Uma simulação baseada em métodos Monte Carlo foi criada com o intuito de avaliar a potencialidade da utilização do espalhamento Compton em altas energias para a obtenção de medidas absolutas e de alta precisão da energia de fótons marcados. Esse método se baseia em medidas angulares dos produtos desse espalhamento para reconstruir a energia dos fótons incidentes, utilizando a cinemática do espalhamento Compton em aproximação de impulso. A simulação inclui vários efeitos relevantes à medida, como espalhamento múltiplo de elétrons, momento interno dos elétrons nos átomos do alvo, resolução do detetor e vários parâmetros geométricos do arranjo experimental. Através da simulação de um experimento que utiliza esse método para a calibração em energia de um feixe de fótons marcados, foi possível identificar duas fontes de erros sistemáticos. Métodos de análise que minimiza um desse erros sistemáticos foram desenvolvidos, bem como métodos para a criação de correções para as medidas de energia. Verificou-se que, pelo menos no arranjo experimental estudado, é possível obter medidas da energia dos fótons incidentes com precisão da ordem de 0.07%. / A simulation based on Monte Carlo methods was created in order to evaluate the potentiality of using Compton scattering at high energies to obtain high precision absolute measurements of tagged photon energies. This method is based on angular measurements of the scattering products to reconstruct the incident photon energy using the kinematics of Compton scattering in impulse approximation. The simulation includes several effects that are relevant to the measurement, such as electron multiple scattering, internal momentum of the electrons in the atoms of the target, detector resolution and several geometrical parameters of the experimental setup. Through simulation of an experiment that uses this method for energy calibration of a tagged photon beam, it was possible to identify two sources of systematic errors. Analysis methods that minimize one of these systematic errors were developed, as well as methods for the creation of corrections to the energy measurements. Our results show that, at least in the studied experimental setup, it is possible to obtain energy measurements with a precision in the order of 0.07%.

Em vista de recentes determinações experimentais do perfil de Compton (Eisenberger, Phys. Rev., A2, 1678(1970); Wellenstein e Bonham, Phys. Rev., A7, 1568(1973}, procuramos efetuar um estudo comparativo de cálculos teóricos do perfil de Compton para o átomo de hélio (1S). Para tal, o conjunto de funções de onda elaboradas por Shull e L6wdin (J.Chem.Phy., 23, 1362(1955); 23, 1565(1955}; 30, 617(1959} mostrou-se bastante adequado, visto que permitiu observar a influência da função de onda no cálculo de perfil de Compton. Nossos resultados mostram em contraste à idéia geralmente aceita, que mesmo funções de onda igualmente boas para o cálculo da energia podem fornecer perfis de Compton com um erro maior que o experimental. Alem disso, apresentamos um conjunto de novos dados para o perfil de Compton e para a distribuição radial de momentum. Procuramos, também explicar essas discrepâncias relacionando-as com a transformada de Fourier da função de onda no espaço de configuração. / In view of the recent experimental determination of the Compton profile (Eisenberger, Phys., Rev., A2,1678(1970); Wellenstein and Bonham, Phys, Rev., A7, 1568(1973), we have performed a comparative study of theoretical calcu1ation of the Compton profile for the helium atom (1S). For such, the set of wave functions elaborated by Shull and Löwdin (J.Chem. Phys., 23, 1362(1955); 23, 1565(1955); 30, 617(1959) show itself specially suftable since it was possible to observe the influence af the wave functions on the calculated profile. Our results show in, contrast to general accepted idea, that even equally good wave functions in the energy sense may give theoretical profiles in error greater than the experimental one. Besides, we have presented a set of new data for the Compton profile and radial momentum distribution. A1so we have tried to explain the source of these discrepancies relating them to the Fourier transformation of the wave function in the configuration space.

In dieser Arbeit wird die Bildgebung durch eine Compton-Kamera zur Überwachung der Partikelstrahlentherapie erstmals an der Technischen Universität Dresden untersucht. Die inhärenten Beschränkungen der Methode wurden durch Berechnungen und Monte Carlo Simulationen studiert. Im Zuge dieser Untersuchungen erschien der Raumtemperatur-Halbleiter Cadmium Zink Tellurid als ein vielversprechendes Detektor-Material. Zur weiteren Untersuchung wurde eine einfache Compton-Kamera konstruiert bestehend aus einem Cadmium Zink Tellurid Detektor und einem ortsempfndlichen Szintillationsdetektor. Das System hat gezeigt, dass eine akkurate Bildgebung mit radioaktiven Punktquellen unter Laborbedingungen möglich ist. Weitere praktische Beschränkungen der Compton-Bildgebung unter Strahlbedingungen konnten durch Experimente an einem Protonen-Strahl hergeleitet werden. Durch die experimentellen Erfahrungen mit der in dieser Arbeit entwickelten Compton-Kamera konnten wertvolle Informationen gesammelt werden, die erlauben, die Bildrekonstruktion zu evaluieren und dazu beitragen, die weitere Forschung hin zu einer klinisch anwendbaren Compton-Kamera zu leiten. / This work presents the first efforts at the Dresden University of Technology to study the feasibility of Compton imaging as a modality to monitor ion beam radiation therapy. The inherent limitations of the method have been studied by means of calculation and Monte Carlo simulation. As a result, the room-temperature semiconductor cadmium zinc telluride appeared as a promising detector material for a clinical device. For more detailed investigation, a simple Compton camera has been constructed comprising a cadmium zinc telluride detector and a position sensitive scintillation detector. This system has proven that accurate imaging of radioactive point sources in the laboratory is feasible. More practical restrictions of Compton imaging in beam conditions have been derived through experiments at a proton facility. Through the experimental work with the Compton camera developed in this work, valuable information was gathered which allowed to test the image reconstruction and to direct the further research towards a clinical Compton camera system.

Ultrashort, nearly monochromatic hard X-ray pulses enrich the understanding of the dynamics and function of matter, e.g., the motion of atomic structures associated with ultrafast phase transitions, structural dynamics and (bio)chemical reactions. Inverse Compton backscattering of intense laser pulses from relativistic electrons not only allows for the generation of bright X-ray pulses which can be used in a pump-probe experiment, but also for the investigation of the electron beam dynamics at the interaction point. The focus of this PhD work lies on the detailed understanding of the kinematics during the interaction of the relativistic electron bunch and the laser pulse in order to quantify the influence of various experiment parameters on the emitted X-ray radiation. The experiment was conducted at the ELBE center for high power radiation sources using the ELBE superconducting linear accelerator and the DRACO Ti:sapphire laser system. The combination of both these state-of-the-art apparatuses guaranteed the control and stability of the interacting beam parameters throughout the measurement. The emitted X-ray spectra were detected with a pixelated detector of 1024 by 256 elements (each 26μm by 26μm) to achieve an unprecedented spatial and energy resolution for a full characterization of the emitted spectrum to reveal parameter influences and correlations of both interacting beams. In this work the influence of the electron beam energy, electron beam emittance, the laser bandwidth and the energy-angle-correlation on the spectra of the backscattered X-rays is quantified. A rigorous statistical analysis comparing experimental data to ab-initio 3D simulations enabled, e.g., the extraction of the angular distribution of electrons with 1.5% accuracy and, in total, provides predictive capability for the future high brightness hard X-ray source PHOENIX (Photon electron collider for Narrow bandwidth Intense X-rays) and potential all optical gamma-ray sources. The results will serve as a milestone and starting point for the scaling of the X-ray flux based on available interaction parameters of an ultrashort bright X-ray source at the ELBE center for high power radiation sources. The knowledge of the spatial and spectral distribution of photons from an inverse Compton scattering source is essential in designing future experiments as well as for tailoring the X-ray spectral properties to an experimental need. / Ultrakurze, quasi-monochromatische harte Röntgenpulse erweitern das Verständnis für die dynamischen Prozesse und funktionalen Zusammenhänge in Materie, beispielsweise die Dynamik in atomaren Strukturen bei ultraschnellen Phasenübergängen, Gitterbewegungen und (bio)chemischen Reaktionen. Compton-Rückstreuung erlaubt die Erzeugung der für ein pump-probe-Experiment benötigten intensiven Röntgenpulse und ermöglicht gleichzeitig einen Einblick in die komplexen kinematischen Prozesse während der Wechselwirkung von Elektronen und Photonen. Ziel dieser Arbeit ist, ein quantitatives Verständnis der verschiedenen experimentellen Einflüsse auf die emittierte Röntgenstrahlung bei der Streuung von Laserphotonen an relativistischen Elektronen zu entwickeln. Die Experimente wurden am ELBE - Zentrum für Hochleistungs-Strahlenquellen des Helmholtz-Zentrums Dresden - Rossendorf durchgeführt. Der verwendete supraleitende Linearbschleuniger ELBE und der auf Titan-Saphir basierende Hochleistungslaser DRACO garantieren ein Höchstmaß an Kontrolle und Stabilität der experimentellen Bedingungen. Zur Messung der emittierten Röntgenstrahlung wurde ein Siliziumdetektor mit 1024x256 Pixeln (Pixelgröße 26μm × 26μm) verwendet, welcher für eine bisher nicht erreichte spektrale und räumliche Auflösung sorgt. Die so erfolgte vollständige Charakterisierung der Energie-Winkel-Beziehung erlaubt Rückschlüsse auf Parametereinflüsse und Korrelationen von Elektronen- und Laserstrahl. Eine umfassende statistische Analyse, bei der ab-initio 3D Simulationen mit den experimentellen Daten verglichen und ausgewertet wurden, ermöglichte u.a. die Bestimmung der Elektronenstrahldivergenz mit einer Genauigkeit von 1.5% und erlaubt Vorhersagen zur zu erwartenden Strahlung der zukünftigen brillianten Röntgenquelle PHOENIX (Photon electron collider for Narrow bandwidth Intense X-rays) und potentiellen lasergetriebenen Gammastrahlungsquellen. Die Ergebnisse dienen als Fixpunkt für die Skalierung des erwarteten Photonenflusses der Röntgenquelle für die verfügbaren Ausgangsgrößen am Helmholtz-Zentrum Dresden - Rossendorf. Das Wissen um die räumliche und spektrale Verteilung der Röntgenstrahlung ist entscheidend für die Planung zukünftiger Experimente sowie zur Anpassung der Quelle an experimentelle Bedürfnisse.

Ultrashort, nearly monochromatic hard X-ray pulses enrich the understanding of the dynamics and function of matter, e.g., the motion of atomic structures associated with ultrafast phase transitions, structural dynamics and (bio)chemical reactions. Inverse Compton backscattering of intense laser pulses from relativistic electrons not only allows for the generation of bright X-ray pulses which can be used in a pumpprobe experiment, but also for the investigation of the electron beam dynamics at the interaction point. The focus of this PhD work lies on the detailed understanding of the kinematics during the interaction of the relativistic electron bunch and the laser pulse in order to quantify the influence of various experiment parameters on the emitted X-ray radiation. The experiment was conducted at the ELBE center for high power radiation sources using the ELBE superconducting linear accelerator and the DRACO Ti:sapphire laser system. The combination of both these state-of-the-art apparatuses guaranteed the control and stability of the interacting beam parameters throughout the measurement. The emitted X-ray spectra were detected with a pixelated detector of 1024 by 256 elements (each 26μm by 26μm) to achieve an unprecedented spatial and energy resolution for a full characterization of the emitted spectrum to reveal parameter influences and correlations of both interacting beams. In this work the influence of the electron beam energy, electron beam emittance, the laser bandwidth and the energy-anglecorrelation on the spectra of the backscattered X-rays is quantified. A rigorous statistical analysis comparing experimental data to ab-initio 3D simulations enabled, e.g., the extraction of the angular distribution of electrons with 1.5% accuracy and, in total, provides predictive capability for the future high brightness hard X-ray source PHOENIX (Photon electron collider for Narrow bandwidth Intense X-rays) and potential all optical gamma-ray sources. The results will serve as a milestone and starting point for the scaling of the Xray flux based on available interaction parameters of an ultrashort bright X-ray source at the ELBE center for high power radiation sources. The knowledge of the spatial and spectral distribution of photons from an inverse Compton scattering source is essential in designing future experiments as well as for tailoring the X-ray spectral properties to an experimental need. / Ultrakurze, quasi-monochromatische harte Röntgenpulse erweitern das Verständnis für die dynamischen Prozesse und funktionalen Zusammenhänge in Materie, beispielsweise die Dynamik in atomaren Strukturen bei ultraschnellen Phasenübergängen, Gitterbewegungen und (bio)chemischen Reaktionen. Compton-Rückstreuung erlaubt die Erzeugung der für ein pump-probe-Experiment benötigten intensiven Röntgenpulse und ermöglicht gleichzeitig einen Einblick in die komplexen kinematischen Prozesse während der Wechselwirkung von Elektronen und Photonen. Ziel dieser Arbeit ist, ein quantitatives Verständnis der verschiedenen experimentellen Einflüsse auf die emittierte Röntgenstrahlung bei der Streuung von Laserphotonen an relativistischen Elektronen zu entwickeln. Die Experimente wurden am ELBE - Zentrum für Hochleistungs-Strahlenquellen des Helmholtz-Zentrums Dresden - Rossendorf durchgeführt. Der verwendete supraleitende Linearbschleuniger ELBE und der auf Titan-Saphir basierende Hochleistungslaser DRACO garantieren ein Höchstmaß an Kontrolle und Stabilität der experimentellen Bedingungen. Zur Messung der emittierten Röntgenstrahlung wurde ein Siliziumdetektor mit 1024x256 Pixeln (Pixelgröße 26μm × 26μm) verwendet, welcher für eine bisher nicht erreichte spektrale und räumliche Auflösung sorgt. Die so erfolgte vollständige Charakterisierung der Energie-Winkel-Beziehung erlaubt Rückschlüsse auf Parametereinflüsse und Korrelationen von Elektronen- und Laserstrahl. Eine umfassende statistische Analyse, bei der ab-initio 3D Simulationen mit den experimentellen Daten verglichen und ausgewertet wurden, ermöglichte u.a. die Bestimmung der Elektronenstrahldivergenz mit einer Genauigkeit von 1.5% und erlaubt Vorhersagen zur zu erwartenden Strahlung der zukünftigen brillianten Röntgenquelle PHOENIX (Photon electron collider for Narrow bandwidth Intense X-rays) und potentiellen lasergetriebenen Gammastrahlungsquellen. Die Ergebnisse dienen als Fixpunkt für die Skalierung des erwarteten Photonenflusses der Röntgenquelle für die verfügbaren Ausgangsgrößen am Helmholtz-Zentrum Dresden - Rossendorf. Das Wissen um die räumliche und spektrale Verteilung der Röntgenstrahlung ist entscheidend für die Planung zukünftiger Experimente sowie zur Anpassung der Quelle an experimentelle Bedürfnisse.

Thesis (Ph. D.)--University of Wisconsin--Madison, 1968. / Typescript. Vita. Description based on print version record. Includes bibliographical references.

No último século, houve grande avanço no entendimento das interações das radiações com a matéria. Essa compreensão se faz necessária para diversas aplicações, entre elas o uso de raios X no diagnóstico por imagens. Neste caso, imagens são formadas pelo contraste resultante da diferença na atenuação dos raios X pelos diferentes tecidos do corpo. Entretanto, algumas das interações dos raios X com a matéria podem levar à redução da qualidade destas imagens, como é o caso dos fenômenos de espalhamento. Muitas abordagens foram propostas para estimar a distribuição espectral de fótons espalhados por uma barreira, ou seja, como no caso de um feixe de campo largo, ao atingir um plano detector, tais como modelos que utilizam métodos de Monte Carlo e modelos que utilizam aproximações analíticas. Supondo-se um espectro de um feixe primário que não interage com nenhum objeto após sua emissão pelo tubo de raios X, este espectro é, essencialmente representado pelos modelos propostos anteriormente. Contudo, considerando-se um feixe largo de radiação X, interagindo com um objeto, a radiação a ser detectada por um espectrômetro, passa a ser composta pelo feixe primário, atenuado pelo material adicionado, e uma fração de radiação espalhada. A soma destas duas contribuições passa a compor o feixe resultante. Esta soma do feixe primário atenuado, com o feixe de radiação espalhada, é o que se mede em um detector real na condição de feixe largo. O modelo proposto neste trabalho visa calcular o espectro de um tubo de raios X, em situação de feixe largo, o mais fidedigno possível ao que se medem em condições reais. Neste trabalho se propõe a discretização do volume de interação em pequenos elementos de volume, nos quais se calcula o espalhamento Compton, fazendo uso de um espectro de fótons gerado pelo Modelo de TBC, a equação de Klein-Nishina e considerações geométricas. Por fim, o espectro de fótons espalhados em cada elemento de volume é somado ao espalhamento dos demais elementos de volume, resultando no espectro total espalhado. O modelo proposto foi implementado em ambiente computacional MATLAB® e comparado com medições experimentais para sua validação. O modelo proposto foi capaz de produzir espectros espalhados em diferentes condições, apresentando boa conformidade com os valores medidos, tanto em termos quantitativos, nas quais a diferença entre kerma no ar calculado e kerma no ar medido é menor que 10%, quanto qualitativos, com fatores de mérito superiores a 90%. / The understanding of the interactions between radiation and matter advanced considerably in the last century. This understanding was needed by several applications, such as the use of X-rays in diagnostic imaging. In diagnostic applications, the image is created by the contrast resulting from the X-ray attenuation by the different body tissues. However, some interactions between the X-rays with the matter may reduce the quality of the images obtained in diagnostic imaging, as is the case of the scattering phenomenon. There are several modeling approaches to estimate the spectral distribution of photons scattered through a barrier, as in the case of a broad beam hitting a spectrometer detector. For instance, there are approaches that use Monte Carlo methods and approaches that use analytical approximations. Assuming a primary spectrum that does not interact with any object after its issuance by the X -ray tube, this spectrum is essentially represented by the previously proposed models. However, considering a broad beam of X-rays interacting with an object, the radiation to be detected by a spectrometer is now composed of the primary beam attenuated by the added material, and a scattered radiation fraction. The sum of these two contributions becomes part of the resulting beam. This sum of attenuated primary beam with the scattered radiation beam is what is measured in a real detector in broad beam condition. The model proposed in this work aims to simulate the spectrum of an x-ray tube in wide beam situation, the most reliable possible to what is measured in real conditions. In this work we propose the discretisation of the volume of interaction into small volume elements, which are used to calculate the Compton scattering. The spectrum of the photon spreading in each volume element is added to other volume elements, resulting in the spectrum of the whole barrier. The proposed model was implemented in MATLAB®, a computational environment. We evaluate the model by comparing the computational results with results from physical experiments. The model we propose was capable of creating accurate distribution of the spectrum spreading, under different conditions and in different experiments. The model results were close to the results obtained by experimental evaluation, both quantitatively, such as the difference smaller than 10% between the simulated air kerma and the measured air kerma obtained in the experimental evaluation, and qualitatively.

Estimamos os valores das polarizabilidades dipolares elétrica e magnética do próton, levando em conta as contribuições das ressonâncias nucleônicas de menor massa: P33 (1236), P11 (1450), D13 (1525), S11(1550), e da ressonância mesônica &#949 (660). O valor obtido para a soma das polarizabilidades concorda bem com os dados experimentais. Por outro lado, o valor obtido para cada uma delas, que depende do valor não bem determinado da largura do decaimento &#949 &#8594 &#933 &#933, é compatível com os valores experimentais / We have estimated the values of electric and magnetic polarizabilities of the proton, taking into account the contributions of the low masses nucleon ressonances : P33 (1236), P11 (1450), D13 (1525), S11(1550) and the meson ressonance &#949 (660). The obtained value for the sumo f the polarizabilities is in good agreement with the experimental data. On the other hand, the value, of each polarizability, which depends on the not too well determined width decay &#949 &#8594 &#933 &#933, is compatible with experimental values

Este trabalho apresenta um novo tomógrafo de espalhamento de fótons por efeito Compton para estudos de solos agrícolas em ambiente de campo. O seu desenvolvimento está fundamentado na física computacional, em uma instrumentação nuclear avançada e nas técnicas do espalhamento Compton. O posicionamento lado a lado da fonte de raios X e do detector de estado sólido, operando em efeito Compton, viabiliza uma técnica não invasiva para aplicação direta em campo agrícola, não necessitando coleta de amostras e preservando as condições naturais do solo. Este tomógrafo Compton de campo possui um sistema de detecção baseado em fotodiodo de Silício (SDD - Silicon Drift Detector) com eficiência de detecção de 18,9% (@ 35 keV), módulo eletrônico de processamento de sinais de dimensões reduzidas (7,0x10,0x2,5 cm) e baixo consumo de energia elétrica (2,5 W). Outro aspecto relevante é a sua sonda de medida que viabiliza a coleta de projeções tomográficas, bem como o georeferenciamento que permite uma correta identificação da localização das análises. Resultados obtidos diretamente em um campo agrícola viabilizaram a obtenção de imagens tomográficas com resolução espacial 1x1 cm2, faixa de abordagem de 10x10 cm2, medidas densitométricas na faixa de 1,0 a 1,3 g/cm3 e energia de 37,8 keV, o que viabilizou medidas em profundidade de interesse agrícola. / This research presents a new tomograph scattering of photons by the Compton Effect for studies of agricultural soils in a field environment. Its development is based on computational physics, in an advanced nuclear instrumentation and techniques of Compton scattering. The side by side position of X-ray source and solid-state detector, operating in the Compton Effect, enables a noninvasive technique for direct application in the agricultural field, without sampling and preserving the natural soil conditions. This field Compton tomograph has a detection system based on Silicon photodiode (SDD Silicon Drift Detector) with detection efficiency of 18.9% (@ 35keV), electronic module of signal processing with reduced dimensions (7.0 x 10.0 x 2.5 cm) and low power consumption (2.5 W). Another relevant aspect is its measuring probe that enables the acquisition of tomographic projections and its georeferencing that allows a correct identification of the analysis location. Results obtained directly in agricultural field enabled the achievement of tomographic images with spatial resolution of 1x1cm2, range approach of 10x10 cm2, densitometric measurements in the range from 1.0 to 1.3 g/cm3 and energy of 37.8 keV, which enabled in-depth measures of agricultural interest.

La diffusion Compton inverse est un moyen unique pour produire des rayons X quasi-monochromatiques via l'interaction entre des électrons relativistes et une impulsion laser. Ce processus présente l'avantage de produire des flux très élevés de rayons X avec des énergies supérieures à quelques dizaines de keV. De plus, la divergence du faisceau de sortie est beaucoup plus grande que dans les sources de lumière synchrotron classiques et le faisceau de rayons X est donc plus facile à manipuler. Nous présentons une source de rayons X en construction à l'Université Paris-Sud, ThomX. Cette source utilise un faisceau d'électrons de 50 MeV qui interagit à 16,7 MHz avec une impulsion laser de quelques picosecondes dont la puissance moyenne est à l'état de l'art avec 600 kW, permettant de produire des rayons X entre 30 et 50 keV avec un flux de 10^{13} ph/s. Cette gamme d'énergie ainsi que la dépendance énergie-angulaire provenant du processus physique conviennent aux applications sociétales comme la radiothérapie ou l'histoire de l'art.Une cavité optique de très haute finesse (> 24000) est utilisée comme prototype pour effectuer des travaux de R&D pour la source ThomX. 400 kW de puissance laser moyenne ont été stockés avec succès dans cette cavité, en utilisant un faisceau laser d'entrée de seulement 40 W. Ce résultat, unique au monde, permet d'envisager l'achèvement de la source de rayons X de faible coût et de haut flux ThomX. Cette thèse explique les études expérimentales et analytiques qui ont été réalisées pour atteindre cette performance, dont une généralisation du processus d'empilement des impulsions laser pour les faisceaux laser ayant une fréquence de répétition différente de celle de la cavité, et les méthodes développées pour l'amélioration expérimentale du couplage spatial. / Inverse Compton Scattering provides a unique way to produce quasi-monochromatic X-rays via the interaction of relativistic electrons with a laser pulse. This process has the advantage of producing very high fluxes of X-rays with energies above a few tens of keV. In addition the output beam divergence is much larger than in classical synchrotron light sources and the X-ray beam is thus easier to manipulate. We present an X-ray source under construction at Paris-Sud University, ThomX. This source uses a 50 MeV electron beam that collides at 16.7 MHz with a few picoseconds pulsed laser beam whose power is enhanced at the state of the art 600 kW average power to produce X-rays between 30 and 50 keV with a flux of 10^{13} ph/s. This energy range as well as the energy-angular dependence coming from the physical process are suitable for societal applications like radiotherapy or art history.A very high finesse optical cavity (> 24000) is used as a prototype to perform R&D for the ThomX source. 400 kW of average laser power have been successfully stored in this cavity, using an input laser beam of only 40 W. This result, unique in the world, is a pathway towards the completion of the low-cost, compact, high flux X-ray source ThomX. This thesis explains the experimental and analytical studies that have been performed to reach this performance, including a generalization of the process of laser pulse stacking to frequency-detuned laser beams, and the methods developped for experimental spatial coupling enhancement.