Готові списки джерел за темами / Cosmic rays Measurement

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Добірка наукової літератури з теми "Cosmic rays Measurement"

Автор: Grafiati
Опубліковано: 4 червня 2021
Оновлено: 19 лютого 2022

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Статті в журналах з теми "Cosmic rays Measurement"

1

Rossetto, L., S. Buitink, A. Corstanje, J. E. Enriquez, H. Falcke, J. R. Hörandel, A. Nelles, et al. "Measurement of cosmic rays with LOFAR." Journal of Physics: Conference Series 718 (May 2016): 052035. http://dx.doi.org/10.1088/1742-6596/718/5/052035.

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2

Mockler, Daniela. "Measurement of the cosmic ray spectrum with the Pierre Auger Observatory." EPJ Web of Conferences 209 (2019): 01029. http://dx.doi.org/10.1051/epjconf/201920901029.

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Анотація:
The flux of ultra-high energy cosmic rays above 3×1017 eV has been measured with unprecedented precision at the Pierre Auger Observatory. The flux of the cosmic rays is determined by four different measurements. The surface detector array provides three data sets, two formed by dividing the data into two zenith angle ranges, and one obtained from a nested, denser detector array. The fourth measurement is obtained with the fluorescence detector. By combing all four data sets, the all-sky flux of cosmic rays is determined. The spectral features are discussed in detail and systematic uncertaintie
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3

Norman, Colin A. "The Highest Energy Cosmic Rays." Symposium - International Astronomical Union 175 (1996): 291–96. http://dx.doi.org/10.1017/s0074180900080864.

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Анотація:
The current data on the highest energy cosmic rays (UHECRs) is discussed and an understanding of the origin of these particles is reviewed. New and proposed facilities for measurement of UHECRs, neutrinos and γ-rays can interestingly and significantly constrain the physics of the source origin. Cosmic magnetic field strengths are the most uncertain physical parameter.
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4

Nozzoli, Francesco, and Cinzia Cernetti. "Beryllium Radioactive Isotopes as a Probe to Measure the Residence Time of Cosmic Rays in the Galaxy and Halo Thickness: A “Data-Driven” Approach." Universe 7, no. 6 (June 4, 2021): 183. http://dx.doi.org/10.3390/universe7060183.

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Анотація:
Cosmic rays are a powerful tool for the investigation of the structure of the magnetic fields in the Galactic halo and the properties of the inter-stellar medium. Two parameters of the cosmic ray propagation models, the Galactic halo (half) thickness, H, and the diffusion coefficient, D, are loosely constrained by current cosmic ray flux measurements; in particular, a large degeneracy exists, with only H/D being well measured. The 10Be/9Be isotopic flux ratio (thanks to the 2 My lifetime of 10Be) can be used as a radioactive clock providing the measurement of cosmic ray residence time in a gal
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5

HARARI, DIEGO. "MEASUREMENTS OF COSMIC RAYS AT THE HIGHEST ENERGIES WITH THE PIERRE AUGER OBSERVATORY." International Journal of Modern Physics D 20, no. 05 (May 20, 2011): 685–96. http://dx.doi.org/10.1142/s0218271811019037.

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Анотація:
Measurements with the Pierre Auger Observatory indicate with unprecedented statistics that the flux of cosmic rays is strongly suppressed above 4 × 1019 eV. The suppression is consistent with the prediction that cosmic rays with larger energies can only arrive from nearby sources due to their interaction with the cosmic microwave background, but could also be related to the efficiency of the acceleration processes at the sources. The Observatory has found independent evidence of the nearby extragalactic origin of cosmic rays with energy above ~6×1019 eV with a measurement of the fraction of ar
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6

An, Q., R. Asfandiyarov, P. Azzarello, P. Bernardini, X. J. Bi, M. S. Cai, J. Chang, et al. "Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite." Science Advances 5, no. 9 (September 2019): eaax3793. http://dx.doi.org/10.1126/sciadv.aax3793.

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Анотація:
The precise measurement of the spectrum of protons, the most abundant component of the cosmic radiation, is necessary to understand the source and acceleration of cosmic rays in the Milky Way. This work reports the measurement of the cosmic ray proton fluxes with kinetic energies from 40 GeV to 100 TeV, with 2 1/2 years of data recorded by the DArk Matter Particle Explorer (DAMPE). This is the first time that an experiment directly measures the cosmic ray protons up to ~100 TeV with high statistics. The measured spectrum confirms the spectral hardening at ~300 GeV found by previous experiments
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7

Kostunin, D., P. A. Bezyazeekov, N. M. Budnev, D. Chernykh, O. Fedorov, O. A. Gress, A. Haungs, et al. "Present status and prospects of the Tunka Radio Extension." EPJ Web of Conferences 216 (2019): 01005. http://dx.doi.org/10.1051/epjconf/201921601005.

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The Tunka Radio Extension (Tunka-Rex) is a digital radio array operating in the frequency band of 30-80 MHz and detecting radio emission from air-showers produced by cosmic rays with energies above 100 PeV. The experimentis installed at the site of the TAIGA (Tunka Advanced Instrument for cosmic rays and Gamma Astronomy) observatory and performs joint measurements with the co-located particle and air-Cherenkov detectors in passive mode receiving a trigger from the latter. Tunka-Rex collects data since 2012, and during the last five years went throughseveral upgrades. As a result the density of
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8

Mariazzi, Analisa. "Highest energy particle physics with the Pierre Auger Observatory." International Journal of Modern Physics: Conference Series 31 (January 2014): 1460301. http://dx.doi.org/10.1142/s2010194514603019.

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Анотація:
Astroparticles offer a new path for research in the field of particle physics, allowing investigations at energies above those accesible with accelerators. Ultra-high energy cosmic rays can be studied via the observation of the showers they generate in the atmosphere. The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays, combining two complementary measurement techniques used by previous experiments, to get the best possible measurements of these air showers. Shower observations enable one to not only estimate the energy, direction and most probable mass of the p
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9

Oschlies, K., R. Beaujean, and W. Enge. "Measurement of low energy cosmic rays aboard Spacelab-1." International Journal of Radiation Applications and Instrumentation. Part D. Nuclear Tracks and Radiation Measurements 12, no. 1-6 (January 1986): 407–9. http://dx.doi.org/10.1016/1359-0189(86)90620-5.

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10

DE MELLO NETO, J. R. T. "ULTRA HIGH ENERGY COSMIC RAYS WITH THE PIERRE AUGER OBSERVATORY." International Journal of Modern Physics: Conference Series 18 (January 2012): 221–29. http://dx.doi.org/10.1142/s2010194512008495.

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Анотація:
We present the status and the recent measurements from the Pierre Auger Observatory. The energy spectrum is described and its features discussed. We report searches for anisotropy of cosmic rays arrival directions in large scales and through correlation with catalogues of celestial objects. The measurement of the cross section proton-air is discussed. Finally, the mass composition is addressed with the measurements of the variation of the depth of shower maximum with energy and with the muon density at ground.
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Дисертації з теми "Cosmic rays Measurement"

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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Анотація:
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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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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Анотація:
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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Анотація:
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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Анотація:
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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Анотація:
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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Книги з теми "Cosmic rays Measurement"

1

Keane, Anthony J. Measurement of the charge spectrum of ultra heavy galactic cosmic rays with Z>70. Dublin: University College Dublin, 1997.

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2

Workshop on Balloon-Borne Experiment With a Superconducting Magnet Spectrometer (6th 1996 KEK). Proceedings of the 6th Workshop on Balloon-Borne Experiment with a Superconducting Magnet Spectrometer: Held at National Laboratory for High Energy Physics (KEK), Jan., 29-31, 1996. Oho, Tsukuba-shi, Ibaraki-ken, Japan: Natinal Laboratory for High Energy Physics, 1996.

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3

Zhou, Dazhuang. CR-39 plastic nuclear track detectors in physics research. Hauppauge, N.Y: Nova Science Publishers, 2011.

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4

Boscherini, Massimo. The Time-of-Flight counter for the PAMELA experiment in space: Design, development, construction and qualification. Münster: Verlagshaus Monsenstein und Vannerdat, 2004.

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5

service), SpringerLink (Online, ed. A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012.

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6

Gregory, J. C. A measurement of the energy spectra of cosmic rays from 20 to 1000 GeV per amu: Semiannual report. [Huntsville, Ala.]: University of Alabama in Huntsville, 1991.

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7

Hohlmann, Marcus. Test der Vorwärts-Spurkammern des H1 Detektors mit kosmischen Teilchen. Aachen: Physikalische Institute RWTH Aachen, 1992.

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8

Abunina, Maria, Rolf Bütikofer, Karl-Ludwig Klein, Olga Kryakunova, Monica Laurenza, David Ruffolo, Danislav Sapundjiev, Christian T. Steigies, and Ilya Usoskin, eds. NMDB@Home 2020. Kiel: Universitätsverlag Kiel | Kiel University Publishing, 2021. http://dx.doi.org/10.38072/2748-3150/v1.

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Анотація:
With the 'Proceedings of the 1st virtual symposium on cosmic ray studies with neutron detectors' launches the new open access series 'Cosmic ray studies with neutron detectors'. The volume comprises the papers presented at the online meeting held in July 2020. The contributions show that neutron detectors on the ground provide significant results for studying the interaction of galactic cosmic rays with magnetic fields in the heliosphere, for accelerating energetic particles, and for a growing number of applications, including geophysics and space weather. The easily accessible databases aroun
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9

Nakamura, Takashi. Dosimetry and spectrometry of cosmic-ray neutrons in aircraft: DOSCONA experiment. Chiba: National Institute of Radiological Sciences, 2011.

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10

Flynn, George. "Trace element abundance measurements on cosmic dust particles": Final report. [Washington, DC: National Aeronautics and Space Administration, 1996.

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Частини книг з теми "Cosmic rays Measurement"

1

Hofmann, W., and J. A. Hinton. "Cosmic Particle Accelerators." In Particle Physics Reference Library, 827–63. Cham: Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-34245-6_13.

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AbstractIn the century since the measurements of Victor Hess [1]—considered as the discovery of cosmic rays—the properties of cosmic rays, as they arrive on Earth, have been studied in remarkable detail; we know their energy spectrum, extending to 1020 eV, their elemental composition, their angular distribution, and we understand the basic energetic requirements of cosmic ray production in the Galaxy.
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2

Lesko, K. T., E. B. Norman, R. M. Larimer, and S. G. Crane. "Measurements of Cross Sections Relevant to γ-Ray Line Astronomy." In Genesis and Propagation of Cosmic Rays, 375–79. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-4025-3_24.

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3

Zilles, Anne. "Going to Extreme Precision Measurements: Detecting Cosmic Rays with SKA1-Low." In Emission of Radio Waves in Particle Showers, 89–127. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-63411-1_6.

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4

Ney, E. P., and J. R. Winckler. "High Altitude Cosmic-Ray Measurements During the International Geophysical Year." In Geophysics and the IGY: Proceedings of the Symposium at the Opening of the International Geophysical Year, 81–91. Washington D. C.: American Geophysical Union, 2013. http://dx.doi.org/10.1029/gm002p0081.

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5

Roy, S., R. P. Adak, R. Biswas, D. Nag, D. Paul, S. Rudra, S. Biswas, and S. Das. "Measurement of Angular Variation of Cosmic Ray Intensity with Plastic Scintillator Detector." In Springer Proceedings in Physics, 199–204. Singapore: Springer Singapore, 2018. http://dx.doi.org/10.1007/978-981-10-7665-7_20.

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6

Neher, H. V., and S. E. Forbush. "Correlation of cosmic-ray ionization measurements at high altitudes, at sea level, and neutron intensities at mountain tops." In Cosmic Rays, the Sun and Geomagnetism: The Works of Scott E. Forbush, 181–82. Washington, D. C.: American Geophysical Union, 1993. http://dx.doi.org/10.1029/sp037p0181.

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Wiegel, B., T. Ohrndorf, and W. Heinrich. "Measurements of Cosmic Ray LET-Spectra for the D1 Mission Using Plastic Nuclear Track Detectors." In Terrestrial Space Radiation and Its Biological Effects, 795–807. Boston, MA: Springer US, 1988. http://dx.doi.org/10.1007/978-1-4613-1567-4_52.

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Slayman, Charles. "JEDEC Standards on Measurement and Reporting of Alpha Particle and Terrestrial Cosmic Ray Induced Soft Errors." In Soft Errors in Modern Electronic Systems, 55–76. Boston, MA: Springer US, 2010. http://dx.doi.org/10.1007/978-1-4419-6993-4_3.

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Dorman, Lev I. "Theory of Cosmic Ray Meteorological Effects for Measurements in the Atmosphere and Underground (One-Dimensional Approximation)." In Astrophysics and Space Science Library, 289–330. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-2113-8_5.

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Venkatesan, D., R. B. Decker, and S. M. Krimigis. "Measurement of Radial and Latitudinal Gradients of Cosmic Ray Intensity During the Decreasing Phase of Sunspot Cycle 21." In Astrophysics and Space Science Library, 389–94. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4612-5_46.

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Тези доповідей конференцій з теми "Cosmic rays Measurement"

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AbuZayyad, Tareq. "TALE FD Cosmic Rays Composition Measurement." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0169.

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Ridky, Jan. "Measurement of Cosmic Ray Energy with the Pierre Auger Observatory." In C2CR07: COLLIDERS TO COSMIC RAYS. AIP, 2007. http://dx.doi.org/10.1063/1.2775894.

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Fleischhack, Henrike. "Measurement of the Iron Spectrum in Cosmic Rays with VERITAS." In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0500.

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Ma, PengXiong, Margherita Di Santo, ZhiHui Xu, and Yongjie Zhang. "Charge measurement of cosmic rays by Plastic Scintillantor Detector of DAMPE." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0073.

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Huang, Jing, M. Amenomori, X. J. Bi, D. Chen, T. L. Chen, W. Y. Chen, S. W. Cui, et al. "Measurement of high energy cosmic rays by the new Tibet hybrid experiment." In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0484.

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Bongi, M. "PAMELA: a satellite experiment for antiparticles measurement in cosmic rays." In 2003 IEEE Nuclear Science Symposium. Conference Record (IEEE Cat. No.03CH37515). IEEE, 2003. http://dx.doi.org/10.1109/nssmic.2003.1351878.

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Smolek, Karel, Jakub Cermak, Peter Lichard, Michal Nyklicek, Stanislav Pospisil, Petr Pridal, Jaroslav Smejkal, Ivan Stekl, Vladimir Vicha, and Martin Vojik. "Measurement of High Energy Cosmic Rays in the Experiment CZELTA." In 2008 IEEE Nuclear Science Symposium and Medical Imaging conference (2008 NSS/MIC). IEEE, 2008. http://dx.doi.org/10.1109/nssmic.2008.4774529.

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Salamon, M. H., P. B. Price, and G. Tarle. "Measurement of ultra-heavy cosmic rays at a lunar base." In Physics and Astrophysics from a Lunar Base. AIP, 1990. http://dx.doi.org/10.1063/1.39118.

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9

Libo, WU, Mingyang Cui, Dimitrios Kyratzis, Andrea Parenti, and Yifeng Wei. "Towards the measurement of carbon and oxygen spectra in cosmic rays with DAMPE." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0128.

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10

Di Sciascio, Giuseppe. "Measurement of (p+He)-induced anisotropy in cosmic rays with ARGO-YBJ." In The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0290.

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Звіти організацій з теми "Cosmic rays Measurement"

1

Collica, Laura. Mass composition studies of Ultra High Energy cosmic rays through the measurement of the Muon Production Depths at the Pierre Auger Observatory. Office of Scientific and Technical Information (OSTI), January 2014. http://dx.doi.org/10.2172/1249492.

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2

Eylander, John, Michael Lewis, Maria Stevens, John Green, and Joshua Fairley. An investigation of the feasibility of assimilating COSMOS soil moisture into GeoWATCH. Engineer Research and Development Center (U.S.), September 2021. http://dx.doi.org/10.21079/11681/41966.

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Анотація:
This project objective evaluated the potential of improving linked weather-and-mobility model predictions by blending soil moisture observations from a Cosmic-ray Soil Moisture Observing System (COSMOS) sensor with weather-informed predictions of soil moisture and soil strength from the Geospatial Weather-Affected Terrain Conditions and Hazards (GeoWATCH). Assimilating vehicle-borne COSMOS observations that measure local effects model predictions of soil moisture offered potential to produce more accurate soil strength and vehicle mobility forecast was the hypothesis. This project compared soi
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3

McIntosh, Gordon. Cosmic Ray Measurements A Proposed, Collaborative, Balloon Based Experiment. Ames (Iowa): Iowa State University. Library. Digital Press, January 2012. http://dx.doi.org/10.31274/ahac.8340.

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4

Celmins, Aivars. Feasibility of Cosmic-Ray Muon Intensity Measurements for Tunnel Detection. Fort Belvoir, VA: Defense Technical Information Center, June 1990. http://dx.doi.org/10.21236/ada223355.

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5

Verbeke, J. M., N. J. Snyderman, and L. F. Nakae. Comparison between Neutron Counting Experimental Measurements and Simulations: Cosmic Ray Contribution. Office of Scientific and Technical Information (OSTI), February 2008. http://dx.doi.org/10.2172/1113922.

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6

Hocker, Andy, Paul Rubinov, Doug Glenzinski, Sten Hansen, Julie Whitmore, Craig Dukes, Craig Group, Yuriy Oksuzian, Martin Frank, and Ralf Ehrlich. T-1043: Measurements of Photoelectron Yields for Prototype Mu2e Cosmic Ray Veto Scintillation Counters. Office of Scientific and Technical Information (OSTI), August 2013. http://dx.doi.org/10.2172/1128251.

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