Bibliografías temáticas / Cosmic ray direct detection

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Literatura académica sobre el tema "Cosmic ray direct detection"

Autor: Grafiati
Publicado: 11 de marzo de 2023

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Artículos de revistas sobre el tema "Cosmic ray direct detection"

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Putze, Antje. "Direct cosmic-ray detection." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 662 (January 2012): S157—S163. http://dx.doi.org/10.1016/j.nima.2010.11.133.

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CHEN, CHUAN-REN. "MODEL-INDEPENDENT STUDIES OF DARK MATTER." International Journal of Modern Physics D 20, no. 08 (2011): 1441–51. http://dx.doi.org/10.1142/s0218271811019621.

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The excess in cosmic-ray positrons and electrons observed by PAMELA, ATIC, PPB-BET and Fermi can be explained by dark matter decay or annihilation. On the other hand, the negative results from CDMS II and XENON direct detections of dark matter put an upper limit on the elastic-scattering cross section between dark matter and nucleon. We adopted model-independent approaches to study dark matter in cosmic-ray electrons, gamma-ray, relic density, direct detection experiments and LHC. We studied the distribution of the cosmic-ray electron flux observed at the Earth and found that it can reflect th
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Vernstrom, T., G. Heald, F. Vazza, et al. "Discovery of magnetic fields along stacked cosmic filaments as revealed by radio and X-ray emission." Monthly Notices of the Royal Astronomical Society 505, no. 3 (2021): 4178–96. http://dx.doi.org/10.1093/mnras/stab1301.

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ABSTRACT Diffuse filaments connect galaxy clusters to form the cosmic web. Detecting these filaments could yield information on the magnetic field strength, cosmic ray population, and temperature of intercluster gas; yet, the faint and large-scale nature of these bridges makes direct detections very challenging. Using multiple independent all-sky radio and X-ray maps we stack pairs of luminous red galaxies as tracers for cluster pairs. For the first time, we detect an average surface brightness between the clusters from synchrotron (radio) and thermal (X-ray) emission with ≳5σ significance, on
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Tanimori, Toru. "Detection of TeV Gamma Rays from SN1006." Symposium - International Astronomical Union 188 (1998): 121–24. http://dx.doi.org/10.1017/s0074180900114585.

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In spite of the recent progress of high energy gamma-ray astronomy, there still remains quite unclear and important problem about the origin of cosmic rays. Supernova remnants (SNRs) are the favoured site for cosmic rays up to 1016 eV, as they satisfy the requirements such as an energy input rate. But direct supporting evidence is sparse. Recently intense non-thermal X-ray emission from the rims of the Type Ia SNR SN1006 (G327.6+14.6) has been observed by ASCA (Koyama et al. 1995)and ROSAT (Willingale et al. 1996), which is considered, by attributing the emission to synchrotron radiation, to b
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Morlino, Giovanni. "Supernova Remnant-Cosmic Ray connection: a modern view." Proceedings of the International Astronomical Union 12, S331 (2017): 230–41. http://dx.doi.org/10.1017/s1743921317004793.

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AbstractThe Cosmic Ray (CR) physics has entered a new era driven by high precision measurements coming from direct detection (especially AMS-02 and PAMELA) and also from gamma-ray observations (Fermi-LAT). In this review we focus our attention on how such data impact the understanding of the supernova remnant paradigm for the origin of CRs. In particular we discuss advancement in the field concerning the three main stages of the CR life: the acceleration process, the escape from the sources and the propagation throughout the Galaxy. We show how the new data reveal a phenomenology richest than
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Perrina, Chiara. "The future of the high energy cosmic ray detection: HERD." EPJ Web of Conferences 209 (2019): 01040. http://dx.doi.org/10.1051/epjconf/201920901040.

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The High Energy cosmic-Radiation Detection (HERD) facility will be one of the space astronomy payloads on board the future Chinese space station. The ambitious aim of HERD is the direct detection of cosmic rays towards the “knee” region (~ 1 PeV), with a detector able to measure electrons, photons and nuclei with an excellent energy resolution (1% for electrons and photons at 200 GeV and 20% for nuclei at 100 GeV - PeV), an acceptance 10 times the one of present generation missions (~ 1 m2 sr), and long life-time (> 10 years). The primary objectives of HERD are the indirect search for dark
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Adriani, Oscar, Corrado Altomare, Giovanni Ambrosi, et al. "Design of an Antimatter Large Acceptance Detector In Orbit (ALADInO)." Instruments 6, no. 2 (2022): 19. http://dx.doi.org/10.3390/instruments6020019.

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A new generation magnetic spectrometer in space will open the opportunity to investigate the frontiers in direct high-energy cosmic ray measurements and to precisely measure the amount of the rare antimatter component in cosmic rays beyond the reach of current missions. We propose the concept for an Antimatter Large Acceptance Detector In Orbit (ALADInO), designed to take over the legacy of direct measurements of cosmic rays in space performed by PAMELA and AMS-02. ALADInO features technological solutions conceived to overcome the current limitations of magnetic spectrometers in space with a l
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Coogan, Adam, Benjamin V. Lehmann, and Stefano Profumo. "Connecting direct and indirect detection with a dark spike in the cosmic-ray electron spectrum." Journal of Cosmology and Astroparticle Physics 2019, no. 10 (2019): 063. http://dx.doi.org/10.1088/1475-7516/2019/10/063.

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Urban, Federico R., Stefano Camera, and David Alonso. "Detecting ultra-high-energy cosmic ray anisotropies through harmonic cross-correlations." Astronomy & Astrophysics 652 (August 2021): A41. http://dx.doi.org/10.1051/0004-6361/202038459.

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We propose an observable for ultra-high-energy cosmic ray (UHECR) physics: the harmonic-space cross-correlation power spectrum between the arrival directions of UHECRs and the large-scale cosmic structure mapped by galaxies. This cross-correlation has not yet been considered in the literature, and it permits a direct theoretical modelling of the main astrophysical components. We describe the expected form of the cross-correlation and show how, if the distribution of UHECR sources traces the large-scale cosmic structure, it could be easier to detect with current data than the UHECR auto-correla
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Cheek, Andrew. "Dark Matter Physics in Neutrino Telescopes and Neutrino Physics in Dark Matter Detectors." Journal of Physics: Conference Series 2156, no. 1 (2021): 012215. http://dx.doi.org/10.1088/1742-6596/2156/1/012215.

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Abstract It is often the case that experiments built with a focus on a specific fundamental question are sensitive to a wider range of physical phenomena. In this proceedings I discuss two cases where new insights will come from experiments that have a different primary purpose. First, presents results from Ref. [1], which assesses what simple dark matter models will be uniquely probed by a upcoming Neutrino telescope inspired by KM3NeT. Given the existing constraints from γ-ray telescopes, measurements of the cosmic microwave background and direct dark matter detection, we focus on a secluded
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Tesis sobre el tema "Cosmic ray direct detection"

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WANG, ZHAOMIN. "Measurements of Cosmic Ray Proton + Helium flux with the DAMPE experiment." Doctoral thesis, Gran Sasso Science Institute, 2020. http://hdl.handle.net/20.500.12571/9942.

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This thesis concentrates on the measurement of cosmic-ray light component (proton + helium) spectrum with the Dark Matter Particle Explorer (DAMPE). In chapter one, an introduction on cosmic-ray history is given together with the acceleration mechanism and some recent experiments. A description on DAMPE system is presented in chapter two, which includes its sub-detectors, scientific targets and parameters. There are various challenges in measuring cosmic ray energy with a limited-size calorimeter (like the BGO of DAMPE). In chapter three, various unfolding methods for reconstructing the primar
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Reichhart, Lea. "ZEPLIN-III direct dark matter search : final results and measurements in support of next generation instruments." Thesis, University of Edinburgh, 2013. http://hdl.handle.net/1842/7914.

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Astrophysical observations give convincing evidence for a vast non-baryonic component, the so-called dark matter, accounting for over 20% of the overall content of our Universe. Direct dark matter search experiments explore the possibility of interactions of these dark matter particles with ordinary baryonic matter via elastic scattering resulting in single nuclear recoils. The ZEPLIN-III detector operated on the basis of a dualphase (liquid/gas) xenon target, recording events in two separate response channels { scintillation and ionisation. These allow discrimination between electron recoils
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Mertsch, Philipp. "Cosmic ray backgrounds for dark matter indirect detection." Thesis, University of Oxford, 2010. http://ora.ox.ac.uk/objects/uuid:2734b849-4d7a-4266-8538-d3dc6cab6b20.

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The identification of the relic particles which presumably constitute cold dark matter is a key challenge for astroparticle physics. Indirect methods for their detection using high energy astro- physical probes such as cosmic rays have been much discussed. In particular, recent ‘excesses’ in cosmic ray electron and positron fluxes, as well as in microwave sky maps, have been claimed to be due to the annihilation or decay of dark matter. In this thesis, we argue however that these signals are plagued by irreducible astrophysical backgrounds and show how plausible con- ventional physics can mimi
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Halverson, Peter Georges. "Detection of high-energy cosmic ray showers by atmospheric fluorescence." Diss., The University of Arizona, 1989. http://hdl.handle.net/10150/184779.

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A novel detector for ultra-high energy cosmic rays, and its prototype are discussed. It detects events with primary energy greater than 100 PeV. (1 PeV = 1000 TeV; 1EeV = 1000 PeV.) The detector operates by sensing the near-ultraviolet scintillation light of ionized nitrogen molecules created by the passage of ionizing particles in extensive air showers. (The concept is loosely based on the highly successful Fly's Eye detector situated at Dugway, Utah.) Typical events should consist of 1 to 100 EeV primary energy showers, with near-vertical cores, passing through the detector's field-of-view a
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李耀華 and Yiu-wa Lee. "Investigation of cosmic ray intensity variation at primary rigidity above 1.7 TV." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1986. http://hub.hku.hk/bib/B42574079.

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Lorek, Ryan James. "PIERRE AUGER OBSERVATORY AND TELESCOPEARRAY JOINT COSMIC RAY DETECTION, ANDCROSS CALIBRATION." Case Western Reserve University School of Graduate Studies / OhioLINK, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=case155473314851704.

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Morris, Chad Michael. "Detection Techniques of Radio Emission from Ultra High Energy Cosmic Rays." The Ohio State University, 2009. http://rave.ohiolink.edu/etdc/view?acc_num=osu1254506832.

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Intaniwet, Akarin. "Semiconducting polymers for real time direct X-ray detection." Thesis, University of Surrey, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.538028.

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Existing inorganic materials for radiation dosimeters suffer from several drawbacks, including their inability to cover large curved areas, lack of tissueequivalence, toxicity, and mechanical inflexibility. As an alternative to inorganics, poly(triarylamine) (PTAA)-based devices have been evaluated for their suitability for detecting radiation via the direct creation of X-ray induced photocurrents. The device was prepared by sandwiching an active layer of PT AA between a transparent indium tin oxide (ITO) b()ttom contact and a metal top contact. The charge transport properties of the device we
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Bloomer, Steven David. "The search for ultra high energy gamma ray emission from Cygnus X-3 and Hercules X-1." Thesis, University of Leeds, 1990. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.238644.

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Lee, Yiu-wa. "Investigation of cosmic ray intensity variation at primary rigidity above 1.7 TV." Click to view the E-thesis via HKUTO, 1986. http://sunzi.lib.hku.hk/hkuto/record/B42574079.

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Libros sobre el tema "Cosmic ray direct detection"

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Bertone, Gianfranco. A Tale of Two Infinities. Oxford University Press, 2021. http://dx.doi.org/10.1093/oso/9780192898159.001.0001.

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The spectacular advances of modern astronomy have opened our horizon on an unexpected cosmos: a dark, mysterious Universe, populated by enigmatic entities we know very little about, like black holes, or nothing at all, like dark matter and dark energy. In this book, I discuss how the rise of a new discipline dubbed multimessenger astronomy is bringing about a revolution in our understanding of the cosmos, by combining the traditional approach based on the observation of light from celestial objects, with a new one based on other ‘messengers’—such as gravitational waves, neutrinos, and cosmic r
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Shalchi, Andreas. Nonlinear Cosmic Ray Diffusion Theories. Springer, 2009.

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Nonlinear Cosmic Ray Diffusion Theories. Springer, 2009.

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Capítulos de libros sobre el tema "Cosmic ray direct detection"

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Spurio, Maurizio. "Direct Cosmic Ray Detection: Protons, Nuclei, Electrons and Antimatter." In Astronomy and Astrophysics Library. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-96854-4_3.

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Spurio, Maurizio. "Direct Cosmic Rays Detection: Protons, Nuclei, Electrons and Antimatter." In Astronomy and Astrophysics Library. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-08051-2_3.

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Schlickeiser, Reinhard. "Direct Observations of Cosmic Rays." In Cosmic Ray Astrophysics. Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-04814-6_3.

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Schnyder, Germán, Sergio Nesmachnow, and Gonzalo Tancredi. "Distributed Cosmic Ray Detection Using Cloud Computing." In Communications in Computer and Information Science. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-73353-1_29.

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Spurio, Maurizio. "Indirect Cosmic Ray Detection: Particle Showers in the Atmosphere." In Astronomy and Astrophysics Library. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-96854-4_4.

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Zhou, Zhengdong. "Direct Iterative Basis Image Reconstruction Based on MAP-EM Algorithm for Spectral CT." In Advanced X-Ray Radiation Detection:. Springer International Publishing, 2022. http://dx.doi.org/10.1007/978-3-030-92989-3_10.

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Schnyder, Germán, Sergio Nesmachnow, Gonzalo Tancredi, and Andrei Tchernykh. "Scheduling Algorithms for Distributed Cosmic Ray Detection Using Apache Mesos." In Communications in Computer and Information Science. Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-57972-6_27.

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Siu, K. K. W., S. Sidhu, G. Falzon, et al. "Small Angle X-Ray Scattering Signatures for Breast Cancer Detection: Direct Comparison of Synchrotron and Laboratory X-Ray Sources." In IFMBE Proceedings. Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-642-03879-2_170.

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Kern, Jan, Henning Schroeder, Megan Shelby, et al. "Direct Detection of Oxygen Ligands to the Mn4Ca Complex in Photosystem II by X-ray Emission Spectroscopy." In Advanced Topics in Science and Technology in China. Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-32034-7_48.

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Kleinknecht, Konrad, and Ulrich Uwer. "Symmetry Violations and Quark Flavour Physics." In Particle Physics Reference Library. Springer International Publishing, 2020. http://dx.doi.org/10.1007/978-3-030-38207-0_9.

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AbstractOne of the surprising facts in our present understanding of the development of the Universe is the complete absence of “primordial” antimatter from the Big Bang about 13.7 billion years ago. The detection of charged cosmic-ray particles by magnetic spectrometers borne by balloons, satellites, and the space shuttle has shown no evidence for such primordial (high-energy) antibaryons; nor has the search for gamma rays from antimatter–matter annihilation yielded any such observation. In the early phases of the expanding Universe, a hot (1032 K) and dense plasma of quarks, antiquarks, leptons, antileptons and photons coexisted in equilibrium. This plasma expanded and cooled down, and matter and antimatter could recombine and annihilate into photons. If all interactions were symmetric with respect to matter and antimatter, and if baryon and lepton numbers were conserved, then all particles would finally convert to photons, and the expansion of the Universe would shift the wavelength of these photons to the far infrared region.
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Actas de conferencias sobre el tema "Cosmic ray direct detection"

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Mori, Nicola, and Lorenzo Pacini. "The High Energy Cosmic-Radiation Detection (HERD) facility for direct cosmic-ray measurements." In 41st International Conference on High Energy physics. Sissa Medialab, 2022. http://dx.doi.org/10.22323/1.414.0123.

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Quinn, Sean, S. Colognes, B. Courty, et al. "Auger at the Telescope Array: toward a direct cross-calibration of surface-detector stations." In 35th International Cosmic Ray Conference. Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0395.

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Maestro, Paolo. "Cosmic rays: direct measurements." In The 34th International Cosmic Ray Conference. Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0016.

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Mertsch, Philipp. "Rapporteur Talk: Cosmic Ray Direct." In 37th International Cosmic Ray Conference. Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0044.

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Rando, Riccardo. "Gamma rays: direct observations." In 36th International Cosmic Ray Conference. Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0029.

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Tomassetti, Nicola. "Direct Measurements of Galactic Cosmic Rays." In 27th European Cosmic Ray Symposium. Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.423.0007.

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Caputo, Regina. "ICRC 2021: Gamma-ray Direct Rapporteur." In 37th International Cosmic Ray Conference. Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0045.

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Holt, Stephen S. "Telescope systems for x-ray astronomy." In OSA Annual Meeting. Optica Publishing Group, 1987. http://dx.doi.org/10.1364/oam.1987.wp2.

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Because of the opacity of the atmosphere, x-ray astronomy must be conducted from space. Twenty-five years ago, the first detections of nonsolar x rays were made with simple proportional counters from sounding rockets. Collimated counters aboard rockets and satellites were used to follow up these discoveries, and more recently true x-ray telescopes have been used for the study of x rays from the cosmos. There are now thousands of cataloged x-ray sources ranging from nearby stars to distant quasars. The primary advantages afforded by telescopes for x-ray astronomy are twofold: direct imagery all
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Nuntiyakul, Waraporn, Pierre-Simon Mangeard, David Ruffolo, et al. "Direct Determination of a Bare Neutron Counter Yield Function." In 37th International Cosmic Ray Conference. Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.1242.

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Burnett, T. H., S. Dake, J. H. Derrickson, et al. "The direct observation of cosmic ray composition in JACEE." In Cosmic abundances of matter. AIP, 1989. http://dx.doi.org/10.1063/1.37973.

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Informes sobre el tema "Cosmic ray direct detection"

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Van Nest, Jordan D. High Altitude Cosmic Ray Detection. Iowa State University. Library. Digital Press, 2016. http://dx.doi.org/10.31274/ahac.9513.

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Van Nest, Jordan D. High Altitude Cosmic Ray Detection. Iowa State University. Library. Digital Press, 2016. http://dx.doi.org/10.31274/ahac.9765.

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Rosenberg, L., and A. Bernstein. Feasibility of Sea-level Cosmic-Ray Muon-Capture SNM Detection. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/15015181.

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

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Pan, M. Determining Muon Detection Efficiency Rates of Limited Streamer Tube Modules using Cosmic Ray Detector. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/833115.

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Matthews, John A. J., and Michael S. Gold. Exploring the Cosmic Frontier, Task A - Direct Detection of Dark Matter, Task B - Experimental Particle Astrophysics. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1289694.

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