Дисертації з теми "Observational signatures"
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Sming, Yue-Lin Sming. "Observational signatures of supersymmetric dark matter." Thesis, University of Sheffield, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.544174.
Повний текст джерелаSarkar, Tamal. "Search for some observational signatures of general relativity." Thesis, University of North Bengal, 2017. http://hdl.handle.net/123456789/2643.
Повний текст джерелаHamilton, Devon. "Observational signatures of convection in solar type stars." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 2001. http://www.collectionscanada.ca/obj/s4/f2/dsk3/ftp04/NQ58914.pdf.
Повний текст джерелаHarding, Paul. "The formation of the Galactic bulge and halo: Observational signatures." Diss., The University of Arizona, 2001. http://hdl.handle.net/10150/289743.
Повний текст джерелаBending, Victoria Louise. "Extra-solar planetary atmospheres and interior structure : implications for observational signatures." Thesis, Open University, 2016. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.701075.
Повний текст джерелаPatrick, Antolin Tobos. "Predicting observational signatures of coronal heating by Alfven waves and nanoflares." 京都大学 (Kyoto University), 2009. http://hdl.handle.net/2433/126571.
Повний текст джерела0048
新制・課程博士
博士(理学)
甲第14894号
理博第3463号
新制||理||1507(附属図書館)
27332
UT51-2009-M808
京都大学大学院理学研究科物理学・宇宙物理学専攻
(主査)教授 柴田 一成, 教授 一本 潔, 教授 嶺重 慎
学位規則第4条第1項該当
Jürgens, Gero [Verfasser], and Matthias [Akademischer Betreuer] Bartelmann. "Evolution and observational signatures of cosmic structures / Gero Jürgens ; Betreuer: Matthias Bartelmann." Heidelberg : Universitätsbibliothek Heidelberg, 2013. http://d-nb.info/1177148463/34.
Повний текст джерелаOgawa, Takumi. "Observational Signatures of Super-Eddington Accretors:Views from Radiation Hydrodynamics/Radiation Transfer Simulations." Doctoral thesis, Kyoto University, 2021. http://hdl.handle.net/2433/263470.
Повний текст джерелаHall, Cassandra. "Using numerical simulations to identify observational signatures of self-gravitating protostellar discs." Thesis, University of Edinburgh, 2017. http://hdl.handle.net/1842/29585.
Повний текст джерелаZach, Juergen Johann. "Observational Signatures of the Macroscopic Formation of Strange Matter during Core Collapse Supernovae." The Ohio State University, 2003. http://rave.ohiolink.edu/etdc/view?acc_num=osu1053470113.
Повний текст джерелаWinner, Georg Eckhard Verfasser], and Christoph [Akademischer Betreuer] [Pfrommer. "On the Evolution and Observational Signatures of Cosmic Ray Electrons in Magnetohydrodynamical Simulations / Georg Eckhard Winner ; Betreuer: Christoph Pfrommer." Heidelberg : Universitätsbibliothek Heidelberg, 2020. http://nbn-resolving.de/urn:nbn:de:bsz:16-heidok-289531.
Повний текст джерелаWinner, Georg Eckhard [Verfasser], and Christoph [Akademischer Betreuer] Pfrommer. "On the Evolution and Observational Signatures of Cosmic Ray Electrons in Magnetohydrodynamical Simulations / Georg Eckhard Winner ; Betreuer: Christoph Pfrommer." Heidelberg : Universitätsbibliothek Heidelberg, 2020. http://d-nb.info/1220836303/34.
Повний текст джерелаJohnston, Katharine G. "Observational signatures of massive star formation : an investigation of the environments in which they form, and the applicability of the paradigm of low-mass star formation." Thesis, University of St Andrews, 2011. http://hdl.handle.net/10023/1895.
Повний текст джерелаEtienne, Christian. "Réalisation et évaluation d'un sodar monostatique : étude des signatures sodars en fonction de paramètres météorologiques." Orléans, 1986. http://www.theses.fr/1986ORLE0404.
Повний текст джерелаTrottier, Eric. "Recherche de signatures spectrales d’objets astronomiques variant ultra rapidement dans les relevés spectroscopiques." Thesis, Université Laval, 2013. http://www.theses.ulaval.ca/2013/29658/29658.pdf.
Повний текст джерелаMeng, Huan Y. A., George H. Rieke, Kate Y. L. Su, and András Gáspár. "The First 40 Million Years of Circumstellar Disk Evolution: The Signature of Terrestrial Planet Formation." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/623246.
Повний текст джерелаAlkahtani, Abdulaziz M. A. l.-Musa. "Free hand simulation of Arabic signatures : Forensic examination and statistical observations." Thesis, Staffordshire University, 2010. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.522387.
Повний текст джерелаMatthews, Sarah H. "Thermal and nonthermal radiation signatures in solar flares : models and observations." Thesis, University of Glasgow, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.309388.
Повний текст джерелаGaspar, Andras. "Observations and Models of Infrared Debris Disk Signatures and their Evolution." Diss., The University of Arizona, 2011. http://hdl.handle.net/10150/202982.
Повний текст джерелаVontrat-Reberac, Aurélie Karine. "Etude des cornets polaires : observations in-situ à haute altitude et modélisation et observations des signatures ionosphériques." Versailles-St Quentin en Yvelines, 2003. http://www.theses.fr/2003VERS0023.
Повний текст джерелаNear the magnetic poles, the magnetic field lines converge and form funnels called polar cusps. These very localized regions are very sensitive to interplanetary conditions. With its four satellites in, the CLUSTER mission allows for the first time the study of the tri-dimensional structure of boundary regions and the separation of spatial and temporal effects. We have exploited this capability to analyse the space and time dynamics of particle structures observed in the high-altitude polar cusp during events of reconnection between the terrestrial and interplanetary magnetic fields. Ionospheric observations at the footprint of polar cusps by the radar ESR show that polar cusp particles collide with the ionosphere and create ionization, heating. We have interpreted these observations from the modeling of their immediate and long-term effects on the ionospheric parameters
Occhipinti, Giovanni. "Observations multi-paramètres et modélisation de la signature ionosphérique du grand séisme de Sumatra." Paris, Institut de physique du globe, 2006. http://www.theses.fr/2006GLOB0012.
Повний текст джерелаBoudin, Nathalie. "Recherche de signatures spectrales de cations aromatiques dans l'absorption diffuse interstellaire : confrontation spectroscopie de laboratoire, observations astronomiques." Paris 11, 2001. http://www.theses.fr/2001PA112348.
Повний текст джерелаPolycyclic Aromatic Hydrocarbons (PAHs) are now recognized as an important constituent of the interstellar medium gaseous phase. This family of molecules and in particular their ionic derivatives seems to be one of the most promising candidates for identification of the Diffuse Interstellar Bands (DIBs). These absorption bands are observed in the visible spectral range in the spectra of stars partially masked by gas cloud. The possible identification of PAHs as molecules responsible for these bands must be done through direct comparison with PAHs spectra recorded in conditions as close as possible to those of the interstellar medium. These low temperature and collision-free conditions can be recreated in the laboratory with supersonic beams. A van der Waals complex PAH-Ar is then ionized by resonant two-photon ionization. The ion absorption of a tunable visible laser photon causes the argon departure, and the detection of this dissociation by a mass spectrometer allows the recording of the PAH cation spectrum. Using this technique, the spectra of phenylacetylene(+)-Ar and of acenaphthene(+)-Ar could be obtained. The spectral profile is wide and lorentzian, showing an intramolecular dynamics dominated by ultrafast internal conversion. Two observation campaigns with the Télescope Bernard Lyot at the Pic du Midi allowed us to perform a systematic search for this broad bands, thanks to specific observational protocole and data processing. Upper-limits of abundance were determined for five PAH cations. Interstellar absorption zones identified in our spectra are of variable width and some of them are very likely the result of a combination due to several species. According to our measurements between 525 and 840 nm, the diffuse interstellar absorption represents 87 % of the interstellar absorption in front of BD +404220 star
Bernard, Jérémy. "Signature géographique et météorologique des variations spatiales et temporelles de la température de l'air au sein d'une zone urbaine." Thesis, Ecole centrale de Nantes, 2017. http://www.theses.fr/2017ECDN0006.
Повний текст джерелаThis thesis presents a method to model air temperature differences within a conurbation . It relies on the analysis of the existing relationships between urban microclimate,geographical context and weather conditions. To do so, five air temperature networks located in three western France conurbations are utilized : Nantes, Angers and La Roche sur-Yon. A state of the art of the methods used to analyze urban climate is realized in chapter 1. In Chapter 2, air temperature networks are presented and analyzed and a methodology to correct biased data is proposed. In Chapter3 air temperature differences observed between the network sites are modelled from multiple linear regressions, using weather variables such as wind speed or solar radiation as explicative variables. Before the calibration step, data is sorted in a variety of ways in order to elaborate several models. The most performant model is identified in chapter4, confronting data observed using the five temperature networks to data estimated from each of the models.Chapter 5 illustrates the results of the work through three practical applications
Deligny, Olivier. "Observatoire Pierre Auger : analyse des gerbes inclinées, Observation de neutrinos d'ultra haute énergie, et signatures d'une origine locale pour les rayons cosmiques chargés." Paris 6, 2003. https://tel.archives-ouvertes.fr/tel-00002995.
Повний текст джерелаWilson, Belinda R. "The Forgotten Signature: An Observational Study on Policy of Securing Identity in Prevention of Identity Theft and Credit/Debit Card Fraud at Retail Store POS Terminals." Digital Commons @ East Tennessee State University, 2016. https://dc.etsu.edu/etd/3074.
Повний текст джерелаDeligny, Olivier. "Observatoire Pierre Auger : Analyse des gerbes inclinées, observation de neutrinos d'ultra haute énergie, et signature d'une origine locale pour les rayons cosmiques chargés." Phd thesis, Université Pierre et Marie Curie - Paris VI, 2003. http://tel.archives-ouvertes.fr/tel-00002995.
Повний текст джерелаAprès avoir étudié l'effet des champs magnétiques extragalactiques sur la propagation des rayons cosmiques et l'influence sur le spectre, une grande partie du chapitre consacré à la description de l'expérience Auger sera laissée au système d'acquisition des données.
L'étude des gerbes atmosphériques initiées dans la haute atmosphère sous incidence rasante est riche d'enseignements concernant la possibilité de détection de neutrinos. Une procédure de reconstruction de l'énergie des gerbes rasantes hadroniques est formalisée et appliquée aux événements du prototype dans le chapitre 4, et le calcul de la sensibilité aux neutrinos du détecteur complet est donné dans le chapitre 5.
Enfin, l'analyse des données de l'année 2002 du réseau prototype de l'expérience Auger est l'objet du chapitre 6.
Quentin, Céline. "Etude de la surface océanique, de la signature radar et de ses interactions avec les flux turbulents de quantité de mouvement dans le cadre de l'expérience FETCH." Paris 6, 2002. https://tel.archives-ouvertes.fr/tel-00010934.
Повний текст джерелаQUENTIN, Céline Gwenaëlle. "Etude de la surface océanique, de sa signature radar et de ses interactions avec les flux turbulents de quantité de mouvement dans le cadre de l'experience FETCH." Phd thesis, Université Pierre et Marie Curie - Paris VI, 2002. http://tel.archives-ouvertes.fr/tel-00010934.
Повний текст джерелаRiccio, Giuseppe. "The Observational Signatures of Cosmic Strings." Tesi di dottorato, 2009. http://www.fedoa.unina.it/3790/1/riccio.pdf.
Повний текст джерелаFernandez, Elizabeth Rose. "Observational signatures of the first stars : from the near infrared background to Lyman-[alpha] emitters." 2008. http://hdl.handle.net/2152/17868.
Повний текст джерелаBogdanovic, Tamara. "Close encounters of black holes, stars, and gas in galactic nucle a study of the observational signatures /." 2006. http://etda.libraries.psu.edu/theses/approved/WorldWideIndex/ETD-1537/index.html.
Повний текст джерелаChe-WeiChang and 張哲維. "Observation of Kondo Signatures in Spin-Orbit Coupled Quantum Wires." Thesis, 2016. http://ndltd.ncl.edu.tw/handle/13338835550030194844.
Повний текст джерелаLaw, Colin Christian. "Observations of magnetic signatures and structure in the dayside ionosphere of Venus." Thesis, 1993. http://hdl.handle.net/1911/13753.
Повний текст джерелаCorlies, Lauren Nicole. "Observationally Constrained Metal Signatures of Galaxy Evolution in the Stars and Gas of Cosmological Simulations." Thesis, 2016. https://doi.org/10.7916/D8FF3SJC.
Повний текст джерелаLiu, Chih-Yuan, and 劉志原. "SEARCH FOR SIGNATURE OF WAVES ON THE SURFACE OF NEUTRON STARS - LONG-TERM X-RAY OBSERVATIONS OF PSR B1509-58." Thesis, 2003. http://ndltd.ncl.edu.tw/handle/07743504838549394738.
Повний текст джерела國立清華大學
天文研究所
91
The stable pulsar PSR B1509-58 has been monitored with the Rossi X-ray Timing Explorer (RXTE) for seven years, since the start of that mission in January 1996. The long-term observation has enabled us to determine the first and the se cond period derivatives which can help us to search for other possible periodicities with data over a long time span. These possible periods may reveal properties of MHD waves on the surface of neutron stars, and thus promote our understand ing of neutron star physics. As the first of such attempts, we applied the H-test to RXTE/PCA data of PSR B1509-58 spanning from 1996 to 2002, consisting of more than 3*10^7 photon events, to search for periods other than the spin period. A search in the period range of 0~0.3 sec with 1-msec steps was conducted. No other periods were found. Some suspicious signatures, however, deserve further investigation. Moreover, the search sampling rate (1 msec per step) is too loose. A study with a higher sampling rate and a wider search range, which requires more computing time, is in preparation.