazione delle hazes combinando osservazioni al nadir e al lembo. La caratterizzazione delle nubi è avvenuta su un campione di oltre 3700 osservazioni al nadir. È stato creato un ampio dataset di spettri sintetici modificando, in un modello iniziale, vari parametri di nube quali composizione chimica, numero e dimensione delle particelle. Un processo di fit è stato applicato alle osservazioni per stabilire quale modello potesse descrivere gli spettri osservati. Si è poi effettuata una analisi statistica sui risultati del campione. Si è ricavata una concentrazione di acido solforico molto elevata nelle nubi basse, pari al 96% in massa, che si discosta dal valore generalmente utilizzato del 75%. Si sono poi integrati i risultati al nadir con uno studio mirato su poche osservazioni al lembo, selezionate in modo da intercettare nel punto di tangenza la colonna atmosferica osservata al nadir, per ricavare informazioni sulle hazes. I risultati di un modello Monte Carlo indicano che il numero e le dimensioni delle particelle previste dal modello base devono essere ridotte in maniera significativa. In particolare si osserva un abbassamento della quota massima delle hazes rispetto ad osservazioni diurne.

Two-dimensional linear-combination model fitting of magnetic resonance spectra to define the macromolecule baseline using FiTAID, a Fitting Tool for Arrays of Interrelated Datasets

To propose the determination of the macromolecular baseline (MMBL) in clinical 1H MR spectra based on T(1) and T(2) differentiation using 2D fitting in FiTAID, a general Fitting Tool for Arrays of Interrelated Datasets.

Magnetization exchange with water and T(1) relaxation of the downfield resonances in human brain spectra at 3.0 T

The use of water suppression for in vivo proton MR spectroscopy diminishes the signal intensities from resonances that undergo magnetization exchange with water, particularly those downfield of water. To investigate these exchangeable resonances, an inversion transfer experiment was performed using the metabolite cycling technique for non-water-suppressed MR spectroscopy from a large brain voxel in 11 healthy volunteers at 3.0 T. The exchange rates of the most prominent peaks downfield of water were found to range from 0.5 to 8.9 s(-1), while the T(1) relaxation times in absence of exchange were found to range from 175 to 525 ms. These findings may help toward the assignments of the downfield resonances and a better understanding of the sources of contrast in chemical exchange saturation transfer imaging.