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Dissertations / Theses on the topic 'Roy Hart'

Author: Grafiati

Published: 4 June 2021

Last updated: 2 February 2022

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1

Backes, Laura Beatriz. "Voz & emoção : provocações a partir de Wolfsohn, Roy Hart e Pantheatre." reponame:Biblioteca Digital de Teses e Dissertações da UFRGS, 2010. http://hdl.handle.net/10183/26996.

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Esta dissertação se propõe a discutir princípios e identificar alguns procedimentos técnicos que provoquem a descoberta, particularmente por atores e bailarinos, de novos territórios de vocalidade, que contribuam para enriquecer a construção da poética cênica. Considerando a emoção como elemento fundamental na descoberta de possibilidades para a voz, o estudo parte das pesquisas pioneiras de Alfred Wolfsohn (1896-1962) e de seu aluno Roy Hart (1926-1975) para se concentrar nas práticas pedagógicas do Pantheatre, companhia fundada na França por Enrique Pardo junto a outros integrantes originais

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2

Colomb, Laurent. "Le Roy Hart Theatre : contribution à une étude pluridisciplinaire de la voix." Paris 8, 2000. http://www.theses.fr/2000PA081840.

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Le @Roy Hart Theatre entretient avec la voix une relation inattendue aux multiples incidences. Ses applications relèvent tout à la fois des domaines du chant, de la thérapie et du théâtre. Elles sont l'aboutissement d'une recherche méthodique et continuelle sur la voix qui couvre une période de près d'un siècle. Cette relation polyvalente à la voix a pour point de départ le traumatisme psychique dont fut victime Alfred Wolfsohn, brancardier sur les charniers de la guerre 14-18. Partant du pouvoir d'expression de la voix, il fixe les bases fondamentales d'une cure par le chant dont il évalue pe

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3

Chiochetta, Letícia. "A criação da cena teatral à luz de Alfred Wolfsohn e Roy Hart." Universidade de São Paulo, 2013. http://www.teses.usp.br/teses/disponiveis/27/27155/tde-28012014-115432/.

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Esta pesquisa teórico-prática realiza um estudo do pensamento e dos princípios de trabalho de dois importantes artistas e pesquisadores da voz ainda pouco conhecidos no universo das Artes Cênicas no Brasil: o alemão Alfred Wolfsohn e, seu discípulo, o ator Roy Hart. Wolfsohn desenvolveu, após uma experiência traumática de guerra, uma pesquisa aprofundada sobre a expressão humana através da voz. Já Hart aplicou, à sua maneira, os ensinamentos de Wolfsohn no campo teatral. Esta dissertação de mestrado efetiva ainda uma investigação prática à luz dos fundamentos propostos por esses artistas. Sua

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4

Meehan, Niall. "Tuning out the troubles in southern Ireland : revisionist history, censorship and problematic Protestants." Thesis, University of Bath, 2015. https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.683549.

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This thesis is an examination of the influence and impact of the ‘Troubles’ in Northern Ireland, post 1968, on the practice of Irish history, on southern Irish broadcast media and on the southern Irish modernisation process. I will examine the uneasy and contested transition in systems of hegemony in a society where the state is not coterminous with perceptions of nationhood, where society is anxiously suspended between conservation of its existence and popular nationalist aspirations, where southern economic dependency interacted uneasily with northern political instability and sectarianism.

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5

Olivares, del Real Paloma. "Hare api Hana Roa : Centro educativo Hanga Roa." Tesis, Universidad de Chile, 2012. http://repositorio.uchile.cl/handle/2250/111608.

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Memoria (arquitecto)<br>No autorizada por el autor para ser publicada a texto completo<br>La educación es esencial para generar una serie de cambios. En el caso de Isla de Pascua, además de potenciar directamente la cultura Rapanui, hay formas indirectas para poner en valor esta misma, ya que puede permitir la disminución de la dependencia del continente, teniendo personas calificadas en la isla para hacer las tareas de la isla, lo que significa importar menos mano de obra del continente por ejemplo, lo que permitiría un cierto grado de protección para la isla, puesto que hoy con la

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6

Kim, Victoria. "Hard X-ray test objects." Thesis, KTH, Tillämpad fysik, 2018. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-233228.

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7

Court, A. J. "Hard X-ray astronomy from balloon altitudes." Thesis, University of Southampton, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.377796.

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8

Spooner, Neil John Curwen. "New techniques in hard X-ray astronomy." Thesis, Imperial College London, 1986. http://hdl.handle.net/10044/1/38166.

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9

Lawson, Anthony J. "The hard X-ray emission of quasars." Thesis, University of Leicester, 1995. http://hdl.handle.net/2381/35714.

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The analysis of observations of 50 radio-loud and radio-quiet quasars made by the X-ray satellite Ginga is presented. The spectra, the most accurate and sensitive yet in the 2-20 keV band, provide a unique opportunity to study the hard X-ray emission from these faint, though highly luminous objects. The properties of the X-ray continuum are compatible with previous studies, and reveal a significant measured spread on the spectral index, which is unlikely to be due to spectral variability or to the radio heterogenity of the sample, indicating a true variety of spectral index amongst objects. Th

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10

Mullerworth, Stephen Derek. "Position sensitive detectors for hard X-ray and gamma-ray astronomy." Thesis, University of Southampton, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.386646.

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11

Pleasants, Ian Blair. "Detector elements for hard X-ray and gamma-ray astronomy applications." Thesis, University of Southampton, 1994. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.262152.

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12

Fraser-Mitchell, J. N. "An imaging detector for hard X-ray astronomy." Thesis, University of Southampton, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.383420.

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13

Parisi, Pietro <1982&gt. "Multiwavelength studies of hard X-ray selected sources." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3775/.

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14

Bale, Greg. "CdZnTe radiation detectors for hard X-ray astronomy." Thesis, University of Leicester, 2001. http://hdl.handle.net/2381/30645.

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This thesis is concerned with the development of CdZnTe compound semiconductor detectors for hard X-ray astronomy. The advent of multilayer coated focusing optics for hard X-rays creates the need for compact solid-state X-ray detectors with substantial quantum efficiency above 10 keV. CZT is a material with the necessary properties to meet the requirements. Excellent results from commercially obtained CdZnTe detectors are presented in Chapter 4 of this work. Low-noise preamplifiers and Peltier coolers were employed to obtain high-resolution X-ray and gamma-ray spectra over the 2 - 60 keV energ

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15

Hoffmann, Agnes Irene Dorothee. "Analysis of hard X-ray emission from selected very high energy g-ray." Reutlingen, Bruno-Matzke-Str.15 A. Hoffmann, 2009. http://d-nb.info/999640429/34.

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16

Nilsson, Daniel. "Zone Plates for Hard X-Ray Free-Electron Lasers." Doctoral thesis, KTH, Biomedicinsk fysik och röntgenfysik, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-122161.

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Hard x-ray free-electron lasers are novel sources of coherent x-rays with unprecedented brightness and very short pulses. The radiation from these sources enables a wide range of new experiments that were not possible with previous x-ray sources. Many of these experiments require the possibility to focus the intense x-ray beam onto small samples. This Thesis investigates the possibility to use diffractive zone plate optics to focus the radiation from hard x-ray free-electron lasers. The challenge for any optical element at free-electron laser sources is that the intensity in a single short pul

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17

Bain, Hazel Miller. "Hard X-ray and radio studies of solar flares." Thesis, University of Glasgow, 2010. http://theses.gla.ac.uk/1751/.

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Combined X-ray and radio observations of the Sun provide powerful diagnostics of particle acceleration and transport effects during solar flares. In this thesis we present observations of two solar flares. In the first event we report what we believe to be the first observation of hard X-ray emission formed in a coronal, flare-related jet. Occurring on the 22nd of August 2002, the event was observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI) and the Nobeyama Radioheliograph (NoRH) and Polarimeters (NoRP). During the impulsive phase RHESSI observed significant hard X-r

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18

Bird, Antony John. "A position-sensitive detector for hard X-ray astronomy." Thesis, University of Southampton, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.292524.

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19

Zhang, Shuang Nan. "Instrumentation and data analysis for hard X-ray astronomy." Thesis, University of Southampton, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.252689.

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20

Leddon, Deborah L. "A Statistical Study of Hard X-Ray Solar Flares." Thesis, University of North Texas, 2001. https://digital.library.unt.edu/ark:/67531/metadc3045/.

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The results of a statistical study of hard x-ray solar flares are presented in this dissertation. Two methods of analysis were used, the Diffusion Entropy (DE) method coupled with an analysis of the data distributions and the Rescaled Range (R/S) Method, sometimes referred to as "Hurst's method". Chapter one provides an introduction to hard x-ray flares within the context of the solar environment and a summary of the statistical paradigms solar astronomers currently work under. Chapter two presents the theory behind the DE and R/S methods. Chapter three presents the results of the two analysis

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21

Ahlberg, Erik, and Samin Hasan. "Optimising a small satellite for hard X-ray polarisation studies of gamma ray Bursts." Thesis, KTH, Fysik, 2014. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-149677.

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Gamma ray bursts (GRBs) originate from extremely energetic extra-galactic events, and much is still unknown about them. Whereas the energy and time structure of GRBs have been studied extensively the past years, only a few polarisation measurements have been made on their initial, prompt emission. Determining the polarisation of GRBs will therefore provide a means to test proposed emission models. A small satellite (SPHiNX) has been proposed to measure the polarisation of X-rays from GRBs. The performance of the detector is optimised using Monte Carlo simulations of a typical GRB source, in or

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22

Patommel, Jens. "Hard X-Ray Scanning Microscope Using Nanofocusing Parabolic Refractive Lenses." Doctoral thesis, Saechsische Landesbibliothek- Staats- und Universitaetsbibliothek Dresden, 2011. http://nbn-resolving.de/urn:nbn:de:bsz:14-qucosa-64982.

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Hard x rays come along with a variety of extraordinary properties which make them an excellent probe for investigation in science, technology and medicine. Their large attenuation length in matter opens up the possibility to use hard x-rays for non-destructive investigation of the inner structure of specimens. Medical radiography is one important example of exploiting this feature. Since their discovery by W. C. Röntgen in 1895, a large variety of x-ray analytical techniques have been developed and successfully applied, such as x-ray crystallography, reflectometry, fluorescence spectroscopy, x

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23

Uhlén, Fredrik. "Nanofabrication of Zone Plates for Hard X-Ray Free-Electron Lasers." Doctoral thesis, KTH, Biomedicinsk fysik och röntgenfysik, 2015. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-158121.

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This Thesis describes the development of hard X-ray zone plates intended for focusing radiation at X-ray free-electron lasers (XFELs). XFELs provide unprecedented brightness and zone plates which are put in the intense X-ray beam are at risk of being damaged. Therefore, it is crucial to perform damage tests in order to design zone plates which can survive the XFEL beam. Zone plates are diffractive nanofocusing optics and are regularly used at high brightness synchrotron beamlines in the soft and hard X-ray regime. The resolution of a zone plate is proportional to its outermost zonewidth and th

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24

Müller, Oliver [Verfasser]. "Hard X-ray Synchrotron Beamline Instrumentation for Millisecond Quick Extended X-ray Absorption Spectroscopy / Oliver Müller." Wuppertal : Universitätsbibliothek Wuppertal, 2016. http://d-nb.info/1120339022/34.

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25

Haydock, Esther. "Electron beam wave relaxation and solar flare hard X-ray emission." Thesis, University of Glasgow, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.269508.

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26

Mudie, Stephen. "Characterisation of Group III nitrides using hard X-ray synchrotron radiation." Monash University, School of Physics and Materials Engineering, 2004. http://arrow.monash.edu.au/hdl/1959.1/9729.

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27

Alexander, Robert Calum. "Influence of photospheric back-scatter on flare hard x-ray diagnostics." Thesis, University of Glasgow, 2010. http://theses.gla.ac.uk/1707/.

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In this thesis I present the results of studies on the influence of solar photospheric back–scatter on Hard X–Ray (HXR) flare diagnostics. Specifically the thesis presented is concerned with the effect of back–scatter photons upon the morphology of the Hard X–Ray photon spectrum and its effect on the inferred parent electron spectrum. I present a theoretical investigation into Compton reflected HXR photons, known as the photospheric Albedo, and explore the effect of photospheric albedo on observations of global flare hard X-ray spectra for isotropic emission. I examine, for the Kramers cross-s

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28

Kole, Merlin. "Background Studies for the Balloon-Borne Hard X-ray Polarimeter PoGOLite." Doctoral thesis, KTH, Partikel- och astropartikelfysik, 2014. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-155754.

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The polarisation degree and angle of the X-ray flux emitted by astrophysical objects holds valuable information on the responsible emission mechanisms and on the emission environments. PoGOLite is a balloon-borne hard X-ray polarimeter designed to measure polarisation using a segmented plastic scintillator array. The instrument was launched for its first scientific, near-circumpolar, flight in July 2013 from the Esrange Space Centre in Northern Sweden. The primary observation target for this flight, the Crab, was observed during the first 2 days of flight. One of the main challenges for PoGOLi

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29

Grätz, Matthias. "Characterisation and application of a laser-based hard X-ray source." Lund : Lund Institute of Technology, 1998. http://catalog.hathitrust.org/api/volumes/oclc/68945036.html.

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30

Ivan, Adrian 1964. "Fabrication and characterization of multilayers for focusing hard x-ray optics." Thesis, Massachusetts Institute of Technology, 2002. http://hdl.handle.net/1721.1/30006.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Nuclear Engineering, 2002.<br>Includes bibliographical references.<br>This study investigated the growth of multilayers with depth-graded thicknesses and their performance as x- ray mirrors for the next generation of focusing telescopes. Different material combinations were studied for the first time employing a consistent methodology for the DC magnetron sputtering growth of the multilayers and their characterization by x-ray reflectivity (XRR) measurements. The width of the interfaces was identified as the most important factor

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31

Zborowski, Charlotte. "Characterization of deeply buried interfaces by Hard X-ray Photoelectron Spectroscopy." Thesis, Lyon, 2018. http://www.theses.fr/2018LYSEC025/document.

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Cette thèse vise à améliorer la méthode d'analyse du fond continu inélastique afin de l'appliquer à des cas qui présentent un intérêt technologique. En effet, ces améliorations sont cruciales car elles portent sur des critères de précision et de gain de temps, plus particulièrement pour l’étude de dispositifs présentant plusieurs couches profondément enterrées de matériaux bien distincts. Ainsi, l'analyse du fond continu inélastique associée à la spectroscopie de photoélectrons à rayons X durs (HAXPES) présente un grand intérêt car l’HAXPES permet de sonder plus profondément dans un échantillo

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32

Fioretti, Valentina <1982&gt. "Background minimization issues for next generation hard X-ray focusing telescopes." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3858/.

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The hard X-ray band (10 - 100 keV) has been only observed so far by collimated and coded aperture mask instruments, with a sensitivity and an angular resolution lower than two orders of magnitude as respects the current X-ray focusing telescopes operating below 10 - 15 keV. The technological advance in X-ray mirrors and detection systems is now able to extend the X-ray focusing technique to the hard X-ray domain, filling the gap in terms of observational performances and providing a totally new deep view on some of the most energetic phenomena of the Universe. In order to reach a sensitivity

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33

Langer, Max. "Phase retrieval in the Fresnel region for hard X-ray tomography." Lyon, INSA, 2008. http://theses.insa-lyon.fr/publication/2008ISAL0094/these.pdf.

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The aim of this work was to extend the validity of phase retrieval from Fresnel diffraction patterns to strongly absorbing objects. To this effect, new linear contrast model is presented. It is valid for slowly varying objects and unifies the transport of intensity equation and contrast transfer function in that it approaches each in the limit of small propagation distance and weak absorption respectively. We go on to notice that, due to how the phase information is propagated to the recorded images, the phase retrieval is sensitive to noise in the low-frequency range and is actually singular

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34

Cederström, Björn. "A multi-prism lens for hard X-Rays." Doctoral thesis, KTH, Fysik, 2002. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3423.

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This thesis describes a new type of refractive lens for hardx-rays. It is shown that a linear array of prisms, slightlyinclined with respect to the optical axis, will form a linefocus at a certain distance from the lens. Hence, the namemulti-prism lens. These lenses are free from sphericalaberration and are similar to planar parabolic compoundrefractive lenses in terms of performance. However, theydistinguish themselves in that only planar surfaces need to befabricated. A special feature is that the focal length can beeasily varied by adjusting the inclination angle. Theoretical calculations,

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35

Damauskaitė, Jovita. "Research And Application Of Hard Cosmic Ray Flux For Forecasting Meteorological Conditions." Doctoral thesis, Lithuanian Academic Libraries Network (LABT), 2010. http://vddb.laba.lt/obj/LT-eLABa-0001:E.02~2010~D_20101222_130615-72153.

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The thesis investigates cosmic rays and their scattering in the atmosphere and the change in their intensity caused by the frequency of meteorological phenomenon. The main objective of the research is the change in cosmic rays as well as atmospheric pressure and estimation of their connection. A thorough analysis and interpretation allow to supplement meteorological information for weather forecasts.<br>Disertacijoje nagrinėjama kosminė spinduliuotė ir jos sklaida atmosferoje bei jos intensyvumo kaita, kurią lemią meteorologinių reiškinių dažnumas. Pagrindinis tyrimo objektas yra kietosios kos

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36

Lyu, Chunhai [Verfasser], and Christoph H. [Akademischer Betreuer] Keitel. "Narrow-band hard-x-ray lasing / Chunhai Lyu ; Betreuer: Christoph H. Keitel." Heidelberg : Universitätsbibliothek Heidelberg, 2018. http://d-nb.info/1177252597/34.

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37

Lingham, Manohar. "Plasma-assisted sputter deposition of multilayer mirrors for hard X-ray synchrotron." Thesis, University of London, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.298365.

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Chakrabarty, Deepto Prince Thomas A. Prince Thomas A. "Hard X-ray detection and timing of accretion-powered pulsars with BATSE /." Diss., Pasadena, Calif. : California Institute of Technology, 1996. http://resolver.caltech.edu/CaltechETD:etd-09022008-132322.

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39

Carstairs, Ian Ruthven. "Kernel density estimators applied to hard X-ray observations of the Crab Pulsar." Thesis, University of Southampton, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.315292.

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40

Brocksopp, Catherine. "Multiwavelength variability of black hole x-ray binaries in the low/hard state." Thesis, [n.p.], 2000. http://oro.open.ac.uk/19112/.

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41

Stampanoni, Marco. "A novel approach towards hard X-ray submicrometer computer tomography with synchrotron radiation." [S.l. : s.n.], 2002. http://e-collection.ethbib.ethz.ch/ecol-pool/diss/fulltext/eth14884.pdf.

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Chen, Chi Ming Hubert Harrison Fiona A. "Development of hard X-ray imaging detectors for the High Energy Focusing Telescope /." Diss., Pasadena, Calif. : California Institute of Technology, 2008. http://resolver.caltech.edu/CaltechETD:etd-04202008-135222.

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43

Scaringi, Simone. "Machine learning from hard X-ray surveys : applications to magnetic cataclysmic variable studies." Thesis, University of Southampton, 2009. https://eprints.soton.ac.uk/161197/.

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Within this thesis are discussed two main topics of contemporary astrophysics. The first is that of machine learning algorithms for astronomy whilst the second is that of magnetic cataclysmic variables (mCVs). To begin, an overview is given of ISINA: INTEGRAL Scouce Identifiction Network Algorithm. This machine learning algorithm, using random forests, is applied to the IBIS/ISGRI data set in order to ease the production of unbiased future soft gamma-ray source catalogues. The feature extraction process on an initial candidate list is described together with feature merging. Three trainng and

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44

Tsuboi, Yoko. "Hard X-ray Probing of Dark Clouds : Protostar Structure and the Magnetic Activities." 京都大学 (Kyoto University), 1999. http://hdl.handle.net/2433/181945.

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45

Almqvist, Heléne. "Studies on root hard-tissue demineralization and remineralization measured by ¹²⁵I absorptiometry." Stockholm : Karolinska Institutet, 1993. http://catalog.hathitrust.org/api/volumes/oclc/29572338.html.

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46

Jeanjean, Sébastien. "Vers l' optimisation du rayonnement d' un haut-parleur dans un habitacle automobile : résolution des problèmes de modélisation." Paris 6, 2005. http://www.theses.fr/2005PA066314.

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47

Baumgartner, Wayne. "Elemental abundances via X-ray observations of galaxy clusters and the InFOC[mu]S [i.e. InFOCuS] hard X-ray telescope." College Park, Md. : University of Maryland, 2004. http://hdl.handle.net/1903/1387.

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Thesis (Ph. D.) -- University of Maryland, College Park, 2004.<br>InFOCuS on t.p. of PDF has the Greek letter for MU instead of u. Thesis research directed by: Astronomy. InFOCuS in PDF has the Greek letter for mu instead of u. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.

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48

Hoffmann, Agnes Irene Dorothee [Verfasser]. "Analysis of hard X-ray emission from selected very high energy γ-ray [gamma-ray] sources observed with INTEGRAL / vorgelegt von Agnes Irene Dorothee Hoffmann". Reutlingen, Bruno-Matzke-Str.15 : A. Hoffmann, 2009. http://d-nb.info/999640429/34.

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49

Geck, Jochen. "Spins, charges, and orbitals in perovskite manganites : resonant and hard x-ray scattering studies /." Berlin : Mensch & Buch Verl, 2004. http://www.loc.gov/catdir/toc/fy0804/2007464041.html.

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Ion, Valentina. "Nonlinear approaches for phase retrieval in the Fresnel region for hard X-ray imaging." Phd thesis, INSA de Lyon, 2013. http://tel.archives-ouvertes.fr/tel-01015814.

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The development of highly coherent X-ray sources offers new possibilities to image biological structures at different scales exploiting the refraction of X-rays. The coherence properties of the third-generation synchrotron radiation sources enables efficient implementations of phase contrast techniques. One of the first measurements of the intensity variations due to phase contrast has been reported in 1995 at the European Synchrotron Radiation Facility (ESRF). Phase imaging coupled to tomography acquisition allows threedimensional imaging with an increased sensitivity compared to absorption C

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