A space camera is a promising candidate to address the non-stop rising interest for astrophysics research in the Compton regime. The MeVCube mission is intended to be launched in 2022, hosting an on-board Compton Camera. To better support the development of the instrument in this early stage, a series of feasibility studies to assess two potential launch orbits were performed. The studies were composed by a series of mission analysis simulations which permitted the characterisation of the orbital environments for the two orbital options. Several sources of background noise to the instrument were identified. The population of trapped protons and trapped electrons were simulated for the periods of Solar Minimum and Solar Maximum, as well as the levels of Galactic Cosmic Ray (GCR) flux. The performance of trade-off studies concluded that an equatorial orbit is more preferable for reducing the influence of background noise. To better estimate the environment effects at the equatorial orbit, the number of particles which can penetrate the detector shielding were simulated. The next step was to perform a series secondary studies whose aim were to simulate the induced current on the electrodes, produced by the interactions occurring within the detector. The actualisation of these simulations required the study of photon interaction with matter, the various Cadmium-Zink-Telluride (CZT) types and the how they operate, and the use of a sophisticated software to perform the appropriate simulations. COMSOL, which allows the method of FEA, was chosen as the tool to perform the simulations. The geometry of the detector voxel was primarily designed in SIEMENS NX. The geometry was inserted into COMSOL, where a number of iterations were performed to finalise the appropriate mesh size, which ensured an accurate representation of the Electric field and the Weighting potential within the detector voxel. The induced current on the electrodes was decided to be calculated via MATLAB. As a verification step it was thought useful to firstly plot the weighting potential of the three electrodes under test; the chosen anode pixel, the steering grid and the cathode. The process revealed a series of numerical errors, most likely introduced by the type of mesh chosen or by the data manipulation process via MATLAB. Significant reduction of the numerical errors would lead to more accurate values for the induced current. Unfortunately, due to time constraints this was a task that was not completed. Solving this problem would be optimal for future studies with MATLAB, as the induced current on the electrodes can be correctly calculated based on charge transport within the detector bulk. / MeVCube, DESY

Le sujet de thèse s'inscrit dans le cadre d'un nouveau projet de détermination de la constante de von Klitzing débuté depuis quelques années au LNE et dont l'aboutissement est prévu pour 2018. A ce jour, la mesure la plus exacte de cette constante traçable au Système International d’unités (SI) est obtenue via le raccordement de l'ohm produit par l'effet Hall quantique au farad, matérialisé à l'aide d'un condensateur calculable dit de Thompson-Lampard. Afin d'améliorer sa précédente détermination délivrée en 2000 avec une incertitude relative de 5.10-8,le LNE a décidé de construire un nouvel étalon calculable de Thompson-Lampard (déjà en cours de développement) et d'améliorer l'exactitude de l'ensemble des dispositifs de mesure associés avec pour objectif de réduire l’incertitude globale sur cette détermination à une valeur proche de 10-8. Le travail de thèse porte sur la réalisation, la caractérisation et/ou l’automatisation de la chaîne de mesure associée à cette détermination. / The comparison of electrical quantities expressed in units of the International System of Units (SI) and the same quantities generated from quantum effects is a direct way of determining physical constants. The determination of the von Klitzing constant (quantum of resistance) from a calculable capacitor is a part of this process. The last determination of this constant was conducted at LNE in 2000 with an uncertainty of 5.10-8. To achieve a target uncertainty of 1.10-8, the LNE decided to build a new standard capacitor and improve the associated measurement chain. The work presented here is implemented in the framework of the design/amelioration and the characterization of the measurement chain leading to the relative uncertainty of 1.10-8. Exploratory studies were also conducted about the possible partial or full automation of elements of the measurement chain.

L'impact des nuages de glace sur le cycle de l'eau et le bilan radiatif est encore incertain en raison de la complexité des processus nuageux qui rend difficile l'acquisition d'observations adéquates sur les propriétés des nuages de glace et leur représentation dans les modèles de circulation générale. Les instruments de télédétection actifs et passifs, tels que les radiomètres, les radars et les lidars, sont couramment utilisés pour les étudier. La restitution des propriétés microphysiques des nuages (extinction, contenu en glace, rayon effectif, ...) peut être effectuée à partir d'un seul instrument ou de la combinaison de plusieurs instruments. L’intérêt de l’utilisation de synergies instrumentales pour restituer les propriétés nuageuses réside dans le fait que cela permet de réduire les incertitudes dues aux lacunes des différents instruments pris séparément. La constellation de satellites A-Train a considérablement amélioré notre connaissance des nuages. Depuis 2006, le lidar à rétrodiffusion visible CALIOP embarqué à bord du satellite CALIPSO et le radar nuage à 94GHz CPR embarqué à bord du satellite CloudSat ont permis l’acquisition de profils nuageux sur l’ensemble du globe et de nombreuses méthodes synergiques de restitution ont été adaptées à ces instruments. En 2021 sera lancé un nouveau satellite, EarthCARE, embarquant des instruments de télédétection de pointe, notamment ATLID, un lidar à haute résolution spectrale (HSRL) à 355 nm et un radar nuage Doppler à 94 GHz. La mission principale de ce satellite est de quantifier les interactions entre les nuages, les aérosols et le bilan radiatif de la Terre afin d'améliorer les prévisions météorologiques et des modèles climatiques. Grâce à son instrumentation avancée installée sur une plate-forme unique, cette nouvelle mission devrait fournir des observations sans précédent des nuages depuis l'espace. Cependant, pour ce faire, les algorithmes synergiques développés pour les mesures de l'A-Train doivent être adaptés à cette nouvelle configuration instrumentale. Au cours de ma thèse, je me suis concentrée sur l'algorithme Varcloud développé en 2007 par Delanoë et Hogan et basé sur une technique variationnelle. La première partie du travail a consisté à adapter certains paramètres du modèle microphysique de l’algorithme aux études récentes d’une large base de données in situ. En particulier, les questions de la paramétrisation du rapport lidar et du choix de la relation masse-diamètre pour les cristaux de glace ont été abordées. La deuxième partie de mon travail a consisté à adapter l'algorithme de restitution Varcloud aux plates-formes aéroportées. Les plates-formes aéroportées sont idéales pour préparer et valider les missions spatiales, permettant de réaliser des mesures sous-trace, colocalisées avec les instruments spatiaux. En particulier, le HALO allemand et le Falcon 20 français ont des charges utiles très complémentaires et sont parfaitement conçus pour la préparation et la validation de la mission EarthCare. Les deux avions embarquent notamment un lidar à haute résolution spectrale (355 nm sur le Falcon et 532 nm sur le HALO) et un radar Doppler à 36 GHz (HALO) et 95 GHz (Falcon). À l'automne 2016, une campagne aéroportée dans laquelle les deux avions étaient impliqués s'est déroulée en Islande, à Keflavik, dans le cadre du projet NAWDEX. Les mesures recueillies au cours de cette campagne fournissent un ensemble de données intéressant pour caractériser la microphysique et la dynamique des nuages dans l'Atlantique Nord, région qui présent un grand intérêt pour les missions Cloudsat-CALIPSO et EarthCARE. En outre, une série de vols communs avec observation de la même scène nuageuse par les deux plates-formes ont été réalisées, fournissant des données permettant d'étudier l'influence de la configuration instrumentale sur les propriétés des nuages de glace restituées. / The impact of ice clouds on the water cycle and radiative budget is still uncertain due to the complexity of cloud processes that makes it difficult to acquire adequate observations of ice cloud properties and parameterize them into General Circulation Models. Passive and active remote sensing instruments, radiometers, radars and lidars, are commonly used to study ice clouds. Inferring cloud microphysical properties (extinction, ice water content, effective radius, ...) can be done from one instrument only, or from the synergy of several. The interest of using instrumental synergies to retrieve cloud properties is that it can reduce the uncertainties due to the shortcomings of the different instruments taken separately. The A-Train constellation of satellites has considerably improved our knowledge of clouds. Since 2006, the 532nm backscattering lidar CALIOP on board the satellite CALIPSO and the 94GHz cloud radar CPR on board the satellite CloudSat have acquired cloud vertical profiles globally and many lidar-radar synergetic methods have been adapted to CloudSat and CALIPSO data. In 2021 will be launched a new satellite, EarthCARE, boarding state of the art remote sensing instrumentation, in particular ATLID, a High Spectral Resolution Lidar (HSRL) at 355nm and a Doppler cloud radar at 94 GHz. The main mission of this satellite is to quantify interactions between clouds, aerosols and the Earth's radiation budget in order to improve weather prediction and climate models. Thanks to its advanced instrumentation mounted on a single platform, this new mission is expected to provide unprecedented observations of clouds from space. However, to do so, the synergistic algorithms that were developed for A-Train measurements have to be adapted to this new instrumental configuration. During my PhD, I focused on the Varcloud algorithm that was developed in 2007 by Delanoë and Hogan, based on a variational technique. The first part of the work consisted in adapting some parameters of the microphysical model of the algorithm to recent studies of a large dataset of in-situ measurements. In particular, the questions of a parameterization of the lidar extinction-to-backscatter ratio and the choice of the mass-size relationship for ice crystals were addressed. The second part of my work consisted in adapting the Varcloud retrieval algorithm to airborne platforms. Airborne platforms are ideal to prepare and validate space missions, allowing for direct underpasses of spaceborne instruments. Moreover, German and French aircraft, respectively HALO and French Falcon 20 have very complementary payloads and are perfectly designed for the preparation, the calibration and the validation of EarthCare. Both aircraft board a high spectral resolution lidar (355 nm on the French Falcon and 532 nm on the HALO) and a Doppler radar at 36 GHz (HALO) and 95 GHz (Falcon). In fall 2016 a field campaign related to the NAWDEX project took place in Iceland, Keflavik with both aircraft involved. The measurements collected during this campaign provide an interesting dataset to characterize cloud microphysics and dynamics in the North Atlantic, which are of high interest regarding the Cloudsat-CALIPSO and EarthCARE missions. In addition, a series of common legs with the same cloud scene observed by both platforms were performed, providing data to study the influence of the instrumental configuration on the retrieved ice cloud properties.

This thesis investigates a new approach for dealing with the adverse effects of large-scale deformations in the main reflector of large Cassegrain antennas. In this method, the incident aperture distribution is imaged onto a tertiary focal plane. This is accomplished by using an optical imaging system consisting of a lens mounted behind the Cassegrain focus of the antenna. The lens forms a real image of the product of the incident aperture distribution and the pupil function of the antenna. The pupil function describes the profile of the main reflector of the antenna. If the incident aperture distribution is a plane wave, a real image of the pupil function of the main reflector will be produced at the focal plane of the image lens. Any imperfections in the main reflector will be imaged onto the tertiary focal plane but over a smaller area as defined by the magnification of the system. In principle, an active correcting element placed into the tertiary focal plane could compensate for these errors, thus preserving the maximum efficiency of the antenna. Experimental verification of this principle was carried out in the lab using a dielectric lens 152.4mm in diameter. Phase perturbations were simulated by placing dielectric shims in the incident aperture plane. The phase of these shims in most cases was measured to within 10 degrees in the image plane. This degree of accuracy is found to be quite adequate for correcting large-scale errors in the main reflector of the antenna.

No description available.

Le European Extremely Large Telescope présentement en construction au Chili, sera le plus grand télescope optique jamais construit, avec son miroir primaire de 39 mètres de diamètre. Un de ses instruments, ANDES (ArmazoNes high Dispersion Echelle Spectrograph), combinera l’optique adaptative et la spectroscopie à haute dispersion dans les bandes photométriques YJH pour permettre notamment l’étude de la composition chimique d’atmosphères d’exoplanètes potentiellement habitables. La détection de la vie sur une exoplanète candidate commence nécessairement par l’étude de son atmosphère, et spécifiquement sa composition chimique. Celle-ci peut en effet révéler la présence de biosignatures, c’est-à-dire la signature spectrale de molécules qui ne pourraient exister sans la présence de la vie. Une paire de molécules particulièrement intéressante est la paire dioxygène (O2) et méthane (CH4), soient deux molécules qui peuvent être créées par des processus biotiques, mais qui, laissées à elles-mêmes, réagissent ensemble dans l’atmosphère pour générer de l’eau (H2O) et du dioxyde de carbone (CO2) jusqu’à la déplétion de l’une des deux (Thompson et al., 2022). La présence simultanée d’O2 et de CH4 nécessite donc des réactions chimiques hors équilibre comme celles associées avec l’activité biologique. ANDES sera équipé de tous les modules théoriquement nécessaires pour détecter la lumière réfléchie d'une exoplanète, incluant une interface d'optique adaptative qui minimise la lumière parasite de l'exoplanète localisée tout près du coeur de l'étoile, une unité de champ intégral permettant de disséquer l'image de l'étoile en des dizaines de spaxels, chacun alimentant un spectrographe infrarouge à haute dispersion. Des techniques statistiques bayesiennes sont ensuite utilisées pour détecter le signal atmosphérique de l'exoplanète enfoui dans le spectre de l'étoile. Ce travail décrit des simulations détaillées de tous ces modules afin de déterminer les capacités d’ANDES à détecter l’atmosphère d’exoplanètes potentiellement habitables, notamment Proxima b, la plus rapprochée du Système Solaire. Les simulations révèlent que si Proxima b a une atmosphère identique à celle de la Terre, l’eau y serait détectable en moins d'une nuit (6 heures), alors que les détections d’O2, de CO2 et de CH4 nécessiteraient jusqu’à 320, 420 et 1200 heures d’observation, respectivement. / The European Extremely Large Telescope, currently under construction in Chile, will be the largest telescope ever built, with its primary mirror measuring 39 meters in diameter. One of its instruments, ANDES (ArmazoNes high Dispersion Echelle Spectrograph), will combine adaptive optics and high dispersion dpectroscopy in the Y JH photometric bands. This combination will allow the study of the chemical composition of atmospheres of potentially habitable exoplanets. The search for life on a candidate exoplanet necessitates the study of its atmosphere, specically its chemical composition. This can reveal the presence of biosignatures, i.e the spectral signature of molecules that cannot exist without life. One inriguing pair of molecules is dioxygen (O2) and methane (CH4). Both can be created through biotic processes, but left to themselves, they form water (H2O) and carbon dioxide (CO2) until one of the two is depleted. The simultaneous presence of O2 and CH4 requires out-of-equilibrium chemical reactions, such as those associated with biological activity. ANDES will be equipped with all the crucial modules to detect the reflected light from an exoplanet. It includes an adaptive optics front-end interface that minimizes the stray light from the exoplanet located very close to the star’s core, an integrated field unit that dissects the star’s image into dozens of spaxels, each feeding a high-dispersion infrared spectrograph. Bayesian statistics are then used to detect the exoplanet’s atmospheric signal buried within the star’s spectrum This work describes detailed simulations of all these modules to determine ANDES’ ca- pabilities in detecting the atmosphere of potentially habitable exoplanets, notably Proxima b, the closest to the Solar System. The simulations reveal that if Proxima b has an atmo- sphere similar to Earth’s, water could be detectable in less than one night (6 hours), while detections of O2, CO2 and CH4 could require up to 320, 420 and 1200 hours of observations, respectively.

This project explores the possibilities and challenges associated with writing for and performing with an unconventional, and for the composer new set of instruments. With the purpose of creating music out of intuitive, creative ideas rather than instrumentally based knowledge and habitual patterns I wrote and/or arranged six original songs for an ensemble consisting of lead vocals, accordion, trumpet/flugel horn, electric guitar, and a cellist and vocalist combined in one. We later performed the music at my bachelor’s recital which took place on the 3rd of April 2024 at the Royal College of Music in Stockholm.  The analysis of the musical result highlighted two compositional structures which in turn effected the co-playing in the group and divided the role-based responsibilities differently. The structure which was based around homophonic voices led to a common phrasing being the most important focus in comparison to the other which divided the ensemble into smaller groups with different functions where a joint time feel was of most importance. / <p><strong>Musik:</strong></p><p>Sinking into a Dream</p><p>Buss 61</p><p>Time and Places </p><p>Utegymmet</p><p>Botanical Garden</p><p>Pick Up </p><p>Kompositioner och arrangemang av: Ellen Mansten Bruchfeld</p><p></p><p><strong>Medverkande musiker:</strong></p><p>Anna Østerby – dragspel</p><p>Hannes Arason – trumpet och flygelhorn</p><p>Linnea Hildén – cello och sång</p><p>Svante Qvennerstedt – elgitarr</p><p>Ellen Mansten Bruchfeld – sång </p>

Doctor of Philosophy / Department of Physics / Kristan L. Corwin / Optical frequency references have been widely used in applications such as navigation, remote sensing, and telecommunication industry. For stable frequency references in the near-infrared (NIR), lasers can be locked to narrow absorption features in gases such as acetylene. Currently, most Near NIR references are realized in free space setups. In this thesis, a low-loss hollow-core optical fiber with a diameter of sub millimeters is integrated into the reference setup to provide long interaction lengths between the filling gas and the laser field, also facilitate the optical interaction with low power levels. To make portable NIR reference, gas can be sealed inside the hollow-core fiber, by creating a photonic microcell. This work has demonstrated all-fiber optical frequency references in the Near IR by fabricating and integrating gas sealed photonic microcells in the reference setup. Also, a thoughtful study regarding the lineshape of the fiber-based reference has been accomplished. According the proper modeling of a shift due to lineshape, a correction was applied to our previous absolute frequency measurement of an NIR optical frequency reference. Furthermore, effects of the hollow-core fibers, including mode-dependence frequency shift related to surface modes are explored. In addition, angle splicing techniques, which will improve the performance of the fiber-based frequency reference have been created. Low transmission and return loss angle splices of photonic bandgap fiber, single mode PCF, and large core kagome to SMF-28 are developed and those fibers are demonstrated to be promising for photonic microcell based optical frequency references. Finally, a potentially portable optical metrology system is demonstrated by stabilizing a fiber-laser based frequency comb to an acetylene-filled optical fiber frequency reference. Further work is necessary to fabricate an all-fiber portable optical metrology system with high optical transmission and low molecular contamination.

Vocal folds are the twin in-folding of the mucous membrane stretched horizontally across the larynx. They vibrate modulating the constant air flow initiated from the lungs. The pulsating pressure wave blowing through the glottis is thus the source for voiced speech production. Study of vocal fold dynamics during voicing are critical for the treatment of voice pathologies. Since the vocal folds move at 100 - 350 cycles per second, their visual inspection is currently done by strobosocopy which merges information from multiple cycles to present an apparent motion. High Speed Digital Laryngeal Imaging(HSDLI) with a temporal resolution of up to 10,000 frames per second has been established as better suited for assessing the vocal fold vibratory function through direct recording. But the widespread use of HSDLI is limited due to lack of consensus on the modalities like features to be examined. Development of the image processing techniques which circumvents the need for the tedious and time consuming effort of examining large volumes of recording has room for improvement. Fundamental questions like the required frame rate or resolution for the recordings is still not adequately answered. HSDLI cannot get the absolute physical measurement of the anatomical features and vocal fold displacement. This work addresses these challenges through improved signal processing. A vocal fold edge extraction technique with subpixel accuracy, suited even for hard to record pediatric population is developed first. The algorithm which is equally applicable for pediatric and adult subjects, is implemented to facilitate user inspection and intervention. Objective features describing the fold dynamics, which are extracted from the edge displacement waveform are proposed and analyzed on a diverse dataset of healthy males, females and children. The sampling and quantization noise present in the recordings are analyzed and methods to mitigate them are investigated. A customized Kalman smoothing and spline interpolation on the displacement waveform is found to improve the feature estimation stability. The relationship between frame rate, spatial resolution and vibration for efficient capturing of information is derived. Finally, to address the inability to measure physical measurement, a structured light projection calibrated with respect to the endoscope is prototyped.

ITC/USA 2006 Conference Proceedings / The Forty-Second Annual International Telemetering Conference and Technical Exhibition / October 23-26, 2006 / Town and Country Resort & Convention Center, San Diego, California / This paper presents the description of the updated Data Display Markup Language (DDML), a neutral format for data display configurations. The development of DDML is motivated by the fact that in joint service program systems, there is a critical need for common data displays to support distributed T&E missions, irrespective of the test location, data acquisition system, and display system. DDML enables standard data displays to be specified for any given system under test, irrespective of the display vendor or system in which they will be implemented. The version 3.0 of DDML represents a more mature language than the version 1.0 presented at the 2003 ITC. The updated version has been validated for completeness and robustness by developing translators between DDML and numerous vendor formats. The DDML schema has been presented to the Range Commander’s Council (RCC) Data Multiplex Committee for consideration for inclusion in the IRIG 106 standard. The DDML model will be described in terms of both the XML schema and the UML model, and various examples of DDML models will be presented. The intent of this paper is to solicit specific input from the community on this potential RCC standard.