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Tesis sobre el tema "Cosmic rays Measurement"

Autor: Grafiati

Publicado: 4 de junio de 2021

Última modificación: 19 de febrero de 2022

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1

Brobeck, Elina Stone Edward McKeown R. D. "Measurement of ultra-high energy cosmic rays with CHICOS /." Diss., Pasadena, Calif. : California Institute of Technology, 2009. http://resolver.caltech.edu/CaltechETD:etd-10192008-143041.

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2

Moats, Anne Rosalie Myers. "LEAP: A balloon-borne search for low energy cosmic ray antiprotons." Diss., The University of Arizona, 1989. http://hdl.handle.net/10150/184723.

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The LEAP (Low-Energy Antiproton) experiment is a search for cosmic-ray antiprotons in the 120 MeV to 1.2 GeV kinetic energy range. The motivation for this project was the result announced by Buffington et al. (1981) that indicated an anomalously high antiproton flux below 300 MeV; this result has compelled theorists to propose sources of primary antiprotons above the small secondary antiproton flux produced by high energy cosmic-ray collisions with nuclei in the interstellar medium. LEAP consisted of the NMSU magnet spectrometer, a time-of-flight system designed at Goddard Space Flight Center,

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3

吳本韓 and Pun-hon Ng. "Measurement of PeV cosmic rays extensive air showers at mountain altitude." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1993. http://hub.hku.hk/bib/B31233156.

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4

Ng, Pun-hon. "Measurement of PeV cosmic rays extensive air showers at mountain altitude /." [Hong Kong : University of Hong Kong], 1993. http://sunzi.lib.hku.hk/hkuto/record.jsp?B13781431.

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5

Behlmann, Matthew Daniel. "Measurement of helium isotopic composition in cosmic rays with AMS-02." Thesis, Massachusetts Institute of Technology, 2018. http://hdl.handle.net/1721.1/115695.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2018.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 137-145).<br>The isotopic composition of helium in cosmic ray fluxes provides valuable information about cosmic ray propagation through the Galaxy, which is of particular interest to indirect dark matter searches. Helium-3, mainly a secondary cosmic ray species, is primarily produced by spallation of heavier cosmic rays, such as primary helium-4, with interstellar matter. In six years of data taking, AMS has collected the lar

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6

Fleischhack, Henrike. "Measurement of the iron spectrum in cosmic rays with the VERITAS experiment." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät, 2017. http://dx.doi.org/10.18452/17691.

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Das Energiespektrum der kosmischen Strahlung bietet wichtige Hinweise auf ihren Ursprung und ihre Ausbreitung. Verschiedene Messtechniken müssen kombiniert werden, um den ganzen Energiebereich abdecken zu können: Direkte Messungen mit Teilchendetektoren bei niedrigen Energien sowie indirekte Messungen von Luftschauern bei hohen Energien. Dazu kommt die Messung von Photonen, hauptsächlich im GeV- und TeV-Bereich, die bei der Wechselwirkung von kosmischer Strahlung mit Materie oder elektromagnetischen Feldern entstehen. Im Folgenden werde ich zwei Studien dazu vorstellen, die beide auf Daten des

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7

Vasilas, Dragoş. "Measurement of light isotopes ratios in the cosmic rays with the IMAX balloon experiment." [S.l. : s.n.], 2004. http://deposit.ddb.de/cgi-bin/dokserv?idn=972319077.

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8

Sun, Wei Ph D. Massachusetts Institute of Technology. "Precision measurement of the boron to carbon ratio in cosmic rays with AMS-02." Thesis, Massachusetts Institute of Technology, 2015. http://hdl.handle.net/1721.1/99244.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2015.<br>This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.<br>Cataloged from student-submitted PDF version of thesis.<br>Includes bibliographical references (pages 163-170).<br>A precision measurement of the Boron to Carbon ratio in cosmic rays is carried out in the range 1 GeV/n to 670 GeV/n using the first 30 months of flight data of AMS-02 located on the International Space Station. Above 20 GeV/n, it is the first accu

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9

Jia, Yi Ph D. Massachusetts Institute of Technology. "Measurement of secondary cosmic rays lithium, beryllium, and boron by the alpha magnetic spectrometer." Thesis, Massachusetts Institute of Technology, 2018. http://hdl.handle.net/1721.1/119902.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2018.<br>This electronic version was submitted by the student author. The certified thesis is available in the Institute Archives and Special Collections.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 113-122).<br>Secondary cosmic rays are mainly produced by the collisions of nuclei with the interstellar medium. The precise knowledge of secondary cosmic rays is important to understand the origin and propagation of cosmic rays in the Galaxy. In this thesis, my work on the prec

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10

Tao, Li. "Measurement of the cosmic lepton and electron fluxes with the AMS detector on board of the International Space Station. Monitoring of the energy measurement in the calorimeter." Thesis, Université Grenoble Alpes (ComUE), 2015. http://www.theses.fr/2015GRENY016/document.

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Le Spectromètre Magnétique Alpha (AMS) est un détecteur de particules installé à bord de la Station Spatiale Internationale ; il enregistre des données depuis mai 2011. L'expérience a pour objectif d'identifier la nature des rayons cosmiques chargés et des photons et de mesurer leur flux dans la gamme d'énergie du GeV au TeV. Ces mesures permettent d'affiner les modèles de propagation de rayons cosmiques, d'effectuer une recherche indirecte de matière noire, et de chercher l'antimatière primordiale (anti-hélium). Dans ce mémoire, les données des premières années ont été utilisées pour mesurer

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11

Weber, Niclas. "A measurement of the antiproton and proton fluxes in cosmic rays using the CAPRICE experiment." Doctoral thesis, KTH, Physics, 1997. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2469.

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12

Chen, Hai Ph D. Massachusetts Institute of Technology. "Precision measurement of electron and positron flux in cosmic rays with the AMS-02 Detector." Thesis, Massachusetts Institute of Technology, 2016. http://hdl.handle.net/1721.1/103243.

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Thesis: Ph. D., Massachusetts Institute of Technology, Department of Physics, 2016.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (pages 159-169).<br>The cosmic ray electron and positron flux measurement can address a series of astrophysics and particle physics questions. This thesis presents an analysis of electron and positron flux from 0.5 GeV to 1 TeV using the first 30 months of data taking( over 41 billion events), with the AMS-02 detector on the International Space Station(ISS) 330-410 km above earth. A precise calibration of the Electromagnetic Calorim

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13

Kislat, Fabian. "Measurement of the energy spectrum of cosmic rays with the 26 station configuration of the IceTop detector." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2012. http://dx.doi.org/10.18452/16443.

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IceTop ist ein Luftschauerdetektor am geographischen Südpol und die Oberflächenkomponente des Neutrinoteleskops IceCube. Seit der Fertigstellung im Dezember 2010 besteht IceTop aus 81 Detektorstationen auf einer Fläche von einem Quadratkilometer. Die vorliegende Dissertation umfasst eine Analyse von Daten, die im Jahr 2007 mit den 26 damals installierten Stationen genommen wurden. Dazu wurden zunächst Schauerposition und -richtung und ein Maß für die Größe des Schauers aus den Signalen rekonstruiert. Der Zusammenhang zwischen Primärenergie und Schauergröße wurde aus Monte-Carlo-Simulationen

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14

Schulz, Alexander [Verfasser], and J. [Akademischer Betreuer] Blümer. "Measurement of the Energy Spectrum and Mass Composition of Ultra-high Energy Cosmic Rays / Alexander Schulz. Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2016. http://d-nb.info/1095665456/34.

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15

Schüssler, Fabian. "Measurement of the Energy Spectrum of Ultra-High Energy Cosmic Rays using Hybrid Data of the Pierre Auger Observatory." [S.l. : s.n.], 2008. http://digbib.ubka.uni-karlsruhe.de/volltexte/1000009955.

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16

Schüssler, Fabian. "Measurement of the energy spectrum of ultra-high energy cosmic rays using hybrid data of the Pierre Auger Observatory." Karlsruhe Forschungszentrum Karlsruhe, 2009. http://d-nb.info/995867089/34.

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17

Weidenhaupt, Klaus Frank [Verfasser]. "Antenna calibration and energy measurement of ultra-high energy cosmic rays with the Auger Engineering Radio Array / Klaus Frank Weidenhaupt." Aachen : Hochschulbibliothek der Rheinisch-Westfälischen Technischen Hochschule Aachen, 2014. http://d-nb.info/1065959966/34.

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18

Kühl, Patrick [Verfasser]. "Energy Spectra of near relativistic Galactic Cosmic Rays and Solar Energetic Particles - Extending the Measurement Capabilities of EPHIN / Patrick Kühl." Kiel : Universitätsbibliothek Kiel, 2017. http://d-nb.info/1141176114/34.

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19

Schüssler, Fabian [Verfasser]. "Measurement of the energy spectrum of ultra-high energy cosmic rays using hybrid data of the Pierre Auger Observatory / Fabian Schüssler." Karlsruhe : Forschungszentrum Karlsruhe, 2009. http://d-nb.info/995867089/34.

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20

Fleischhack, Henrike [Verfasser], Gernot [Gutachter] Maier, Thomas [Gutachter] Lohse, and Markus [Gutachter] Risse. "Measurement of the iron spectrum in cosmic rays with the VERITAS experiment / Henrike Fleischhack ; Gutachter: Gernot Maier, Thomas Lohse, Markus Risse." Berlin : Mathematisch-Naturwissenschaftliche Fakultät, 2017. http://d-nb.info/1125549734/34.

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21

Hugo, Marcelo Rivera Bretel. "Measurement of the energy spectrum of cosmic rays above 3 x 10¹⁷ eV using the infill array of the Pierre Auger Observatory." Paris 7, 2013. http://www.theses.fr/2013PA077028.

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L'observatoire Pierre Auger, situé en Argentine, combine un réseau de surface, étendu sur 3000 km ^2 et composé de détecteurs Cherenkov, avec 4 télescopes de fluorescence pour mesurer des gerbes atmosphériques initiées par les rayons cosmiques d'ultra haute énergie. Cet observatoire "hybride" (en fonctionnement depuis 2004, et dont le déploiement a été achevé en 2008) est pleinement efficace pour des énergies de rayons cosmiques primaires supérieures à 10 ^18 eV, c'est-à-dire à partir de la cheville du spectre en énergie jusqu'aux plus hautes énergies. Après l'achèvement de l'observatoire prin

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22

Getley, Ian L. Department of Aviation Faculty of Science UNSW. "Cosmic and solar radiation monitoring of Australian commercial flight crew at high southern latitudes as measured and compared to predictive computer modelling." Awarded by:University of New South Wales, 2007. http://handle.unsw.edu.au/1959.4/40536.

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This study set out to examine the levels of galactic cosmic radiation exposure to Australian aircrew during routine flight operations, with particular attention to the high southern latitude flights between Australia and South Africa. Latitudes as high as 65?? South were flown to gain the data and are typical of the normal flight routes flown between Sydney and Johannesburg on a daily basis. In achieving this objective it became evident that suitable commercially available radiation monitoring equipment was not readily available and scientific radiation monitors were sourced from overseas res

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23

Göttfert, Tobias. "Background suppression for a top quark mass measurement in the lepton+jets tt decay channel and alignment of the ATLAS silicon detectors with cosmic rays." kostenfrei, 2010. https://mediatum2.ub.tum.de/node?id=956486.

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24

Plum, Matthias [Verfasser], Thomas Akademischer Betreuer] Hebbeker, and Christopher Henrik V. [Akademischer Betreuer] [Wiebusch. "Measurement of the chemical composition of ultra high energy cosmic rays with the HEAT telescopes of the Pierre Auger Observatory / Matthias Plum ; Thomas Hebbeker, Christopher Wiebusch." Aachen : Universitätsbibliothek der RWTH Aachen, 2016. http://d-nb.info/1156922151/34.

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25

Klepser, Stefan. "Reconstruction of extensive air showers and measurement of the cosmic ray energy spectrum in the range of 1 - 80 PeV at the South Pole." Doctoral thesis, Humboldt-Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2008. http://dx.doi.org/10.18452/15790.

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IceTop ist ein Detektorfeld fuer kosmische Strahlung, das momentan am Suedpol errichtet wird. Es ist Teil des IceCube-Observatoriums und wird nach Fertigstellung eine Flaeche von 1km^2 ueberspannen. Es zielt auf den Nachweis von Teilchenkaskaden ab, die von kosmischer Strahlung mit Energien im PeV-Bereich induziert werden. Die Dissertation beinhaltet die erste Analyse hochenergetischer kosmischer Strahlung mit IceTop. Zunaechst wird hierfuer die Lichtausbeute der Detektortanks untersucht. Dies ermoeglicht die Erstellung einer Erwartungswertverteilung der Schauersignale, und eines

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26

Porcelli, Alessio [Verfasser], and J. [Akademischer Betreuer] Blümer. "Measurement of the Depth of Shower Maximum in the Transition Region between Galactic and Extragalactic Cosmic Rays with the Pierre Auger Observatory / Alessio Porcelli. Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2014. http://d-nb.info/1059157489/34.

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27

Kislat, Fabian [Verfasser], Hermann [Akademischer Betreuer] Kolanoski, Thomas K. [Akademischer Betreuer] Gaisser, and Gernot [Akademischer Betreuer] Maier. "Measurement of the energy spectrum of cosmic rays with the 26 station configuration of the IceTop detector / Fabian Kislat. Gutachter: Hermann Kolanoski ; Thomas K. Gaisser ; Gernot Maier." Berlin : Humboldt Universität zu Berlin, Mathematisch-Naturwissenschaftliche Fakultät I, 2012. http://d-nb.info/1019165642/34.

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28

Heil, Melanie [Verfasser], and W. de [Akademischer Betreuer] Boer. "Measurement of the positron fraction in cosmic rays from 0.5-350 GeV with the AMS-02 detector on the International Space Station / Melanie Heil. Betreuer: W. de Boer." Karlsruhe : KIT-Bibliothek, 2013. http://d-nb.info/1037154355/34.

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29

Painter, William [Verfasser], and J. [Akademischer Betreuer] Blümer. "Development of a SiPM camera for detection and measurement of fluorescence emission from extensive air-showers generated by ultra high energy cosmic rays / William Painter ; Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2019. http://d-nb.info/1197138757/34.

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30

Andreasen, Mie, Karsten H. Jensen, Marek Zreda, Darin Desilets, Heye Bogena, and Majken C. Looms. "Modeling cosmic ray neutron field measurements." AMER GEOPHYSICAL UNION, 2016. http://hdl.handle.net/10150/621996.

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The cosmic ray neutron method was developed for intermediate-scale soil moisture detection, but may potentially be used for other hydrological applications. The neutron signal of different hydrogen pools is poorly understood and separating them is difficult based on neutron measurements alone. Including neutron transport modeling may accommodate this shortcoming. However, measured and modeled neutrons are not directly comparable. Neither the scale nor energy ranges are equivalent, and the exact neutron energy sensitivity of the detectors is unknown. Here a methodology to enable comparability o

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31

Wu, Juan. "Measurements of Cosmic Ray Antiprotons with PAMELA." Licentiate thesis, KTH, Particle and Astroparticle Physics, 2010. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-12378.

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32

Zhou, Feng Ph D. Massachusetts Institute of Technology. "Cosmic ray lithium isotope measurement with AMS-01." Thesis, Massachusetts Institute of Technology, 2009. http://hdl.handle.net/1721.1/63009.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2009.<br>Cataloged from PDF version of thesis.<br>Includes bibliographical references (p. 105-112).<br>The AMS-01 detector measured charged cosmic rays during 10 days on the Space Shuttle Discovery in 1998 and collected 108 events. By identifying 8349 Lithium and 22709 Carbon nuclei from the raw data, this thesis presents the measurement of cosmic ray Lithium to Carbon ratio of presently highest statistics and momentum resolutions in the rigidity range of 2 GV to 100 GV. The 7Li to 6Li ratio is measured to be 1.07±0.16 i

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33

Mocchiutti, Emiliano. "Atmospheric and Interstellar Cosmic Rays Measured With the CAPRICE98 Experiment." Doctoral thesis, KTH, Physics, 2003. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-3643.

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34

Bultena, Sandra Lyn. "Direction measurement capabilities of the LEDA cosmic ray detector." Thesis, McGill University, 1988. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=63930.

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35

Murthy, Kavita. "Energy measurement capabilities of the LEDA cosmic ray detector." Thesis, McGill University, 1988. http://digitool.Library.McGill.CA:80/R/?func=dbin-jump-full&object_id=64058.

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36

Cossavella, Fabiana. "Measurements of high energy cosmic rays above 10 PeV with KASCADE-Grande." Eggenstein-Leopoldshafen Forschungszentrum Karlsruhe GmbH, 2009. http://d-nb.info/999765329/34.

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37

Alsop, C. "A large detector for cosmic ray abundance and energy measurements." Thesis, University of Bristol, 1988. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.384391.

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38

Cossavella, Fabiana [Verfasser]. "Measurements of high energy cosmic rays above 10 PeV with KASCADE-Grande / Fabiana Cossavella." Eggenstein-Leopoldshafen : Forschungszentrum Karlsruhe GmbH, 2009. http://d-nb.info/999765329/34.

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39

Lee, Ka-pik, and 李嘉碧. "Studies of gadolinium-loaded liquid scintillator used in the Aberdeen tunnel experiment in Hong Kong." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 2008. http://hub.hku.hk/bib/B41508658.

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40

Camp, David L. "Using a two-scintillator paddle telescope for cosmic ray flux measurements." Digital Archive @ GSU, 2012. http://digitalarchive.gsu.edu/phy_astr_theses/17.

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A two-scintillator paddle muon telescope with variable angular acceptance at the earth's surface was used to study correlations between flux distribution and barometric pressure. The detector was placed in 2 different locations around Georgia State University with varying paddle separations of 0, 7, and 14 inches. Correlation and anti-correlation analyses were conducted by using the muon count from the detector along with the barometric pressure, surface temperature, stratospheric temperature and solar activity. It was observed that there was a short and long-term variation relationship be

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41

Rivera, Villarreyes Carlos Andres. "Cosmic-ray neutron sensing for soil moisture measurements in cropped fields." Phd thesis, Universität Potsdam, 2014. http://opus.kobv.de/ubp/volltexte/2014/6974/.

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This cumulative dissertation explored the use of the detection of natural background of fast neutrons, the so-called cosmic-ray neutron sensing (CRS) approach to measure field-scale soil moisture in cropped fields. Primary cosmic rays penetrate the top atmosphere and interact with atmospheric particles. Such interaction results on a cascade of high-energy neutrons, which continue traveling through the atmospheric column. Finally, neutrons penetrate the soil surface and a second cascade is produced with the so-called secondary cosmic-ray neutrons (fast neutrons). Partly, fast neutrons are absor

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42

Nehls, Steffen. "Calibrated measurements of the radio emission of cosmic ray air showers." Karlsruhe : Forschungszentrum Karlsruhe, 2008. http://d-nb.info/992107431/34.

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43

Grove, Jon Eric Stone Edward Stone Edward. "A balloon measurement of the isotopic composition of galactic cosmic ray iron /." Diss., Pasadena, Calif. : California Institute of Technology, 1989. http://resolver.caltech.edu/CaltechETD:etd-05312007-121425.

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44

Lordello, Vitor Diorio. "Cosmic ray 2H/1H flux ratio measurement with the AMS-02 experiment." Universidade de São Paulo, 2017. http://www.teses.usp.br/teses/disponiveis/76/76132/tde-30012018-163850/.

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The Alpha Magnetic Spectrometer (AMS-02) is a cosmic ray detector operating aboard the International Space Station (ISS) since May 2011. The identification of cosmic ray deuterium and hydrogen particles is the main goal of this work. Using the data collected by the AMS-02 experiment between May 2011 and May 2014 we provide the measurement of the 2H to the 1H ratio between 0.7 and 7 GeV/n. Cosmic rays are mainly composed of hydrogen nuclei. No significant amount of deuterium nuclei is expected to be released from galactic sources since they are destroyed rather than formed in thermonuclear reac

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45

Mikuni, Vinicius Massami. "Measurement of cosmic ray electrons and positrons with the AMS-02 experiment." Universidade de São Paulo, 2017. http://www.teses.usp.br/teses/disponiveis/76/76131/tde-29092017-143310/.

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The Alpha Magnetic Spectrometer (AMS-02) is a high-energy particle physics detector operating on the International Space Station (ISS) since May 2011. Since its launch, the AMS-02 provided a large amount of data whose precision was never before achieved, opening a new path for the study of cosmic rays (CRs). The first published results of AMS-021-3 show tension with the current understanding of the cosmic ray theory, particularly at higher energies. These tensions are directly linked to many fundamental questions like the dark matter nature, the CR origin and their propagation through the gala

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46

Hiller, Roman [Verfasser], and J. [Akademischer Betreuer] Blümer. "Radio measurements for determining the energy scale of cosmic rays / Roman Hiller. Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2016. http://d-nb.info/1097380858/34.

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47

Perrett, J. C. "Measurements of scintillation and water-Cerenkov detector densities in extensive air showers produced by 10sup(16) - 5x10sup(19) eV cosmic rays." Thesis, University of Leeds, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.355950.

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48

Wu, Juan. "Measurements of cosmic ray antiprotons with PAMELA and studies of propagation models." Doctoral thesis, KTH, Partikel- och astropartikelfysik, 2012. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-95331.

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Studying the acceleration and propagation mechanisms of Galactic cosmic rays can provide information regarding astrophysical sources, the properties of our Galaxy, and possible exotic sources such as dark matter. To understand cosmic ray acceleration and propagation mechanisms, accurate measurements of different cosmic ray elements over a wide energy range are needed. The PAMELA experiment is a satellite-borne apparatus which allows different cosmic ray species to be identified over background. Measurements of the cosmic ray antiproton flux and the antiproton-to-proton flux ratio from 1.5 GeV

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49

Nehls, Steffen [Verfasser]. "Calibrated measurements of the radio emission of cosmic ray air showers / Steffen Nehls." Karlsruhe : FZKA, 2008. http://d-nb.info/998341746/34.

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50

Nierstenhoefer, Nils [Verfasser]. "On the Origin and Propagation of Ultra-High Energy Cosmic Rays (Measurements & Prediction Techniques) / Nils Nierstenhoefer." Wuppertal : Universitätsbibliothek Wuppertal, 2011. http://d-nb.info/101622592X/34.

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