Non-common path aberrations (NCPA) in an adaptive optics system are static aberrations that appear due to the difference in optical path between light arriving at the wavefront sensor (WFS) and at the science detector. If the adaptive optics are calibrated to output an unaberrated wavefront, then any optics outside the path of the light arriving at the WFS inherently introduce aberrations to this corrected wavefront. NCPA corrections calibrate the adaptive optics system such that it outputs a wavefront that is inverse in phase to the aberrations introduced by these non-common path optics, and therefore arrives unaberrated at the science detector, rather than at the output of the corrective elements. Focal plane sharpening (FPS) is one technique used to calibrate for NCPA in adaptive optics systems. Small changes in shape to the deformable element(s) are implemented and images are taken and analyzed for image quality (IQ) on the science detector. This process is iterated until the image quality is maximized and hence the NCPA are corrected. The work carried out as described in this paper employs two FPS techniques at Gemini North to attempt to mitigate up to 33% of the adaptive optics performance and image quality degradations currently under investigation. Changes in the NCPA correction are made by varying the Zernike polynomial coefficients in the closed-loop correction file for Altair (the facility adaptive optics system). As these coefficients are varied during closed-loop operation, a calibration point-source at the focal plane of the telescope is imaged through Altair and NIRI (the facility near-infrared imager) at f/32 in K-prime (2.12 μm). These images are analyzed to determine the Strehl ratio, and a parabolic fit is used to determine the appropriate coefficient correction that maximizes the Strehl ratio. Historic calibrations of the NCPA file in Altair's control loop were done at night on a celestial point source, and used a separate, high-resolution WFS (with its own inherent aberrations not common to either NIRI nor Altair) to measure phase corrections directly. In this paper it is shown that using FPS on a calibration source negates both the need to use costly time on the night sky and the use of separate optical systems (which introduce their own NCPA) for analysis. An increase of 6% in Strehl ratio is achieved (an improvement over current NCPA corrections of 11%), and discussions of future improvements and extensions of the technique is presented. Furthermore, a potentially unknown problem is uncovered in the form of high spatial frequency degradation in the PSF of the calibration source.

L'objectif de ce travail est le développement d'un interféromètre à chemin commun entièrement passif pour détecter des ondes acoustiques hautes fréquences (GHz-THz). Ce travail s'inscrit dans le domaine de l'acoustique picoseconde. La génération et la détection des ultrasons sont réalisées par l'utilisation combinée de lasers impulsionnels et de dispositifs pompe-sonde résolus en temps. L'originalité de la détection interférométrique proposée réside dans l'utilisation d'un unique cristal biréfringent pour créer une paire d'impulsions séparée de quelques picosecondes puis les recombiner et générer les interférences. Nous dressons dans le premier chapitre un état de l'art des différentes méthodes interférométriques actuellement utilisées en acoustique picoseconde. Dans le second chapitre nous détaillons le principe de l'interféromètre développé et nous modélisons son fonctionnement à l'aide du formalisme de Jones. Nous montrons que, suite à l'excitation induite par l'impulsion pompe, il est possible de mesurer indépendamment la dérivée temporelle de l'amplitude ou de la phase du changement relatif de réflectivité de l'échantillon. Enfin, le troisième chapitre est consacré à la caractérisation expérimentale de l'interféromètre puis à l'illustration des potentialités de cet interféromètre en acoustique picoseconde. Les expériences ont été réalisées sur deux échantillons différents : un film mince optiquement absorbant puis un film transparent déposé sur un transducteur métallique. / The purpose of this work is to develop a fully passive in-line common-path femtosecond interferometer for the detection of high frequencies acoustic waves (GHz-THz). This work falls within the picosecond acoustic domain. The generation and the detection of ultrasounds are performed through the combined use of pulsed lasers and optical pump-probe time-resolved setups. The originality of the interferometric detection we propose lies in the use of a single birefringent crystal frst to generate a pair of phase-locked pulses and second to recombine them to interfere. We present in the first chapter a state-of-the-art of the interferometric setups currently used in picosecond acoustics. In the second chapter, we describe the principle of operation of the interferometer we have developed. Then we model the sensitivity of the interferometer inthe framework of the Jones formalism. We show that it is possible to measure independently the pump-induced modification of either the real or imaginary parts of the complex reflection coefficient of the sample. Finally, in the third chapter, the experimental characterization of the setup is detailed and we illustrate the performance of the interferometer through picosecond opto-acoustic measurements. Experiments are performed on two different samples : an opticallyabsorbing thin film and a transparent substrate coated with a metallic transducer.

The Swedish Energy Agency has a target to increase solar photovoltaics (PV) power production by up to 5-10% of the total electricity demand by the year 2040. The PV potential for the residential market is high and its contribution to the total installed PV capacity is expected to increase significantly. The technical requirements should be met to keep high reliability and good power quality at the customers, therefore, it is important for planning reasons to proactively find the maximum amount PV power that can be connected at each low-voltage network without violating the performance of the grid. This amount is known as the hosting capacity. A method for PV hosting capacity estimation by taking overvoltage and transformer overload as performance indices was developed in this thesis. The method does not require any knowledge about the topology of the network. The overload hosting capacity can be estimated for any combination of customers having PV power and for the overvoltage hosting, the minimum at each penetration level can be estimated. The method was implemented on four low-voltage networks located in a typical Vattenfall medium-voltage network and the comparison of the estimation results to a power flow simulation showed good correspondence. It was shown how the impact of PV power in adjacent secondary substations can be accounted for. Using SS-EN50160 voltage limits, the studied networks were able to handle 3-7 times the PV penetration level needed (8 kWp at 20% of the customers) to achieve the national goal in Sweden without grid investments.