The Gemini planet-finding campaign: the frequency of giant planets aroud debris disk stars

We have completed a high-contrast direct imaging survey for giant planets around 57 debris disk stars as part of the Gemini NICI Planet-Finding Campaign. We achieved median H-band contrasts of 12.4 mag at 0.''5 and 14.1 mag at 1'' separation. Follow-up observations of the 66 candidates with projected separation <500 AU show that all of them are background objects. To establish statistical constraints on the underlying giant planet population based on our imaging data, we have developed a new Bayesian formalism that incorporates (1) non-detections, (2) single-epoch candidates, (3) astrometric and (4) photometric information, and (5) the possibility of multiple planets per star to constrain the planet population. Our formalism allows us to include in our analysis the previously known β Pictoris and the HR 8799 planets. Our results show at 95% confidence that <13% of debris disk stars have a ≥5 M Jup planet beyond 80 AU, and <21% of debris disk stars have a ≥3 M Jup planet outside of 40 AU, based on hot-start evolutionary models. We model the population of directly imaged planets as d 2 N/dMdavpropm α a β, where m is planet mass and a is orbital semi-major axis (with a maximum value of a max). We find that β < –0.8 and/or α > 1.7. Likewise, we find that β < –0.8 and/or a max < 200 AU. For the case where the planet frequency rises sharply with mass (α > 1.7), this occurs because all the planets detected to date have masses above 5 M Jup, but planets of lower mass could easily have been detected by our search. If we ignore the β Pic and HR 8799 planets (should they belong to a rare and distinct group), we find that <20% of debris disk stars have a ≥3 M Jup planet beyond 10 AU, and β < –0.8 and/or α < –1.5. Likewise, β < –0.8 and/or a max < 125 AU. Our Bayesian constraints are not strong enough to reveal any dependence of the planet frequency on stellar host mass. Studies of transition disks have suggested that about 20% of stars are undergoing planet formation; our non-detections at large separations show that planets with orbital separation >40 AU and planet masses >3 M Jup do not carve the central holes in these disks.

The Gemini NICI planet-finding campaign: the frequency of giant planets around young B and A stars

We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5-2.5 M ☉) conducted to date and includes the planet hosts β Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58$^{+21}_{-20}$ M Jup and 55$^{+20}_{-19}$ M Jup, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M ☉ stars can have giant planets greater than 4 M Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M Jup between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M Jup, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.

Mass extinctions, galactic orbits in the solar neighborhood and the Sun: a connection?

The orbits of the stars in the disk of the Galaxy, and their passages through the Galactic spiral arms, are a rarely mentioned factor of biosphere stability which might be important for long-term planetary climate evolution, with a possible bearing on mass extinctions. The Sun lies very near the co-rotation radius, where stars revolve around the Galaxy in the same period as the density wave perturbations of the spiral arms. conventional wisdom generally considers that this status makes for few passages through the spiral arms. Controversy still surrounds whether time spent inside or around spiral arms is dangerous to biospheres and conductive to mass extinctions. Possible threats include giant molecular clouds disturbing the Oort comet cloud and provoking heavy bombardment: a higher exposure to cosmic rays near star forming regions triggering increased cloudiness in Earth atmosphere and ice ages; and the desctruction of Earth's ozone layer posed by supernova explosiosn. We present detailed calculations of the history of spiral arm passages for all 212 solar-type stars nearer than 20 parsecs, including the total time spent inside armsin the last 500 Myr, when the spiral arm position can be traced with good accuracy. We found that there is a large diversity of stellar orbits in the solar neighborhood, and the time fraction spent inside spiral arms can vary from a few percent to nearly half the time. The Sun, despite its proximity to the galactic co-rotation radius, has exceptionally low eccentricity and a low vertical velocity component, and therefore spends 30% of its lifetime crossing the spiral arms, more than most nearby stars. We discuss the possible implications of this fact to the long-term habitability of the Earth, and possible correlations of the Sun's passage through the spiral arms with the five great mass extinctions of the Earth's biosphere from the Late Ordovician to the Cretaceous-Tertiary.

Sulla energia dissipata in alcuni organi di macchina

Questa tesi riguarda l'analisi delle trasmissioni ad ingranaggi e delle ruote dentate in generale, nell'ottica della minimizzazione delle perdite di energia. È stato messo a punto un modello per il calcolo della energia e del calore dissipati in un riduttore, sia ad assi paralleli sia epicicloidale. Tale modello consente di stimare la temperatura di equilibrio dell'olio al variare delle condizioni di funzionamento. Il calcolo termico è ancora poco diffuso nel progetto di riduttori, ma si è visto essere importante soprattutto per riduttori compatti, come i riduttori epicicloidali, per i quali la massima potenza trasmissibile è solitamente determinata proprio da considerazioni termiche. Il modello è stato implementato in un sistema di calcolo automatizzato, che può essere adattato a varie tipologie di riduttore. Tale sistema di calcolo consente, inoltre, di stimare l'energia dissipata in varie condizioni di lubrificazione ed è stato utilizzato per valutare le differenze tra lubrificazione tradizionale in bagno d'olio e lubrificazione a “carter secco” o a “carter umido”. Il modello è stato applicato al caso particolare di un riduttore ad ingranaggi a due stadi: il primo ad assi paralleli ed il secondo epicicloidale. Nell'ambito di un contratto di ricerca tra il DIEM e la Brevini S.p.A. di Reggio Emilia, sono state condotte prove sperimentali su un prototipo di tale riduttore, prove che hanno consentito di tarare il modello proposto [1]. Un ulteriore campo di indagine è stato lo studio dell’energia dissipata per ingranamento tra due ruote dentate utilizzando modelli che prevedano il calcolo di un coefficiente d'attrito variabile lungo il segmento di contatto. I modelli più comuni, al contrario, si basano su un coefficiente di attrito medio, mentre si può constatare che esso varia sensibilmente durante l’ingranamento. In particolare, non trovando in letteratura come varia il rendimento nel caso di ruote corrette, ci si è concentrati sul valore dell'energia dissipata negli ingranaggi al variare dello spostamento del profilo. Questo studio è riportato in [2]. È stata condotta una ricerca sul funzionamento di attuatori lineari vite-madrevite. Si sono studiati i meccanismi che determinano le condizioni di usura dell'accoppiamento vite-madrevite in attuatori lineari, con particolare riferimento agli aspetti termici del fenomeno. Si è visto, infatti, che la temperatura di contatto tra vite e chiocciola è il parametro più critico nel funzionamento di questi attuatori. Mediante una prova sperimentale, è stata trovata una legge che, data pressione, velocità e fattore di servizio, stima la temperatura di esercizio. Di tale legge sperimentale è stata data un'interpretazione sulla base dei modelli teorici noti. Questo studio è stato condotto nell'ambito di un contratto di ricerca tra il DIEM e la Ognibene Meccanica S.r.l. di Bologna ed è pubblicato in [3].

Eduardo Zamacois: attività editoriale e opera letteraria

Eduardo Zamacois (Pinar del Río, 1873- Buenos Aires, 1971) was a main actor of the spanish’s literature and edition movement from the first third of the 20th century. He was the founder of magazines that had a big impact like “Germinal”, introductive of the sicalipsis (“La Vida Galante”) or so innovative that deserved an special chapter in the history of literature (“El Cuento Semanal” e “Los Contemporáneos”). With this work, it is intended to recreate the most significant stages from his autobiography adventure including the new information that offers his non before published letters exchange with his last sentimental partner. As a writer, his work was very popular in his homeland, translated to the world and reissued in Ibero-America. His literature work is based in three different phases. He began with the use of gallant literature (with books like La enferma, Punto negro) and took an adventure with the pays of mystery and irony (El otro, El misterio de un hombre pequñito, La opinion ajena) to finally focused in a narrative style of a realistic kind, that includes social critique (Las raíces). His last published novel in Spain is a portrait of Madrid during its long siege by the nationalist troops (El asedio de Madrid), a profound tribute to the people’s heroism and a declaration of love to the capital, that was his place of residence for a long time. While his exile, that took him to Cuba, New York and Buenos Aires, he worked in the radio, the dubbing industry and in finishing his most detailed bibliography, Un hombre que se va, a valuable document of that time.

Ovidio e Marziale tra poesia e retorica

This 
study
 participates 
of
 the 
vivacious
 and
 recent 
interest
 for
 the 
Martial’s
 work, 
that
 has
 brought
 to
 discover
 a
 wealth
 and 
a 
complexity,
 remained 
for 
a
long
 time
 hidden, 
of 
the 
epigrammatic
 kind.
 Of
 this
 complexity
 is
 an
 important
 part
 the
 refined
 allusive
 game
 with
 the
 preceding
 tradition,
 as
 that
 with 
Ovid.
 My 
work
 is
 divided
 in
 two
 sections: 
the 
first
 one
 is dedicated
 to 
the 
passages 
in 
which
 Martial
 quotes
 Ovid
 and
 to
 the
 surest
 and
 more
 important
 recalls.
 The
 single
 chapters
 are
 dedicated
 to
 a
 detail
 theme
 (the
 apostrophe
 to
 the
 book;
 the
 mythology;
 the
 love;
 the
 exile).
 The
 second
 section, 
instead, 
is
 dedicated 
to 
the 
rhetoric,
 with
 an 
analysis 
of
 the
 structure 
of 
the 
poetic
 discourse
 in
 the
 elegy
 and
 in
 the
 epigram,
 and
 to
 the study
 of
 some
 rhetorical
 figures,
 in
 primis
 the
 sententia,
 key‐element
 in
 the
 Martial’s
 work,
 but
 also
 decisive
 in
 the
 innovative
 poetic process
 begun by
 Ovid.


Libro, diaspora e ri-costruzioni identitarie. Per una storia della tipografia sefardita portoghese nell'Italia del Cinquecento

Il lavoro ripercorre le tracce che gli ebrei portoghesi, esuli dopo il biennio 1496-97, lasciarono nel loro cammino attraverso l'Europa. In particolare, l'interesse si concentra sulla breve parentesi italiana, che grazie all'apertura e alla disponibilità  di alcuni Signori, come i Gonzaga di Mantova, i Medici, i Dogi della Serenissima e gli Este, risulta ricchissima di avvenimenti e personaggi, decisivi anche per la storia culturale del Portogallo. L'analisi parte evidenziando l'importanza che ebbe la tipografia ebraica in Portogallo all'epoca della sua introduzione nel Paese; in secondo luogo ripercorre la strada che, dal biennio del primo decreto di espulsione e del conseguente battesimo di massa, porta alla nascita dell'€™Inquisizione in Portogallo. Il secondo capitolo tenta di fare una ricostruzione, il più possibile completa e coerente, dei movimenti degli esuli, bollati come marrani e legati alle due maggiori famiglie, i Mendes e i Bemveniste, delineando poi il primo nucleo di quella che diventerà  nel Seicento la comunità  sefardita portoghese di Amsterdam, dove nasceranno le personalità  dissidenti di Uriel da Costa e del suo allievo Spinoza. Il terzo capitolo introduce il tema delle opere letterarie, effettuando una rassegna dei maggiori volumi editi dalle officine tipografiche ebraiche stanziatesi in Italia fra il 1551 e il 1558, in modo particolare concentrando l'attenzione sull'€™attività  della tipografia Usque, da cui usciranno numerosi testi di precettistica in lingua ebraica, ma soprattutto opere cruciali come la famosa «Bibbia Ferrarese» in castigliano, la «Consolação às Tribulações de Israel», di Samuel Usque e la raccolta composta dal romanzo cavalleresco «Menina e Moça» di Bernardim Ribeiro e dall'ecloga «Crisfal», di un autore ancora non accertato. L'ultimo capitolo, infine, si propone di operare una disamina di queste ultime tre opere, ritenute fondamentali per ricostruire il contesto letterario e culturale in cui la comunità  giudaica in esilio agiva e proiettava le proprie speranze di futuro. Per quanto le opere appartengano a generi diversi e mostrino diverso carattere, l'€™ipotesi è che siano parte di un unicum filosofico e spirituale, che intendeva sostanzialmente indicare ai confratelli sparsi per l'Europa la direzione da prendere, fornendo un sostegno teoretico, psicologico ed emotivo nelle difficili condizioni di sopravvivenza, soprattutto dell'integrità religiosa, di ciascun membro della comunità.

Troposphere Calibration Techniques for Deep Space Probe Tracking

Ground-based Earth troposphere calibration systems play an important role in planetary exploration, especially to carry out radio science experiments aimed at the estimation of planetary gravity fields. In these experiments, the main observable is the spacecraft (S/C) range rate, measured from the Doppler shift of an electromagnetic wave transmitted from ground, received by the spacecraft and coherently retransmitted back to ground. If the solar corona and interplanetary plasma noise is already removed from Doppler data, the Earth troposphere remains one of the main error sources in tracking observables. Current Earth media calibration systems at NASA’s Deep Space Network (DSN) stations are based upon a combination of weather data and multidirectional, dual frequency GPS measurements acquired at each station complex. In order to support Cassini’s cruise radio science experiments, a new generation of media calibration systems were developed, driven by the need to achieve the goal of an end-to-end Allan deviation of the radio link in the order of 3×〖10〗^(-15) at 1000 s integration time. The future ESA’s Bepi Colombo mission to Mercury carries scientific instrumentation for radio science experiments (a Ka-band transponder and a three-axis accelerometer) which, in combination with the S/C telecommunication system (a X/X/Ka transponder) will provide the most advanced tracking system ever flown on an interplanetary probe. Current error budget for MORE (Mercury Orbiter Radioscience Experiment) allows the residual uncalibrated troposphere to contribute with a value of 8×〖10〗^(-15) to the two-way Allan deviation at 1000 s integration time. The current standard ESA/ESTRACK calibration system is based on a combination of surface meteorological measurements and mathematical algorithms, capable to reconstruct the Earth troposphere path delay, leaving an uncalibrated component of about 1-2% of the total delay. In order to satisfy the stringent MORE requirements, the short time-scale variations of the Earth troposphere water vapor content must be calibrated at ESA deep space antennas (DSA) with more precise and stable instruments (microwave radiometers). In parallel to this high performance instruments, ESA ground stations should be upgraded to media calibration systems at least capable to calibrate both troposphere path delay components (dry and wet) at sub-centimetre level, in order to reduce S/C navigation uncertainties. The natural choice is to provide a continuous troposphere calibration by processing GNSS data acquired at each complex by dual frequency receivers already installed for station location purposes. The work presented here outlines the troposphere calibration technique to support both Deep Space probe navigation and radio science experiments. After an introduction to deep space tracking techniques, observables and error sources, in Chapter 2 the troposphere path delay is widely investigated, reporting the estimation techniques and the state of the art of the ESA and NASA troposphere calibrations. Chapter 3 deals with an analysis of the status and the performances of the NASA Advanced Media Calibration (AMC) system referred to the Cassini data analysis. Chapter 4 describes the current release of a developed GNSS software (S/W) to estimate the troposphere calibration to be used for ESA S/C navigation purposes. During the development phase of the S/W a test campaign has been undertaken in order to evaluate the S/W performances. A description of the campaign and the main results are reported in Chapter 5. Chapter 6 presents a preliminary analysis of microwave radiometers to be used to support radio science experiments. The analysis has been carried out considering radiometric measurements of the ESA/ESTEC instruments installed in Cabauw (NL) and compared with the requirements of MORE. Finally, Chapter 7 summarizes the results obtained and defines some key technical aspects to be evaluated and taken into account for the development phase of future instrumentation.

Analisi della dinamica e composizione chimica del particolato atmosferico mediante un modello alla mesoscala

The vertical profile of aerosol in the planetary boundary layer of the Milan urban area is studied in terms of its development and chemical composition in a high-resolution modelling framework. The period of study spans a week in summer of 2007 (12-18 July), when continuous LIDAR measurements and a limited set of balloon profiles were collected in the frame of the ASI/QUITSAT project. LIDAR observations show a diurnal development of an aerosol plume that lifts early morning surface emissions to the top of the boundary layer, reaching maximum concentration around midday. Mountain breeze from Alps clean the bottom of the aerosol layer, typically leaving a residual layer at around 1500-2000 m which may survive for several days. During the last two days under analysis, a dust layer transported from Sahara reaches the upper layers of Milan area and affects the aerosol vertical distribution in the boundary layer. Simulation from the MM5/CHIMERE modelling system, carried out at 1 km horizontal resolution, qualitatively reproduced the general features of the Milan aerosol layer observed with LIDAR, including the rise and fall of the aersol plume, the residual layer in altitude and the Saharan dust event. The simulation highlighted the importance of nitrates and secondary organics in its composition. Several sensitivity tests showed that main driving factors leading to the dominance of nitrates in the plume are temperature and gas absorption process. A modelling study turn to the analysis of the vertical aerosol profiles distribution and knowledge of the characterization of the PM at a site near the city of Milan is performed using a model system composed by a meteorological model MM5 (V3-6), the mesoscale model from PSU/NCAR and a Chemical Transport Model (CTM) CHIMERE to simulate the vertical aerosol profile. LiDAR continuous observations and balloon profiles collected during two intensive campaigns in summer 2007 and in winter 2008 in the frame of the ASI/QUITSAT project have been used to perform comparisons in order to evaluate the ability of the aerosol chemistry transport model CHIMERE to simulate the aerosols dynamics and compositions in this area. The comparisons of model aerosols with measurements are carried out over a full time period between 12 July 2007 and 18 July 2007. The comparisons demonstrate the ability of the model to reproduce correctly the aerosol vertical distributions and their temporal variability. As detected by the LiDAR, the model during the period considered, predicts a diurnal development of a plume during the morning and a clearing during the afternoon, typically the plume reaches the top of the boundary layer around mid day, in this time CHIMERE produces highest concentrations in the upper levels as detected by LiDAR. The model, moreover can reproduce LiDAR observes enhancement aerosols concentrations above the boundary layer, attributing the phenomena to dust out intrusion. Another important information from the model analysis regard the composition , it predicts that a large part of the plume is composed by nitrate, in particular during 13 and 16 July 2007 , pointing to the model tendency to overestimates the nitrous component in the particular matter vertical structure . Sensitivity study carried out in this work show that there are a combination of different factor which determine the major nitrous composition of the “plume” observed and in particular humidity temperature and the absorption phenomena are the mainly candidate to explain the principal difference in composition simulated in the period object of this study , in particular , the CHIMERE model seems to be mostly sensitive to the absorption process.

Untersuchungen zur troposphärischen Photochemie am GAW-Observatorium Izana

Im Rahmen dieser Promotionsarbeit wurden Fragestellungen der troposphärischen Ozonproduktion, des photostationären Gleichgewicht des NO2-NO-O3-ROx-Systems, des Einflusses von heterogenen Reaktionen an Mineralstauboberflächen und der Bedeutung lokaler anthropogener Emissionen für Spurengasmessungen an einem Gebirgsobservatorium untersucht. Dazu wurde insbesondere ein atmosphärenchemisch-meteorologischer Datensatz ausgewertet, welcher während der Feldmesskampagne MINATROC II im Juli/August 2002 am Global Atmosphere Watch (GAW) Observatorium Izana (2360m über NN) auf Teneriffa gewonnen wurde. Der Datensatz enthält Messdaten von Aerosolen, Spurengasen, Strahlungsgrößen und meteorologischen Parametern. Eine dichte Sahara-Staubwolke passierte die Messstation zwischen dem 28. und 31.07.2002. Die Mischungsverhältnisse von O3, H2O2, NOx und ROx zeigten während dieses Ereignisses Abnahmen zwischen 10% und 50%. Insbesondere infolge der Reduktion von NO und HO2 wurde eine deutliche Verringerung der Netto-Ozon-Produktion in der Staubwolke berechnet. Die Bewertung der verschiedenen Terme der Ozonproduktion bzw. –vernichtung zeigte relativ geringe Beiträge der einzelnen photochemischen Verlustreaktionen am Ozonbudget. Im Rahmen einer Boxmodellstudie, welche die Eingangsdaten von MINATROC II verwendete, wurde ein Vergleich zwischen Simulation und Messung kurzlebiger Spurengase angestellt. Die Modellrechnungen weisen darauf hin, dass die reduzierten H2O2-Mischungsverhältnisse in der Sahara-Staubwolke unter Berücksichtigung heterogener Reaktionen von HO2 bzw. H2O2 an Stauboberflächen erklärt werden können. Die Betrachtungen zum photostationären Gleichgewicht des NO2-NO-O3-ROx-Systems ergeben hauptsächlich stark überhöhte Leighton-Verhältnisse. Die Abweichungen der Messdaten vom photostationären Gleichgewichtszustand sind dabei zum Verschmutzungsgrad der Atmosphäre antikorreliert. Eine Reihe potentieller Einflüsse auf das NO2-NO-O3-ROx-System wurde diskutiert, wobei gezeigt werden konnte, dass das bisherige Betrachtungsmodell nicht ausreicht, um die beobachteten Abweichungen vom photostationären Gleichgewicht zu erklären. Während für die Nachtmessungen von MINATROC II Bedingungen der freien Troposphäre vorlagen, waren die Messungen am Tage von der Kopplung zwischen photochemischer Aktivität und thermisch getriebener Hangströmung betroffen. Die zum Messort gelangte anthropogen beeinflusste Grenzschichtluft konnte dabei auf maximalen Mischungsanteilen zwischen 15% und 85% quantifiziert werden. Abschließend wurden verschiedene Aspekte der Quellen und der Verteilung anthropogener Verschmutzungen auf Teneriffa im Zusammenhang der zuvor behandelten Fragen diskutiert.

Interactions between the hydrological cycle and atmospheric chemistry

The land-atmosphere exchange of atmospheric trace gases is sensitive to meteorological conditions and climate change. It contributes in turn to the atmospheric radiative forcing through its effects on tropospheric chemistry. The interactions between the hydrological cycle and atmospheric processes are intricate and often involve different levels of feedbacks. The Earth system model EMAC is used in this thesis to assess the direct role of the land surface components of the terrestrial hydrological cycle in the emissions, deposition and transport of key trace gases that control tropospheric chemistry. It is also used to examine its indirect role in changing the tropospheric chemical composition through the feedbacks between the atmospheric and the terrestrial branches of the hydrological cycle. Selected features of the hydrological cycle in EMAC are evaluated using observations from different data sources. The interactions between precipitation and the water vapor column, from the atmospheric branch of the hydrological cycle, and evapotranspiration, from its terrestrial branch, are assessed specially for tropical regions. The impacts of changes in the land surface hydrology on surface exchanges and the oxidizing chemistry of the atmosphere are assessed through two sensitivity simulations. In the first, a new parametrization for rainfall interception in the densely vegetated areas in the tropics is implemented, and its effects are assessed. The second study involves the application of a soil moisture forcing that replaces the model calculated soil moisture. Both experiments have a large impact on the local hydrological cycle, dry deposition of soluble and insoluble gases, emissions of isoprene through changes in surface temperature and the Planetary Boundary Layer height. Additionally the soil moisture forcing causes changes in local vertical transport and large-scale circulation. The changes in trace gas exchanges affect the oxidation capacity of the atmosphere through changes in OH, O$_3$, NO$_x$ concentrations.

Aufbau und Charakterisierung eines flugzeuggetragenen Einzelpartikel-Massenspektrometers

Im Rahmen dieser Arbeit wurde ein flugzeuggetragenes Laserablations-Einzelpartikel-Massenspektrometer von Grund auf entworfen, gebaut, charakterisiert und auf verschiedenen Feldmesskampagnen eingesetzt. Das ALABAMA (Aircraft-based Laser ABlation Aerosol MAss Spectrometer) ist in der Lage die chemische Zusammensetzung und Größe von einzelnen Aerosolpartikeln im submikrometer-Bereich (135 – 900 nm) zu untersuchen.rnNach dem Fokussieren in einer aerodynamischen Linse wird dafür zunächst derrnaerodynamische Durchmesser der einzelnen Partikel mit Hilfe einer Flugzeitmessung zwischen zwei Dauerstrichlasern bestimmt. Anschließend werden die zuvor detektierten und klassifizierten Partikel durch einen gezielten Laserpuls einzeln verdampft und ionisiert. Die Ionen werden in einem bipolaren Flugzeit-Massenspektrometer entsprechend ihrem Masse zu- Ladungs Verhältnisses getrennt und detektiert. Die entstehenden Massenspektren bieten einen detaillierten Einblick in die chemische Struktur der einzelnen Partikel.rnDas gesamte Instrument wurde so konzipiert, dass es auf dem neuen Höhenforschungsflugzeug HALO und anderen mobilen Plattformen eingesetzt werden kann. Um dies zu ermöglichen wurden alle Komponenten in einem Rahmen mit weniger als 0.45 m³ Volumen untergebracht. Das gesamte Instrument inklusive Rahmen wiegt weniger als 150 kg und erfüllt die strengen sicherheitsvorschriften für den Betrieb an Bord von Forschungsflugzeugen. Damit ist ALABAMA das kleinste und leichteste Instrument seiner Art.rnNach dem Aufbau wurden die Eigenschaften und Grenzen aller Komponenten detailliert im Labor und auf Messkampagnen charakterisiert. Dafür wurden zunächst die Eigenschaften des Partikelstrahls, wie beispielsweise Strahlbreite und –divergenz, ausführlich untersucht. Die Ergebnisse waren wichtig, um die späteren Messungen der Detektions- und Ablationseffizienz zu validieren.rnBei den anschließenden Effizienzmessungen wurde gezeigt, dass abhängig von ihrer Größe und Beschaffenheit, bis zu 86 % der vorhandenen Aerosolpartikel erfolgreich detektiert und größenklassifiziert werden. Bis zu 99.5 % der detektierten Partikel konnten ionisiert und somit chemisch untersucht werden. Diese sehr hohen Effizienzen sind insbesondere für Messungen in großer Höhe entscheidend, da dort zum Teil nur sehr geringe Partikelkonzentrationen vorliegen.rnDas bipolare Massenspektrometer erzielt durchschnittliche Massenauflösungen von bis zu R=331. Während Labor- und Feldmessungen konnten dadurch Elemente wie Au, Rb, Co, Ni, Si, Ti und Pb eindeutig anhand ihres Isotopenmusters zugeordnet werden.rnErste Messungen an Bord eines ATR-42 Forschungsflugzeuges während der MEGAPOLI Kampagne in Paris ergaben einen umfassenden Datensatz von Aerosolpartikeln innerhalb der planetaren Grenzschicht. Das ALABAMA konnte unter harten physischen Bedingungen (Temperaturen > 40°C, Beschleunigungen +/- 2 g) verlässlich und präzise betrieben werden. Anhand von charakteristischen Signalen in den Massenspektren konnten die Partikel zuverlässig in 8 chemische Klassen unterteilt werden. Einzelne Klassen konnten dabei bestimmten Quellen zugeordnet werden. So ließen sich beispielsweise Partikel mit starkerrnNatrium- und Kaliumsignatur eindeutig auf die Verbrennung von Biomasse zurückführen.rnALABAMA ist damit ein wertvolles Instrument um Partikel in-situ zu charakterisieren und somit verschiedenste wissenschaftliche Fragestellungen, insbesondere im Bereich der Atmosphärenforschung, zu untersuchen.

Diagnose der Residuumszirkulation und ihre Bedeutung für die Klimavariabilität der Stratosphäre

Mit einem in dieser Arbeit entwickelten Diagnose-Werkzeug wird im Rahmenrneines einfachen mechanistischenModells die Residuumszirkulation in der Stratosphärernermittelt. Die Residuumszirkulation wird als eine Schlüsselgröße für diernKlimavariabilität der Stratosphäre angesehen. Für die Diagnose wird mit einemrnmechanistischem Modell die Ausbreitung und das Brechen planetarer Wellenrnbeschrieben und der daraus resultierende Wellenantrieb bestimmt. Dieser Wellenantriebrnwird verwendet, um mit der numerischen Lösung einer elliptischenrnDifferentialgleichung die Residuumszirkulation zu berechnen.rnDieses Diagnose-Werkzeug wird genutzt, um in atmosphärischen Reanalysedatenrnden Zusammenhang der Residuumszirkulation mit verschiedenen Modenrnstratosphärischer Klimavariabilität zu untersuchen. Während für unterschiedlichernPhasen der quasi-zweijährigen Schwingung und der Nordatlantischen Oszillationrndie Residuumszirkulation deutliche Unterschiede aufzeigt, kann ein Einflussrndes 11-jährigen Sonnenfleckenzyklus auf die Residuumszirkulation nichtrneindeutig nachgewiesen werden. Eine Datenstudie zeigt, dass in den WintermonatenrnDezember und Januar die Stärke der Residuumszirkulation mit derrnTemperatur der unteren polaren Stratosphäre signifikant korreliert ist.

I Gesuiti americani espulsi in Italia e Joaquín Camaño (1767-1814)

Joaquín Camaño fu un gesuita della Provincia del Paraguay, vissuto nell' esilio italiano la maggior parte della sua vita dal 1767 al 1820. Il suo lavoro e la sua fama possono essere considerati di minore importanza se paragonati a molti altri gesuiti esiliati per ordine di Carlo III alla fine del XVIII secolo in Emilia-Romagna. Attraverso la mia ricerca approfondisco il ruolo di J. Camaño quale personaggio minore che entra nella vita degli altri espulsi tramite un dinamico network relazionale di cui è stato uno dei principali artefici. Il mio obiettivo è stato quello di studiare l'impatto che ebbero gli esuli gesuiti americani, attraverso la vita di Joaquin Camaño, sul mondo intellettuale italiano, europeo ed americano dopo l'espulsione del 1767. Egli, con i suoi studi, si inserisce nella rinnovata e vivace retorica del “Mondo Nuovo” che in quegli anni assume un grande dinamismo. Nato nella modesta città di La Rioja, in Argentina, si erge come un brillante cartografo, etnografo e linguista nel contesto dell'Illustrazione europea grazie alla sua particolare vita da missionario. Dopo l'espulsione, Joaquin Camaño, insieme ad altri numerosi confratelli americani, arriverà a Faenza, nello Stato Pontificio, dedicandosi allo studio della cartografia, dell'etnografia e delle lingue americane. Le sue ricerche si collocano in un momento nevralgico per la storia del pensiero linguistico-antropologico, quando l'osservazione diretta e la riflessione teorica dei fenomeni si misuravano con la grande varietà umana ormai riscontrata nel mondo.

Egemonia, socialismo e democrazia nell’occidente periferico. Gli studi gramsciani di Aricó e Portantiero tra Argentina e Messico.

La ricerca si propone di mostrare come il pensiero gramsciano sia stato riferimento prioritario di due intellettuali argentini in esilio in Messico dal 1976 al 1983: Juan Carlos Portantiero e José Maria Aricó. In quel periodo incentrarono le loro elaborazioni teorico-politiche sull’analisi della relazione tra Stato, società civile, democrazia e socialismo, partendo da una prospettiva gramsciana. Il fallimento della guerra di movimento in Argentina nei primi anni settanta li condusse a riflettere su strategie alternative di transizione al socialismo, il cui punto focale fu il concetto di "Egemonia". A partire dal 1975 indirizzarono la ripresa del pensiero di Gramsci alla creazione di un progetto politico adatto ad un contesto sempre più "occidentale", caratterizzato dalla presenza di una "società civile complessa", in cui risultava necessario combattere "guerre di posizione" e non "guerre di movimento". La prospettiva che connotò questo approccio alle riflessioni gramsciane rappresenta il culmine di un percorso che iniziarono negli anni ’50, quando sorsero i primi studi del pensiero gramsciano in Argentina. Sin da allora, Aricó e Portantiero si occuparono di Gramsci insieme al dirigente del PC argentino Agosti e continuarono a farlo anche durante gli anni sessanta e i primi anni settanta sulla rivista Pasado y Presente. Fu, però, nel periodo dell’esilio che ne ripresero il pensiero considerandolo nella sua totalità, a partire dagli scritti giovanili sino ai Quaderni del Carcere, rielaborandolo in maniera originale e costruendo una propria proposta di cammino verso socialismo nell' "occidente periferico" dell'Argentina, influenzati dall'azione del Partito Comunista Italiano.