Relevant bibliographies by topics / Cosmic air shower

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Cosmic air shower'

Author: Grafiati
Published: 4 June 2021
Last updated: 1 February 2022

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Journal articles on the topic "Cosmic air shower"

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Sanyal, S., B. Ghosh, SK Sarkar, A. Bhadra, A. Mukherjee, and N. Chaudhuri. "An Analysis of Cosmic Ray Air Showers for the Determination of Shower Age." Australian Journal of Physics 46, no. 4 (1993): 589. http://dx.doi.org/10.1071/ph930589.

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A sample of 8651 air showers in the size range 104 . 3_106 . 2 has been analysed to determine the distribution of the measured age in terms of (i) the number of showers in a specified size range, and (ii) the radial distances in individual showers. It is shown that the radial age distribution in an individual shower leads to an average shower age approximately the same as the prediction of the electron-photon cascade theory. The other results include a study of the variation of (i) shower age, as measured by the x2-minimisation technique, with shower size of vertically incident showers, and (ii) the measured electron density at any point with its radial distance from the shower axis, as a function of the age of a large shower group with very small spread in size. A comparison of similar measurements with relevant theory is also included.
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Haungs, A., W. D. Apel, J. C. Arteaga, T. Asch, A. F. Badea, L. Bähren, K. Bekk, et al. "Cosmic Ray Air Shower Detection with LOPES." Nuclear Physics B - Proceedings Supplements 175-176 (January 2008): 227–32. http://dx.doi.org/10.1016/j.nuclphysbps.2007.11.003.

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ARDOUIN, D., A. BELLETOILE, D. CHARRIER, R. DALLIER, L. DENIS, P. ESCHSTRUTH, T. GOUSSET, et al. "CODALEMA: A COSMIC RAY AIR SHOWER RADIO DETECTION EXPERIMENT." International Journal of Modern Physics A 21, supp01 (July 2006): 192–96. http://dx.doi.org/10.1142/s0217751x0603360x.

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The CODALEMA experimental device currently detects and characterizes the radio contribution of cosmic ray air showers : arrival directions and electric field topologies of radio transient signals associated to cosmic rays are extracted from the antenna signals. The measured rate, about 1 event per day, corresponds to an energy threshold around 5.1016eV. These results allow to determine the perspectives offered by the present experimental design for radiodetection of Ultra High Energy Cosmic Rays at a larger scale.
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Schröder, Frank G. "Air Shower Detection by Arrays of Radio Antennas." EPJ Web of Conferences 208 (2019): 15001. http://dx.doi.org/10.1051/epjconf/201920815001.

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Antenna arrays are beginning to make important contributions to high energy astroparticle physics supported by recent progress in the radio technique for air showers. This article provides an update to my more extensive review published in Prog. Part. Nucl. Phys. 93 (2017) 1. It focuses on current and planned radio arrays for atmospheric particle cascades, and briefly references to a number of evolving prototype experiments in other media, such as ice. While becoming a standard technique for cosmic-ray nuclei today, in future radio detection may drive the field for all type of primary messengers at PeV and EeV energies, including photons and neutrinos. In cosmic-ray physics accuracy becomes increasingly important in addition to high statistics. Various antenna arrays have demonstrated that they can compete in accuracy for the arrival direction, energy and position of the shower maximum with traditional techniques. The combination of antennas and particles detectors in one array is a straightforward way to push the total accuracy for high-energy cosmic rays for low additional cost. In particular the combination of radio and muon detectors will not only enhance the accuracy for the cosmic-ray mass composition, but also increase the gamma-hadron separation and facilitate the search for PeV and EeV photons. Finally, the radio technique can be scaled to large areas providing the huge apertures needed for ultra-high-energy neutrino astronomy.
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Bahmanabadi, Mahmud, Mehdi Khakian Ghomi, Farzaneh Sheidaei, and Jalal Samimi. "Galactic Anisotropy of Cosmic Ray Intensity Observed by an Air Shower Experiment." Publications of the Astronomical Society of Australia 23, no. 3 (2006): 129–34. http://dx.doi.org/10.1071/as06015.

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AbstractWe have monitored multi-TeV cosmic rays by a small air shower array in Tehran (35°43′ N, 51°20′ E, 1200 m = 890 g cm−2). More than 1.1 × 106 extensive air shower events were recorded. These observations enabled us to analyse sidereal variation of the galactic cosmic ray intensity. The observed sidereal daily variation is compared to the expected variation which includes the Compton–Getting effect due to the motion of the earth in the Galaxy. In addition to the Compton–Getting effect, an anisotropy has been observed which is due to a unidirectional anisotropy of cosmic ray flow along the Galactic arms.
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Wada, T., N. Ochi, T. Kitamura, W. Unno, M. Chikawa, Y. Kato, T. Konishi, et al. "Observation of time correlation in cosmic air shower network." Nuclear Physics B - Proceedings Supplements 75, no. 1-2 (March 1999): 330–32. http://dx.doi.org/10.1016/s0920-5632(99)00282-0.

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HUEGE, TIM, and HEINO FALCKE. "SIMULATIONS OF RADIO EMISSION FROM COSMIC RAY AIR SHOWERS." International Journal of Modern Physics A 20, no. 29 (November 20, 2005): 6831–33. http://dx.doi.org/10.1142/s0217751x05030223.

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Radio emission from cosmic ray air showers has the potential to become an additional, cost-effective observing technique for cosmic ray research, being largely complementary to the well-established particle detector and air fluorescence techniques. We present Monte Carlo simulations of radio emission from extensive air showers in the scheme of coherent geosynchrotron radiation from electron-positron pairs gyrating in the earth's magnetic field. Preliminary results of our simulations are the predicted frequency, primary particle energy, shower zenith angle, shower azimuth angle and polarization dependence of the radio emission. These properties can be directly related to data measured by LOPES and other experiments.
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WERNER, K., and O. SCHOLTEN. "Macroscopic treatment of radio emission from cosmic ray air showers based on shower simulations." Astroparticle Physics 29, no. 6 (July 2008): 393–411. http://dx.doi.org/10.1016/j.astropartphys.2008.04.004.

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Meyhandan, R., and R. W. Clay. "Improving the Angular Resolution of the Buckland Park Air Shower Array." Publications of the Astronomical Society of Australia 9, no. 1 (1991): 113–14. http://dx.doi.org/10.1017/s1323358000025121.

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AbstractAir showers initiated by primary cosmic rays and gamma rays produce shower fronts which are curved. However, the arrival directions of air shower events have normally been fitted assuming a planar shower front. We present a technique which takes the average shower front shape into account to assign an improved shower direction after a first analysis assuming a plane front. We then examine the resulting angular resolution of the Buckland Park array.
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KANG, DONGHWA, W. D. APEL, J. C. ARTEAGA, F. BADEA, K. BEKK, M. BERTAINA, J. BLÜMER, et al. "THE EXTENSIVE AIR SHOWER EXPERIMENT KASCADE-GRANDE." International Journal of Modern Physics: Conference Series 01 (January 2011): 132–39. http://dx.doi.org/10.1142/s2010194511000183.

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The extensive air shower experiment KASCADE-Grande (KArlsruhe Shower Core and Array DEtector and Grande array) is located on site of the Forschungszentrum Karlsruhe in Germany. The original KASCADE experiment consisted of a densely packed scintillator array with unshielded and shielded detectors for the measurement of the electromagnetic and muonic shower component independently, as well as muon tracking devices and a hadron calorimeter. The Grande array as an extension of KASCADE consists of 37 scintillation detector stations covering an area of 700×700 m2. The main goal for the combined measurements of KASCADE and Grande is the investigation of the energy spectrum and composition of primary cosmic rays in the energy range of 1016 to 1018 eV. In this paper an overview of the KASCADE-Grande experiment and recent results will be presented.
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Dissertations / Theses on the topic "Cosmic air shower"

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Hakmana, Witharana Sampath S. "Development of Cosmic Ray Simulation Program -- Earth Cosmic Ray Shower (ECRS)." Digital Archive @ GSU, 2007. http://digitalarchive.gsu.edu/phy_astr_diss/12.

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ECRS is a program for the detailed simulation of extensive air shower initiated by high energy cosmic ray particles. In this dissertation work, a Geant4 based ECRS simulation was designed and developed to study secondary cosmic ray particle showers in the full range of Earth's atmosphere. A proper atmospheric air density and geomagnetic field are implemented in order to correctly simulate the charged particles interactions in the Earth's atmosphere. The initial simulation was done for the Atlanta (33.460 N , 84.250 W) region. Four different types of primary proton energies (109, 1010, 1011 and 1012 eV) were considered to determine the secondary particle distribution at the Earth's surface. The geomagnetic field and atmospheric air density have considerable effects on the muon particle distribution at the Earth's surface. The muon charge ratio at the Earth's surface was studied with ECRS simulation for two different geomagnetic locations: Atlanta, Georgia, USA and Lynn Lake, Manitoba, Canada. The simulation results are shown in excellent agreement with the data from NMSU-WIZARD/CAPRICE and BESS experiments at Lynn Lake. At low momentum, ground level muon charge ratios show latitude dependent geomagnetic effects for both Atlanta and Lynn Lake from the simulation. The simulated charge ratio is 1.20 ± 0.05 (without geomagnetic field), 1.12 ± 0.05 (with geomagnetic field) for Atlanta and 1.22 ± 0.04 (with geomagnetic field) for Lynn Lake. These types of studies are very important for analyzing secondary cosmic ray muon flux distribution at the Earth's surface and can be used to study the atmospheric neutrino oscillations.
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張增 and Tsang Cheung. "Primary cosmic ray composition at 10 [to the power] 15--10 [to the power] 17eV studied from extensive air shower simulations." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1985. http://hub.hku.hk/bib/B31230593.

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Cheung, Tsang. "Primary cosmic ray composition at 10 [to the power] 15--10 [to the power] 17eV studied from extensive air shower simulations /." [Hong Kong : University of Hong Kong], 1985. http://sunzi.lib.hku.hk/hkuto/record.jsp?B12266176.

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Rol, Jan. "Characterization of monopole induced air showers using CORSIKA." Thesis, Uppsala universitet, Högenergifysik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-328049.

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In this thesis a characterization of air showers induced by magnetic monopoles is presented. Monopoles are predicted to exist and be accelerated to relativistic velocities. High energy monopoles traversing earth’s atmosphere continuously deposit energy, inducing an air shower. These air showers have been described based on simulations run in CORSIKA. It was found that monopole air showers are continuous; they plateau after the shower maximum, and have a large electromagnetic component. As such,they can easily be distinguished from normal cosmic rays and most other air shower sources. Very high energy photons and muons could induce similar showers but do not produce identical signals in track-following detectors such as IceCube.
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Chen, Chuxing. "Local atmospheric electricity and its possible application in high-energy cosmic ray air shower detection." Diss., The University of Arizona, 1989. http://hdl.handle.net/10150/184799.

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We have conducted an extensive experimental study on the subject of near ground atmospheric electricity. The main objective was to gain more understanding of this particular aspect of atmospheric phenomena, while testing the possible application to cosmic ray research. The results in atmospheric electricity show that there are certain patterns in ion grouping such as the size and lifetime. The average lifetime of ion group is 0.7 seconds and the average size is about 10 meters at our experimental site. Ultrahigh energy cosmic ray air showers should create sizable slow atmospheric electric pulses according to our theoretical calculations. Preliminary studies on air showers with total particle number N equal or greater than 10⁵ (10¹⁵ eV) have yielded strong evidence that slow atmospheric current pulses are associated with air showers. The theory and the experiment agree with each other fairly well when we average over large numbers of events. With our current experimental arrangement, when the air shower exceeds a certain size, the system response saturates. Therefore it is extremely desirable in future research that the counter array be designed for a much higher threshold level, since this prototype experiment indicates that interesting data would be obtained. Another reason for further experimental research being directed toward ultrahigh energy, e.g., N ≥ 10⁷ (10¹⁷ eV) and higher, is to establish a calibration of the slow atmospheric electric signals generated by cosmic rays as a function of primary cosmic ray energy and core location. This type of slow atmospheric electric signal, if fully understood and calibrated, offers a new and potentially less expensive technique to observe ultrahigh energy cosmic ray events, which hold some fundamental keys to the knowledge of the universe on a large scale.
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Palmieri, Nunzia [Verfasser], and J. [Akademischer Betreuer] Blümer. "Determination of energy and mass of cosmic rays using air shower radio emission / Nunzia Palmieri. Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2012. http://d-nb.info/1032946709/34.

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Maurel, Detlef [Verfasser], and J. [Akademischer Betreuer] Blümer. "Mass composition of ultra-high energy cosmic rays based on air shower universality / Detlef Maurel. Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2013. http://d-nb.info/1044956178/34.

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Stapleton, James C. "Ultra-High Energy Cosmic Rays: Composition, Early Air Shower Interactions, and Xmax Skewness." The Ohio State University, 2015. http://rave.ohiolink.edu/etdc/view?acc_num=osu1431044195.

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Bridgeman, Ariel [Verfasser], and J. [Akademischer Betreuer] Blümer. "Determining the Mass Composition of Ultra-high Energy Cosmic Rays Using Air Shower Universality / Ariel Bridgeman ; Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2018. http://d-nb.info/1166234266/34.

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Schoo, Sven [Verfasser], and J. [Akademischer Betreuer] Blümer. "Energy Spectrum and Mass Composition of Cosmic Rays and How to Publish Air-Shower Data / Sven Schoo. Betreuer: J. Blümer." Karlsruhe : KIT-Bibliothek, 2016. http://d-nb.info/110632997X/34.

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Books on the topic "Cosmic air shower"

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Rao, M. V. S. Extensive air showers. Singapore: World Scientific, 1998.

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Workshop on Observing Giant Cosmic Ray Air Showers From >10²⁰ eV Particles From Space (1997 College Park, Maryland). Workshop on Observing Giant Cosmic Ray Air Showers From >10²⁰ eV Particles From Space: College Park, Maryland, November, 1997. Edited by Krizmanic John F, Ormes J. F. 1939-, and Streitmatter Robert E. Woodbury, New York: AIP, 1998.

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Extensive air showers: High energy phenomena and astrophysical aspects : a tutorial reference manual and data book. Heidelberg: Springer, 2010.

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United States. National Aeronautics and Space Administration., ed. "Cosmic ray air shower measurement from space": Final report, NAS 8-38609 ... (1/18/96 - 11/17/96). [Washington, DC: National Aeronautics and Space Administration, 1997.

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Extensive Air Showers. World Scientific Publishing Company, 1997.

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(Editor), Michael Albrow, and Rajendran Raja (Editor), eds. Hadronic Shower Simulation Workshop (AIP Conference Proceedings / High Energy Physics). American Institute of Physics, 2007.

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(Editor), John F. Krizmanic, Jonathan F. Ormes (Editor), and Robert E. Streitmatter (Editor), eds. Workshop on Observing Giant Air Showers from >10/20 eV Particles from Space: Center for Adult Education, University of Maryland, 13-15 November 1997. (AIP Conference Proceedings). American Institute of Physics, 1998.

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(Editor), Brenda L. Dingus, David B. Kieda (Editor), and Michael H. Salamon (Editor), eds. 26th International Cosmic Ray Conference: ICRC XXVI, Invited Rapporteur, and Highlight Papers, Salt Lake City, Utah, USA 17-25 August 1999 (AIP Conference Proceedings / Astronomy and Astrophysics). American Institute of Physics, 2000.

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Book chapters on the topic "Cosmic air shower"

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Clark, George W. "Air Shower Experiments at MIT." In Early History of Cosmic Ray Studies, 239–46. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5434-2_24.

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Acharya, B. S., P. N. Bhat, S. G. Khairatkar, M. R. Rajeev, M. V. S. Rao, S. Sinha, K. Sivaprasad, et al. "UHE Gamma Ray Observations with the KGF Air Shower Array." In Cosmic Gamma Rays, Neutrinos, and Related Astrophysics, 235–43. Dordrecht: Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0921-2_16.

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Boruah, K., S. Zamal, M. Rahman, B. Tiru, U. Sarma, and P. K. Boruah. "Design of a Small Cosmic Ray Air Shower Array to Study Atmospheric Effects." In Springer Proceedings in Physics, 439–45. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-25619-1_67.

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Grieder, Peter K. F. "Primary Cosmic Radiation and Astrophysical Aspects." In Exentsive Air Showers and High Energy Phenomena, 479–588. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76941-5_11.

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Zilles, Anne. "Introduction to Cosmic Rays and Extensive Air Showers." In Emission of Radio Waves in Particle Showers, 1–13. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-63411-1_1.

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Sokolsky, Pierre. "The Extensive Air Shower." In Introduction to Ultrahigh Energy Cosmic Ray Physics, 19–35. CRC Press, 2018. http://dx.doi.org/10.1201/9780429499654-3.

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"COSMIC RAY SOURCES." In Extensive Air Showers, 303–14. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789812817211_0010.

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"EXTREMELY HIGH ENERGY COSMIC RAYS." In Extensive Air Showers, 205–39. WORLD SCIENTIFIC, 1998. http://dx.doi.org/10.1142/9789812817211_0007.

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Sokolsky, Pierre, and Gordon Thomson. "Extensive Air Showers." In Introduction to Ultrahigh Energy Cosmic Ray Physics, 21–25. CRC Press, 2020. http://dx.doi.org/10.1201/9780429055157-2.

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Chiari, Sophie. "Othello: Shakespeare’s À bout de souffle." In Shakespeare's Representation of Weather, Climate and Environment, 111–49. Edinburgh University Press, 2019. http://dx.doi.org/10.3366/edinburgh/9781474442527.003.0005.

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Chapter 4 shows that Othello (1604) is a play obsessed with breath and wind, a cosmological piece in which climate and air coalesce to make the Moor the victim of his own humours as much as of the satanic Iago. The importance given to cosmic elements as well as to the planets and their influence on men and women’s behaviour serves to elevate and magnify a play sometimes wrongly reduced to the genre of the domestic tragedy. Besides, the recurring imagery related to pneuma turns the scene into a dark carnival with its frightening disaster at the end epitomised by the image of the ‘tragic loading of [the] bed’ (5.2.374). If a providential tempest preserves Cyprus from the assaults of the Turkish fleet, Othello and Desdemona’s love quickly becomes a highly tempestuous affair that ends in tragic suffocation.
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Conference papers on the topic "Cosmic air shower"

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Alania, Marco, Ignacio J. Araya, Adolfo V. Chamorro Gómez, Humberto Martínez Huerta, Alejandra Parra Flores, Johannes Knapp, Carlos Javier Solano Salinas, Jose Bellido, David Wahl, and Oscar Saavedra. "Air Shower Simulations." In COSMIC RAYS AND ASTROPHYSICS: Proceedings of the 3rd School on Cosmic Rays and Astrophysics. AIP, 2009. http://dx.doi.org/10.1063/1.3141351.

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Buckland, Isaac, and Douglas Bergman. "CHASM (CHerenkov Air Shower Model): Simulating the Cherenkov Profiles of Cosmic Ray Air Showers." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0234.

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McIntosh, Gordon. "Cosmic Ray Air Shower Lateral Coincidence." In 2016 Academic High Altitude Conference. Iowa State University Digital Press, 2017. http://dx.doi.org/10.31274/ahac.5565.

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McIntosh, Gordon. "Cosmic Ray Air Shower Lateral Coincidences." In 2015 Academic High Altitude Conference. Iowa State University Digital Press, 2015. http://dx.doi.org/10.31274/ahac.5569.

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Werner, Klaus, and Tanguy Pierog. "Extended Air Shower Simulations Using EPOS." In C2CR07: COLLIDERS TO COSMIC RAYS. AIP, 2007. http://dx.doi.org/10.1063/1.2775903.

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Krolik, Karolina, Aneta Djakonow, Zbigniew Plebaniak, Marika Przybylak, Jacek Szabelski, and Lawrence Wiencke. "Cherenkov Light from Horizontal Air Shower." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0321.

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Reininghaus, Maximilian, Ralf Ulrich, and Tanguy Pierog. "Air shower genealogy for muon production." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0463.

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Gaisser, Thomas K. "Air shower modelling." In WORKSHOP ON OBSERVING GIANT COSMIC RAY AIR SHOWERS FROM >1020 eV Particles from Space. ASCE, 1998. http://dx.doi.org/10.1063/1.56145.

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Balagopal V., Aswathi, Andreas Haungs, Tim Huege, Max Renschler, Frank G. Schröder, and Anne Zilles. "Frequency-optimised radio air arrays for air-shower detection." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0184.

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Pont, Bjarni, Pedro Abreu, Marco Aglietta, Justin M. Albury, Ingomar Allekotte, Alejandro Almela, Jaime Alvarez-Muniz, et al. "The depth of the shower maximum of air showers measured with AERA." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0387.

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