Gotowe bibliografie tematyczne / Atmospheric muon

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Części książek
  4. Streszczenia konferencji
  5. Raporty organizacyjne

Gotowa bibliografia na temat „Atmospheric muon”

Autor: Grafiati
Data publikacji: 7 grudnia 2024
Data aktualizacji: 31 lipca 2025

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Artykuły w czasopismach na temat "Atmospheric muon"

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Kajita, Takaaki. "Atmospheric Neutrinos." Advances in High Energy Physics 2012 (2012): 1–24. http://dx.doi.org/10.1155/2012/504715.

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Atmospheric neutrinos are produced as decay products in hadronic showers resulting from collisions of cosmic rays with nuclei in the atmosphere. Electron-neutrinos and muon-neutrinos are produced mainly by the decay chain of charged pions to muons to electrons. Atmospheric neutrino experiments observed zenith angle and energy-dependent deficit of muon-neutrino events. It was found that neutrino oscillations between muon-neutrinos and tau-neutrinos explain these data well. This paper discusses atmospheric neutrino experiments and the neutrino oscillation studies with these neutrinos.
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Yanchukovsky, Valery. "MUON INTENSITY VARIATIONS AND ATMOSPHERIC TEMPERATURE." Solar-Terrestrial Physics 6, no. 1 (2020): 108–15. http://dx.doi.org/10.12737/stp-61202013.

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Muons in the atmosphere are formed during the decay of pions resulting from nuclear interactions of cosmic rays with nuclei of air atoms. The resulting muons are also unstable particles with a short lifetime. Therefore, not all of them reach the level of observation in the atmosphere. When the atmospheric temperature changes, the distance to the observation level changes too, thus leading to variations in the intensity of muons of temperature origin. These variations, caused by atmospheric temperature variations, are superimposed on continuous observations of muon telescopes. Their exclusion i
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Yanchukovsky, Valery. "MUON INTENSITY VARIATIONS AND ATMOSPHERIC TEMPERATURE." Solnechno-Zemnaya Fizika 6, no. 1 (2020): 134–41. http://dx.doi.org/10.12737/szf-61202013.

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Muons in the atmosphere are formed during the decay of pions resulting from nuclear interactions of cosmic rays with nuclei of air atoms. The resulting muons are also unstable particles with a short lifetime. Therefore, not all of them reach the level of observation in the atmosphere. When the atmospheric temperature changes, the distance to the observation level changes too, thus leading to variations in the intensity of muons of temperature origin. These variations, caused by atmospheric temperature variations, are superimposed on continuous observations of muon telescopes. Their exclusion i
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Cecchini, S., and M. Spurio. "Atmospheric muons: experimental aspects." Geoscientific Instrumentation, Methods and Data Systems Discussions 2, no. 2 (2012): 603–41. http://dx.doi.org/10.5194/gid-2-603-2012.

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Abstract. We present a review of atmospheric muon flux and energy spectrum measurements over almost six decades of muon momentum. Sea-level and underground/water/ice experiments are considered. Possible sources of systematic errors in the measurements are examinated. The characteristics of underground/water muons (muons in bundle, lateral distribution, energy spectrum) are discussed. The connection between the atmospheric muon and neutrino measurements are also reported.
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Cecchini, S., and M. Spurio. "Atmospheric muons: experimental aspects." Geoscientific Instrumentation, Methods and Data Systems 1, no. 2 (2012): 185–96. http://dx.doi.org/10.5194/gi-1-185-2012.

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Abstract. We present a review of atmospheric muon flux and energy spectrum measurements over almost six decades of muon momentum. Sea level and underground/water/ice experiments are considered. Possible sources of systematic errors in the measurements are examined. The characteristics of underground/water muons (muons in bundle, lateral distribution, energy spectrum) are discussed. The connection between the atmospheric muon and neutrino measurements are also reported.
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Янчуковский, Валерий, Valery Yanchukovsky, Василий Кузьменко, and Vasiliy Kuzmenko. "Atmospheric effects of the cosmic-ray mu-meson component." Solar-Terrestrial Physics 4, no. 3 (2018): 76–82. http://dx.doi.org/10.12737/stp-43201810.

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Variations in the intensity of cosmic rays observed in the depth of the atmosphere include the atmospheric component of the variations. Cosmic-ray muon telescopes, along with the barometric effect, have a significant temperature effect due to the instability of detected particles. To take into account atmospheric effects in muon telescope data, meteorological coefficients of muon intensity are found. The meteorological coefficients of the intensity of muons recorded in the depth of the atmosphere are estimated from experimental data, using various methods of factor analysis. The results obtain
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Янчуковский, Валерий, Valery Yanchukovsky, Василий Кузьменко, and Vasiliy Kuzmenko. "Atmospheric effects of the cosmic-ray mu-meson component." Solnechno-Zemnaya Fizika 4, no. 3 (2018): 95–102. http://dx.doi.org/10.12737/szf-43201810.

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Variations in the intensity of cosmic rays observed in the depth of the atmosphere include the atmospheric component of the variations. Cosmic-ray muon telescopes, along with the barometric effect, have a significant temperature effect due to the instability of detected particles. To take into account atmospheric effects in muon telescope data, meteorological coeffi-cients of muon intensity are found. The meteorological coefficients of the intensity of muons recorded in the depth of the atmosphere are estimated from experi-mental data, using various methods of factor analysis. The results obta
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SANUKI, TOMOYUKI. "REVIEW OF BALLOONS MUON MEASUREMENT IN THE ATMOSPHERE." International Journal of Modern Physics A 17, no. 12n13 (2002): 1635–44. http://dx.doi.org/10.1142/s0217751x02011138.

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In order to study neutrino oscillation phenomena using atmospheric neutrinos, it is crucially important to calculate their absolute fluxes and spectral shapes accurately. Since production and decay processes of muons are accompanied by neutrino production, observations of atmospheric muons give fundamental information about atmospheric neutrinos. Atmospheric muons have been measured at various sites; from a ground level to a balloon floating altitude. Very precise measurement has been carried out on the ground. Muon growth curves are measured during balloon ascending periods. These data can be
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MITRA, MALA, and D. P. BHATTACHARYYA. "ESTIMATION OF UPWARD MUON ENERGY SPECTRA IN THE EARTH INDUCED BY DIFFUSE MUON NEUTRINOS EMITTED FROM THE ATMOSPHERIC, GALACTIC AND ACTIVE GALACTIC NUCLEAR SOURCES." International Journal of Modern Physics A 13, no. 02 (1998): 209–21. http://dx.doi.org/10.1142/s0217751x98000081.

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The energy spectra of upward muons in the Earth emitted by atmospheric, galactic and AGN diffuse muon neutrinos incident on the Earth have been estimated using the standard formulation developed by Gaisser based on charge–current interactions in rock along with the QED-based energy loss formulation. The derived primary-cosmic-nucleus–air interaction yield neutrino-induced muon spectrum in the vertical direction is in accord with the recent data available from MACRO, IMB, KAMIOKA and BAKSAN underground experiments for energies below 3 GeV. The TeV muon energy spectra initiated by atmospheric, g
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Кузьменко, Василий, Vasiliy Kuzmenko, Валерий Янчуковский, and Valery Yanchukovsky. "Determination of density of temperature coefficients for the Earth’s atmosphere muons." Solnechno-Zemnaya Fizika 1, no. 2 (2015): 91–96. http://dx.doi.org/10.12737/10403.

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When studying variations of cosmic ray intensity, by the use of muon telescopes located deep in the atmosphere it is necessary to take into account changes in atmospheric parameters, mainly pressure and temperature. The density distribution of temperature coefficients of the atmosphere muon intensity needs to be estimated from observations. To this purpose, the method of principal components regression and meth-ods of projection to latent structures (PLS-1 and PLS-2). We used data of continuous recording of muons, as well as Novosibirsk 2004–2010 aerological data. As shown by comparing results
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Rozprawy doktorskie na temat "Atmospheric muon"

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Bazzotti, Marco <1980&gt. "Studies of the atmospheric muon flux with the ANTARES detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1906/1/bazzotti_marco_tesi.pdf.

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The thesis main topic is the determination of the vertical component of the atmospheric muon flux as a function of the sea depth at the ANTARES site. ANTARES is a Cherenkov neutrino telescope placed at 2500m depth in the Mediterranean Sea at 40 km from the southern cost of France. In order to retrieve back the physical flux from the experimental data a deconvolution algorithm has been perform which takes into consideration the trigger inefficiensies and the reconstruction errors on the zenith angle. The obtained results are in good agreement with other ANTARES indipendent analysis.
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Bazzotti, Marco <1980&gt. "Studies of the atmospheric muon flux with the ANTARES detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2009. http://amsdottorato.unibo.it/1906/.

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The thesis main topic is the determination of the vertical component of the atmospheric muon flux as a function of the sea depth at the ANTARES site. ANTARES is a Cherenkov neutrino telescope placed at 2500m depth in the Mediterranean Sea at 40 km from the southern cost of France. In order to retrieve back the physical flux from the experimental data a deconvolution algorithm has been perform which takes into consideration the trigger inefficiensies and the reconstruction errors on the zenith angle. The obtained results are in good agreement with other ANTARES indipendent analysis.
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Pretz, John. "Detection of atmospheric muon neutrinos with the IceCube 9-String Detector." College Park, Md. : University of Maryland, 2006. http://hdl.handle.net/1903/4163.

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Thesis (Ph. D.) -- University of Maryland, College Park, 2006.<br>Thesis research directed by: Physics. Title from t.p. of PDF. Includes bibliographical references. Published by UMI Dissertation Services, Ann Arbor, Mich. Also available in paper.
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Mauri, Nicoletta <1980&gt. "Measurement of the atmospheric muon charge ratio with the OPERA detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3932/1/Mauri_Nicoletta_Tesi.pdf.

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The atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is an interesting quantity for the study of high energy hadronic interactions in atmosphere and the nature of the primary cosmic rays. The measurement of the charge ratio in the TeV muon energy range allows to study the hadronic interactions in kinematic regions not yet explored at accelerators. The OPERA experiment is a hybrid electronic detector/emulsion apparatus, located in the underground Gran Sasso Laboratory, at an average depth of 3800 meters water equivalent (m.w.e.). OPERA is the first
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Mauri, Nicoletta <1980&gt. "Measurement of the atmospheric muon charge ratio with the OPERA detector." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2011. http://amsdottorato.unibo.it/3932/.

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The atmospheric muon charge ratio, defined as the number of positive over negative charged muons, is an interesting quantity for the study of high energy hadronic interactions in atmosphere and the nature of the primary cosmic rays. The measurement of the charge ratio in the TeV muon energy range allows to study the hadronic interactions in kinematic regions not yet explored at accelerators. The OPERA experiment is a hybrid electronic detector/emulsion apparatus, located in the underground Gran Sasso Laboratory, at an average depth of 3800 meters water equivalent (m.w.e.). OPERA is the first
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Bailly-Salins, Louis. "Atmοspheric muοn studies and light sterile neutrinο search with ΚΜ3ΝeΤ/ΟRCA". Electronic Thesis or Diss., Normandie, 2024. http://www.theses.fr/2024NORMC228.

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La collaboration KM3NeT construit actuellement deux télescopes Cherenkov à neutrinos au fond de la mer Méditerranée, ORCA (Oscillation Research with Cosmics in the Abyss) pour mesurer les oscillations des neutrinos atmosphériques et ARCA (Astroparticle Research with Cosmics in the Abyss) pour détecter les neutrinos provenant de sources astrophysiques.Dans ce manuscrit, après avoir passé en revue l'état des mesures d'oscillation des neutrinos et des recherches de neutrinos stériles légers dans le premier chapitre, les détecteurs KM3NeT sont présentés dans le deuxième chapitre.Dans le chapitre 3
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Versari, Federico <1992&gt. "Measurement of the atmospheric electron and muon neutrino flux with the ANTARES neutrino telescope." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amsdottorato.unibo.it/9664/1/PhD_Thesis____.pdf.

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This thesis presents a combined measurement of the energy spectra of atmospheric electron and muon neutrinos in the energy range between around 100 GeV and 50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period from 2007 to 2017, and selects 1016 neutrino interacting in (or close to) the instrumented volume of the detector, yielding shower-like events and starting track events. The contamination by atmospheric muons is suppressed at the level of a few per mill by different steps in the selection analysis, including a Boosted Decision Tree cla
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Haberland, Marcus. "A search for a prompt atmospheric muon neutrino flux in the northern hemisphere using data releases from IceCube." Thesis, Uppsala universitet, Högenergifysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-415984.

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The IceCube Neutrino Observatory is a cubic kilometre scale detector for high-energy neutrinos above hundreds of GeV produced in Earth’s atmosphere as well as outside our solar system whenever particles are accelerated to ultra-relativistic energies. The prompt atmospheric contribution is a result of the creation of heavy mesons with charm components in the atmosphere. Past studies from IceCube using a maximum likelihood estimation over the whole neutrino energy spectrum always reported a best-fit zero prompt contribution so far [1–5], contrary to theory [6, 7]. In this analysis we tried to me
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Biron, von Curland Alexander. "Search for atmospheric muon neutrinos and extraterrestric neutrino point sources in the 1997 AMANDA-B10 data." [S.l.] : [s.n.], 2002. http://deposit.ddb.de/cgi-bin/dokserv?idn=964841223.

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Geyer, Klaus [Verfasser], and Gisela [Akademischer Betreuer] Anton. "Measurements of the atmospheric muon rate with the ANTARES neutrino telescope / Klaus Geyer. Gutachter: Gisela Anton." Erlangen : Friedrich-Alexander-Universität Erlangen-Nürnberg (FAU), 2015. http://d-nb.info/1076165915/34.

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Części książek na temat "Atmospheric muon"

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Learned, John G. "The Atmospheric Neutrino Anomaly: Muon Neutrino Disappearance." In Current Aspects of Neutrino Physics. Springer Berlin Heidelberg, 2001. http://dx.doi.org/10.1007/978-3-662-04597-8_5.

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Chiarusi, Tommaso. "L3+Cosmics: an atmospheric muon experiment at CERN." In Astrophysical Sources of High Energy Particles and Radiation. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0560-9_28.

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Spurio, Maurizio. "Atmospheric Muons and Neutrinos." In Astronomy and Astrophysics Library. Springer International Publishing, 2014. http://dx.doi.org/10.1007/978-3-319-08051-2_11.

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Spurio, Maurizio. "Atmospheric Muons and Neutrinos." In Astronomy and Astrophysics Library. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-96854-4_11.

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Paul, Surojit, K. P. Arunbabu, M. Chakraborty, et al. "Monitoring the Upper Atmosphere and Interplanetary Magnetic Field Using Atmospheric Muons at GRAPES-3." In Springer Proceedings in Physics. Springer Nature Singapore, 2024. http://dx.doi.org/10.1007/978-981-97-0289-3_267.

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Lee, T. D., H. Robinson, M. Schwartz, and R. Cool. "Intensity of Upward Muon Flux due to Cosmic-Ray Neutrinos Produced in the Atmosphere." In Selected Papers. Birkhäuser Boston, 1986. http://dx.doi.org/10.1007/978-1-4612-5397-6_21.

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Hoffmann, Michael R. "Possible Chemical Transformations in Snow and Ice Induced by Solar (UV PHOTONS) and Cosmic Irradiation (MUONS)." In Chemical Exchange Between the Atmosphere and Polar Snow. Springer Berlin Heidelberg, 1996. http://dx.doi.org/10.1007/978-3-642-61171-1_16.

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"Recent results from SND@LHC, the Scattering and Neutrino Detector at the CERN LHC." In Book of Abstracts - RAD 2025 Conference. RAD Centre, Niš, Serbia, 2025. https://doi.org/10.21175/rad.abstr.book.2025.30.8.

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SND@LHC is a compact and stand-alone experiment to perform measurements with very high energy neutrinos produced at the CERN Large Hadron Collider. The experiment is located 480 m downstream of the proton-proton interaction point IP1 in the unused TI18 tunnel. The detector is composed of a hybrid system based on an 800 kg target mass of tungsten plates, interleaved with emulsion and electronic trackers, followed downstream by a calorimeter and a muon system. The configuration allows efficiently distinguishing between all three neutrino flavours, opening a unique opportunity to probe physics of
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Reines, F., W. R. Kropp, H. W. Sobel, et al. "Muons Produced By Atmospheric Neutrinos: Experiment." In Neutrinos and Other Matters. WORLD SCIENTIFIC, 1991. http://dx.doi.org/10.1142/9789814343060_0034.

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Chen, H. H., W. R. Kropp, H. W. Sobel, and F. Reines. "Muons Produced by Atmospheric Neutrinos: Analysis." In Neutrinos and Other Matters. WORLD SCIENTIFIC, 1991. http://dx.doi.org/10.1142/9789814343060_0035.

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Streszczenia konferencji na temat "Atmospheric muon"

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Gorovtsov, Petr. "Calibration of the DANSS detector with stopped atmospheric muons and their decays." In 42nd International Conference on High Energy Physics. Sissa Medialab, 2024. https://doi.org/10.22323/1.476.0205.

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R. Savić, Mihailo, Nikola B. Veselinović, Aleksandar L. Dragić, et al. "Preliminary Analysis of Barometric and Temperature Effects in Cosmic Muon Datasets Simulated Using CORSIKA." In International scientific conference: Meeting on new trends in Astronomy & Earth Observation. Scientific Society Isaac Newton Belgrade, 2024. https://doi.org/10.69646/aob241219.

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Abstract: Muon detectors are among the most widely used ground- based cosmic ray detectors, alongside neutron monitors. Due to the fact they detect higher energy primary cosmic rays, they serve as a complement to neutron monitors for long-term monitoring of cosmic ray variations and the study of space weather phenomena. Furthermore, alongside the existing independent detector setups and established networks, new muon detector networks are currently being developed and implemented.Secondary cosmic ray muons are sensitive to changes in atmospheric conditions, particularly variations in atmospher
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Kuzmitskiy, A. V., and A. A. Kochanov. "DEPTH INTENSITY RELATION AND ANGULAR DISTRIBUTION OF THE HIGH-ENERGY ATMOSPHERIC MUONS IN WATER MEDIUM: NEW CALCULATION." In Baikal Young Scientists’ International School on Fundamental Physics. Institute of Solar-Terrestrial Physics SB RAS, 2024. http://dx.doi.org/10.62955/0135-3748-2024-51.

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One of the important tasks of high-energy astrophysics is the search for cosmic neutrinos and the determination of their sources. To solve this problem, large-volume detectors are being created – neutrino telescopes that register Cherenkov light from charged particles generated by neutrino interactions in the medium. Cherenkov light can be produced not only by muons from neutrinos or hadron showers, but also by transit atmospheric muons. Therefore, the analysis of events, recorded in neutrino telescopes, requires a thorough study of the background of muons. It is necessary to know the characte
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Savić, M. R., N. B. Veselinović, A. L. Dragić, et al. "Implications of the Temperature Effect Analysis Using Simulated Secondary Cosmic Muon Data." In International Meeting on Data for Atomic and Molecular Processes in Plasmas: Advances in Standards and Modelling. Institute of Physics Belgrade, 2024. https://doi.org/10.69646/aob241110.

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As it propagates through the atmosphere, the muon component of secondary cosmic rays is influenced by variations in atmospheric parameters. The two most significant atmospheric effects affecting the muon flux detected at ground level are the barometric effect, due to changes in atmospheric pressure, and the temperature effect, caused by fluctuations in atmospheric temperature.To enhance the sensitivity of ground-based muon detectors to cosmic ray variations of non-atmospheric origin, these effects must be corrected, with the temperature effect being more complex to model. The most well-establi
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Aamir, Yusuf. "Muon Flux Variance from Severe Atmospheric Conditions." In Muon Flux Variance from Severe Atmospheric Conditions. US DOE, 2024. http://dx.doi.org/10.2172/2429212.

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Garg, Diksha, and Mary Hall Reno. "Atmospheric muon fluxes at sub-orbital neutrino detectors." In 38th International Cosmic Ray Conference. Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.444.0370.

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Bardačová, Zuzana. "Atmospheric muon suppression for Baikal-GVD cascade analysis." In 38th International Cosmic Ray Conference. Sissa Medialab, 2023. http://dx.doi.org/10.22323/1.444.0986.

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CIRCELLA, M. "MUON MEASUREMENTS IN THE ATMOSPHERE IN THE CONTEXT OF THE ATMOSPHERIC NEUTRINO ANOMALY." In Proceedings of the International School of Cosmic Ray Astrophysics 20th Anniversary, 11th Course. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812793997_0005.

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Savić, Mihailo, Nikola Veselinović, Aleksandar Dragić, et al. "Cosmic Rays and Their Connection to Space Weather and Earth’s Climate." In Building bridges between climate science and society through a transdisciplinary network. Scientific Society Isaac Newton, 2024. http://dx.doi.org/10.69646/bbbs2407.

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Cosmic rays have been studied for over a century. In addition to investigating their fundamental properties, such as origin, composition, and acceleration mechanisms, some of the most important studies in the field involve the interaction of cosmic rays within the heliosphere, near-Earth space, and the immediate Earth’s environment. These areas have been of particular interest in recent years.One such type of study focuses on the modulation of cosmic rays by the solar magnetic field and the geomagnetic field in the heliosphere and Earth’s magnetosphere, respectively. Among other things, the st
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Clark, R. "The atmospheric neutrino muon-like fraction above 1 GeV." In INTERSECTIONS BETWEEN PARTICLE AND NUCLEAR PHYSICS. ASCE, 1997. http://dx.doi.org/10.1063/1.54393.

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Raporty organizacyjne na temat "Atmospheric muon"

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Gogos, Jeremy Peter. An atmospheric muon neutrino disappearance measurement with the MINOS far detector. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/932867.

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Molina Bueno, Laura. Measurement of the Muon Atmospheric Production Depth with the Water Cherenkov Detectors of the Pierre Auger Observatory. Office of Scientific and Technical Information (OSTI), 2015. http://dx.doi.org/10.2172/1248227.

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Poirier, J. Calculation of Atmospheric Muons from Cosmic Gamma Rays. Office of Scientific and Technical Information (OSTI), 2005. http://dx.doi.org/10.2172/839832.

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Rahman, Aftabur Dipu. Atmospheric Neutrino Induced Muons in the MINOS Far Detector. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/902865.

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Trost, H. J. On the scattering of atmospheric muons in the rock above Soudan 2. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/5613495.

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Trost, H. J. On the scattering of atmospheric muons in the rock above Soudan 2. Office of Scientific and Technical Information (OSTI), 1992. http://dx.doi.org/10.2172/10132949.

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