Готові списки джерел за темами / Cosmic ray; detector; anisotropy

Добірка наукової літератури з теми "Cosmic ray; detector; anisotropy"

Автор: Grafiati
Опубліковано: 10 грудня 2022
Оновлено: 28 січня 2023

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Статті в журналах з теми "Cosmic ray; detector; anisotropy"

1

Янчуковский, Валерий, Valery Yanchukovsky, Владислав Григорьев, Vladislav Grigoryev, Гермоген Крымский, Germogen Krymsky, Василий Кузьменко, Vasiliy Kuzmenko, Антон Молчанов, and Anton Molchanov. "Receiving vectors of muon telescope of cosmic ray station Novosibirsk." Solar-Terrestrial Physics 2, no. 1 (June 1, 2016): 103–19. http://dx.doi.org/10.12737/19883.

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Анотація:
The method of receiving vectors allows us to determine cosmic ray anisotropy at every moment of time. Also, the method makes it possible to study fast anisotropy fluctuations related to the interplanetary medium dynamics. Receiving vectors have been calculated earlier for neutron monitors and muon telescopes. However, most muon telescopes of the network of cosmic ray stations for which calculations were made does not operate now. In recent years, new, improved detectors have been developed. Unfortunately, the use of them is limited because of the absence of receiving coefficients. These detectors include a matrix telescope in Novosibirsk. Therefore, receiving vector components for muon telescopes of observation cosmic ray station Novosibirsk have been defined. Besides, design features of the facility, its orientation, and directional diagram depending on zenith and azimuth angles were taken into account. Also, for the system of telescopes, we allowed for coupling coefficients found experimentally by the test detector.
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2

Kawata, K., A. di Matteo, T. Fujii, D. Ivanov, C. C. H. Jui, J. P. Lundquist, J. N. Matthews, et al. "TA Anisotropy Summary." EPJ Web of Conferences 210 (2019): 01004. http://dx.doi.org/10.1051/epjconf/201921001004.

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The Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) detector in the northern hemisphere. It consists of an array of 507 surface detectors (SD) covering a total 700 km2 and three fluorescence detector stations overlooking the SD array. In this proceedings, we summarize recent results on the search for directional anisotropy of UHECRs using the latest dataset collected by the TA SD array. We obtained hints of the anisotropy of the UHECRs in the northern sky from the various analyses.
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3

Янчуковский, Валерий, Valery Yanchukovsky, Владислав Григорьев, Vladislav Grigoryev, Гермоген Крымский, Germogen Krymsky, Василий Кузьменко, Vasiliy Kuzmenko, Антон Молчанов, and Anton Molchanov. "Receiving vectors of muon telescope of cosmic ray station “Novosibirsk”." Solnechno-Zemnaya Fizika 2, no. 1 (March 17, 2016): 76–87. http://dx.doi.org/10.12737/16762.

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Анотація:
The method of receiving vectors allows us to determine cosmic ray anisotropy at each moment. Also, the method makes it possible to study fast anisotropy fluctuations related to the interplanetary medium dynamics. Receiving vectors have been calculated earlier for neutron monitors and muon telescopes. However, the most of muon telescopes of the network of cosmic ray stations for which calculations were made does not operate now. In recent years, new improved detectors appeared. Unfortunately, the use of them is limited because of absence of receiving coefficients. These detectors include the matrix telescope in Novosibirsk. Therefore, components of receiving vector for muon telescopes of observation cosmic ray station “Novosibirsk” have been defined. Besides, design features of the facility, its orientation, and directional diagram depending on zenith and azimuth angles were taken into account. Also, for the system of telescopes, we allowed for coupling coefficients found experimentally using the test detector.
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4

Hall, D. L., M. L. Duldig, and J. E. Humble. "The North–South Anisotropy and the Radial Density Gradient of Galactic Cosmic Rays at 1 AU." Publications of the Astronomical Society of Australia 12, no. 2 (August 1995): 153–58. http://dx.doi.org/10.1017/s1323358000020191.

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AbstractThe radial density gradient (Gr) of Galactic cosmic rays in the ecliptic plane points outward from the Sun. This indicates an increasing density of cosmic ray particles beyond the Earth’s orbit. Due to this gradient and the direction of the Sun’s interplanetary magnetic field (IMF) above and below the IMF wavy neutral sheet, there exists an anisotropic flow of cosmic ray particles approximately perpendicular to the ecliptic plane (i.e. in the direction parallel to BIMF × Gr). This effect is called the north–south anisotropy (ξNS) and manifests as a diurnal variation in sidereal time in the particle intensity recorded by a cosmic ray detector. By analysing the yearly averaged sidereal diurnal variation recorded by five neutron monitors and six muon telescopes from 1957 to 1990, we have deduced probable values of the average rigidity spectrum and magnitude of ξNS. Furthermore, we have used determined yearly amplitudes of ξNS to infer the magnitude of Gr for particles with rigidities in excess of 10 GV.
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5

Munakata, Kazuoki. "Probing the heliosphere with the directional anisotropy of galactic cosmic-ray intensity." Proceedings of the International Astronomical Union 7, S286 (October 2011): 185–94. http://dx.doi.org/10.1017/s1743921312004826.

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AbstractBecause of the large detector volume that can be deployed, ground-based detectors remain state-of-the-art instrumentation for measuring high-energy galactic cosmic-rays (GCRs). This paper demonstrates how useful information can be derived from observations of the directional anisotropy of the high-energy GCR intensity, introducing the most recent results obtained from the ground-based observations. The anisotropy observed with the global muon detector network (GMDN) provides us with a unique information of the spatial gradient of the GCR density which reflects the large-scale magnetic structure in the heliosphere. The solar cycle variation of the gradient gives an important information on the GCR transport in the heliosphere, while the short-term variation of the gradient enables us to deduce the large-scale geometry of the magnetic flux rope and the interplanetary coronal mass ejection (ICME). Real-time monitoring of the precursory anisotropy which has often been observed at the Earth preceding the arrival of the ICME accompanied by a strong shock may provide us with useful tools for forecasting the space weather with a long lead time. The solar cycle variation of the Sun's shadow observed in the TeV GCR intensity is also useful for probing the large-scale magnetic structure of the solar corona.
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6

Munakata, K., M. Kozai, C. Kato, Y. Hayashi, R. Kataoka, A. Kadokura, M. Tokumaru, et al. "Large-amplitude Bidirectional Anisotropy of Cosmic-Ray Intensity Observed with Worldwide Networks of Ground-based Neutron Monitors and Muon Detectors in 2021 November." Astrophysical Journal 938, no. 1 (October 1, 2022): 30. http://dx.doi.org/10.3847/1538-4357/ac91c5.

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Abstract We analyze the cosmic-ray variations during a significant Forbush decrease observed with worldwide networks of ground-based neutron monitors and muon detectors during 2021 November 3–5. Utilizing the difference between primary cosmic-ray rigidities monitored by neutron monitors and muon detectors, we deduce the rigidity spectra of the cosmic-ray density (or omnidirectional intensity) and the first- and second-order anisotropies separately for each hour of data. A clear two-step decrease is seen in the cosmic-ray density with the first ∼2% decrease after the interplanetary shock arrival followed by the second ∼5% decrease inside the magnetic flux rope (MFR) at 15 GV. Most strikingly, a large bidirectional streaming along the magnetic field is observed in the MFR with a peak amplitude of ∼5% at 15 GV, which is comparable to the total density decrease inside the MFR. The bidirectional streaming could be explained by adiabatic deceleration and/or focusing in the expanding MFR, which have stronger effects for pitch angles near 90°, or by selective entry of GCRs along a leg of the MFR. The peak anisotropy and density depression in the flux rope both decrease with increasing rigidity. The spectra vary dynamically, indicating that the temporal variations of density and anisotropy appear different in neutron monitor and muon detector data.
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7

Petrera, Sergio. "Recent results from the Pierre Auger Observatory." EPJ Web of Conferences 208 (2019): 08001. http://dx.doi.org/10.1051/epjconf/201920808001.

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In this paper some recent results from the Pierre Auger Collaboration are presented. These are the measurement of the energy spectrum of cosmic rays over a wide range of energies (1017.5 to above 1020 eV), studies of the cosmic-ray mass composition with the fluorescence and surface detector of the Observatory, the observation of a large-scale anisotropy in the arrival direction of cosmic rays above 8 × 1018 eV and indications of anisotropy at intermediate angular scales above 4 × 1019 eV. The astrophysical implications of the spectrum and composition results are also discussed. Finally the progress of the upgrade of the Observatory, AugerPrime is presented.
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8

Takeishi, Ryuji. "Observation of ultra-high energy cosmic rays with the Telescope Array experiment." EPJ Web of Conferences 182 (2018): 02122. http://dx.doi.org/10.1051/epjconf/201818202122.

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The origin of ultra-high energy cosmic rays (UHECRs) has been a longstanding mystery. The Telescope Array (TA) is the largest experiment in the northern hemisphere observing UHECR in Utah, USA. It aims to reveal the origin of UHECR by studying the energy spectrum, mass composition and anisotropy of cosmic rays. TA is a hybrid detector comprised of three air fluorescence stations which measure the fluorescence light induced from cosmic ray extensive air showers, and 507 surface scintillator counters which sample charged particles from air showers on the ground. We present the cosmic ray spectrum observed with the TA experiment. We also discuss our results from measurement of the mass composition. In addition, we present the results from the analysis of anisotropy, including the excess of observed events in a region of the northern sky at the highest energy. Finally, we introduce the TAx4 experiment which quadruples TA, and the TA low energy extension (TALE) experiment.
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9

TAMBURRO, ALESSIO. "MEASUREMENTS OF COSMIC RAYS WITH ICETOP/ICECUBE: STATUS AND RESULTS." Modern Physics Letters A 27, no. 39 (December 13, 2012): 1230038. http://dx.doi.org/10.1142/s0217732312300388.

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The IceCube Observatory at the South Pole is composed of a cubic kilometer scale neutrino telescope buried beneath the icecap and a square-kilometer surface water Cherenkov tank detector array known as IceTop. The combination of the surface array with the in-ice detector allows the dominantly electromagnetic signal of air showers at the surface and their high-energy muon signal in the ice to be measured in coincidence. This ratio is known to carry information about the nuclear composition of the primary cosmic rays. This paper reviews the recent results from cosmic-ray measurements performed with IceTop/IceCube: energy spectrum, mass composition, anisotropy, search for PeV γ sources, detection of high energy muons to probe the initial stages of the air shower development, and study of transient events using IceTop in scaler mode.
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10

Kyratzis, Dimitrios. "Overview of the HERD space mission." Physica Scripta 97, no. 5 (April 12, 2022): 054010. http://dx.doi.org/10.1088/1402-4896/ac63fc.

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Abstract The High Energy cosmic Radiation Detector (HERD) is a prominent space-borne instrument to be installed on-board the Chinese Space Station (CSS) around 2027, resulting from a collaboration among Chinese and European institutions. Primary scientific goals of HERD include: precise measurements of the cosmic ray (CR) energy spectra and mass composition at energies up to few PeV, electron/positron spectra up to tens of TeV, CR anisotropy, gamma ray astronomy and transient studies, along with indirect searches for Dark Matter candidates. The detector is configured to accept incident particles from both its top and four lateral sides. Owing to its pioneering design, more than one order of magnitude increase in geometric acceptance is foreseen, with respect to previous and ongoing experiments. HERD is conceived around a deep (∼55 X 0, 3 λ I ) 3D cubic calorimeter (CALO), forming an octagonal prism. Fiber Trackers (FiTs) are instrumented on all active sides, with a Plastic Scintillator Detector (PSD) covering the calorimeter and tracker. Ultimately, a Silicon Charge Detector (SCD) envelops the above-stated sub-detectors, while a Transition Radiation Detector (TRD) is instrumented on one of its lateral faces, for energy calibration in the TeV scale. This work illustrates HERD’s latest advancements and scientific objectives along with an overview of upcoming activities.
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Дисертації з теми "Cosmic ray; detector; anisotropy"

1

Guillian, G., J. Hosaka, K. Ishihara, J. Kameda, Y. Koshio, A. Minamino, C. Mitsuda, et al. "Observation of the anisotropy of 10 TeV primary cosmic ray nuclei flux with the Super-Kamiokande-I detector." American Physical Society, 2007. http://hdl.handle.net/2237/8844.

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2

Grigat, Marius [Verfasser]. "Large scale anisotropy studies of ultra high energy cosmic rays using data taken with the surface detector of the Pierre Auger Observatory / Marius Grigat." Aachen : Hochschulbibliothek der Rheinisch-Westfälischen Technischen Hochschule Aachen, 2011. http://d-nb.info/1018201106/34.

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3

Smith, Andrew Geoffrey Kent. "Cosmic ray anisotropy at high energies." Title page, contents and overview only, 1996. http://hdl.handle.net/2440/18616.

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Title page, contents and abstract only. The complete thesis in print form is available from the University Library.
Thesis (Ph.D.)--University of Adelaide, Dept. of Physics and Mathematical Physics, 1996
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4

Graham, Lilian Joan. "Ultra high energy gamma ray point sources and cosmic ray anisotropy." Thesis, Durham University, 1994. http://etheses.dur.ac.uk/5594/.

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The experimental set-up at the Baksan Air Shower Array, used to detect air showers above ~0.2xl0(^14)eV, is described. An estimation of the angular resolution using the cosmic ray shadow of the Sun and the Moon gives a value of ~2.5˚ which is consistent with previous estimates from Monte-Carlo simulations. Using data from this array covering 1985-1992, a search is made for 7-ray emission from 18 candidate sources. Upper limits to the flux from these sources are stated in all cases. A periodicity search is made on data for which the excess for a single transit of a particular source is above 3(7. The results of this periodicity analysis on such days points to 4 possible observations of pulsed emission at the 95% confidence level. These are 4U0115+63 on 19.03.89, PSR19534-29 on 12.02.85, 1E2259+586 on 01.08.91 and PSR0655+64 on 12.08.89. Without confirmation from other groups however the findings are not significant enough to stand alone. A harmonic analysis has been performed on the 8 years of data and after pressure corrections and a Farley & Storey analysis to eradicate any spurious sidereal variations we find negligible evidence of 2nd or 3rd harmonic but a 1st harmonic amplitude and phase of (12.7 ±1.2) x 10(^-4) at 23.1 ± 0.3hr right ascension. When one takes into account the cosϐ effect on the sidereal anisotropy this value becomes 17.4±1.6xl0(^-4).Future developments and improvements to be undertaken at BASA, including the building of a muon detector, are outlined.
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5

Boghrat, Pedram. "Search for ultra high energy cosmic ray anisotropy with Auger." Diss., Restricted to subscribing institutions, 2008. http://proquest.umi.com/pqdweb?did=1750728181&sid=5&Fmt=2&clientId=1564&RQT=309&VName=PQD.

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6

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

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7

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

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8

梁淦章 and Kam-cheung Leung. "Muon detector array to discriminate gamma-ray eas at mountainaltitude." Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1995. http://hub.hku.hk/bib/B31213339.

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9

Gurtner, Maria [Verfasser]. "Cosmic ray anisotropy study with the AMANDA Neutrino Telescope / Maria Gurtner." Wuppertal : Universitätsbibliothek Wuppertal, 2013. http://d-nb.info/1046604953/34.

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10

Leung, Kam-cheung. "Muon detector array to discriminate gamma-ray eas at mountain altitude /." Hong Kong : University of Hong Kong, 1995. http://sunzi.lib.hku.hk/hkuto/record.jsp?B17092280.

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Книги з теми "Cosmic ray; detector; anisotropy"

1

Howell, Leonard W. Estimating cosmic-ray spectral parameters from simulated detector responses with detector design implications. MSFC, Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 2001.

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2

Evans, Tom. A search for the dipole anisotropy of the cosmic X-ray background. [Washington, D.C.?: National Aeronautics and Space Administration, 1992.

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3

Peter, Meyer, and George C. Marshall Space Flight Center., eds. Cosmic Ray Nuclei (CRN) detector investigation. Chicago, Ill: University of Chicago, 1991.

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4

George C. Marshall Space Flight Center., ed. Estimating cosmic-ray spectral parameters from simulated detector responses with detector design implications. MSFC, Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 2001.

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5

George C. Marshall Space Flight Center., ed. Estimating cosmic-ray spectral parameters from simulated detector responses with detector design implications. MSFC, Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 2001.

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6

Estimating cosmic-ray spectral parameters from simulated detector responses with detector design implications. MSFC, Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 2001.

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7

Cosmic ray positron research and silicon track detector development: Final technical report. Washington, D.C: National Aeronautics and Space Administration, Space Physics Division, 1990.

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8

P, Wefel J., and United States. National Aeornautics and Space Administration. Space Physics Division., eds. Cosmic ray positron research and silicon track detector development: Final technical report. Washington, D.C: National Aeronautics and Space Administration, Space Physics Division, 1990.

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9

George C. Marshall Space Flight Center., ed. A recommended procedure for estimating the cosmic-ray spectral parameter of a simple power law with applications to detector design. MSFC, Ala: National Aeronautics and Space Administration, Marshall Space Flight Center, 2001.

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Частини книг з теми "Cosmic ray; detector; anisotropy"

1

Forbush, Scott E. "Cosmic ray diurnal anisotropy 1937–1972." In Cosmic Rays, the Sun and Geomagnetism: The Works of Scott E. Forbush, 447–55. Washington, D. C.: American Geophysical Union, 1993. http://dx.doi.org/10.1029/sp037p0447.

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2

Sekido, Yataro. "Intensity and Anisotropy of Cosmic Rays." In Early History of Cosmic Ray Studies, 187–206. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5434-2_19.

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3

Aad, G., B. Abbott, J. Abdallah, A. A. Abdelalim, A. Abdesselam, O. Abdinov, B. Abi, et al. "Studies of the performance of the ATLAS detector using cosmic-ray muons." In The Performance of the ATLAS Detector, 239–74. Berlin, Heidelberg: Springer Berlin Heidelberg, 2011. http://dx.doi.org/10.1007/978-3-642-22116-3_7.

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4

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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5

Forbush, Scott E. "A variation, with a period of two solar cycles, in the cosmic-ray diurnal anisotropy." In Cosmic Rays, the Sun and Geomagnetism: The Works of Scott E. Forbush, 413–15. Washington, D. C.: American Geophysical Union, 1993. http://dx.doi.org/10.1029/sp037p0413.

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6

Duggal, S. P., S. E. Forbush, and M. A. Pomerantz. "The variations with a period of two solar cycles in the cosmic ray diurnal anisotropy for the nucleonic component." In Cosmic Rays, the Sun and Geomagnetism: The Works of Scott E. Forbush, 439–45. Washington, D. C.: American Geophysical Union, 1993. http://dx.doi.org/10.1029/sp037p0439.

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7

Forbush, Scott E. "Variations with a period of two solar cycles in the cosmic-ray diurnal anisotropy and the superposed variations correlated with magnetic activity." In Cosmic Rays, the Sun and Geomagnetism: The Works of Scott E. Forbush, 421–38. Washington, D. C.: American Geophysical Union, 1993. http://dx.doi.org/10.1029/sp037p0421.

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8

Sokolsky, Pierre. "Anisotropy." In Introduction to Ultrahigh Energy Cosmic Ray Physics, 103–14. CRC Press, 2018. http://dx.doi.org/10.1201/9780429499654-8.

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9

Sokolsky, Pierre, and Gordon Thomson. "Searches for Anisotropy." In Introduction to Ultrahigh Energy Cosmic Ray Physics, 89–97. CRC Press, 2020. http://dx.doi.org/10.1201/9780429055157-9.

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10

Dröge, W., B. Heber, M. S. Potgieter, G. P. Zank, and R. A. Mewaldt. "A Cosmic Ray Detector for an Interstellar Probe." In The Outer Heliosphere: The Next Frontiers, Proceedings of the COSPAR Colloquium, 471–74. Elsevier, 2001. http://dx.doi.org/10.1016/s0964-2749(01)80107-4.

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Тези доповідей конференцій з теми "Cosmic ray; detector; anisotropy"

1

Zhezher, Yana, Grigory Rubtsov, Pierre Sokolsky, and Sergey Troitsky. "Anisotropy in the mass composition from the Telescope Array Surface Detector data." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.358.0494.

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2

Nonaka, Toshiyuki. "Anisotropy search in Energy distribution in Northern hemisphere using Telescope Array Surface Detector data." In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0507.

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3

Nakamura, Yoshiaki. "The anisotropy of cosmic rays observed by the Tibet air shower array and muon detector array." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0365.

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4

Munakata, K. "North-south anisotropy of galactic cosmic rays observed with the Global Muon Detector Network (GMDN)." In The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0056.

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5

Nonaka, Toshiyuki, Rasha Abbasi, Tareq Abu-Zayyad, Monica Allen, Yuto Arai, Ryuhei Arimura, Elliott Barcikowski, et al. "Anisotropy search in the Ultra High Energy Cosmic Ray Spectrum in the Northern Hemisphere using latest data obtained with Telescope Array surface detector." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0344.

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6

Cho, Wooram, Eunho Lee, and Hang Bae Kim. "Analysis of anisotropy of ultrahigh energy cosmic ray arrival direction and energy spectrum detected by Telescope array experiment." In 36th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.358.0221.

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7

Al Samarai, Imen. "Indications of anisotropy at large angular scales in the arrival directions of cosmic rays detected at the Pierre Auger Obser." In The 34th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.236.0372.

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8

Nonaka, Toshiyuki. "Anisotropy Search in Energy Distribution in the Northern Hemisphere Using the Telescope Array Surface Detector Data." In Proceedings of 2016 International Conference on Ultra-High Energy Cosmic Rays (UHECR2016). Journal of the Physical Society of Japan, 2018. http://dx.doi.org/10.7566/jpscp.19.011009.

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9

Tkachev, Igor, T. Fujii, D. Ivanov, C. C. H. Jui, K. Kawata, J. H. Kim, M. Yu Kuznetsov, et al. "Telescope Array anisotropy summary." In 37th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.395.0392.

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10

Troitsky, Sergey, Masaki Fukushima, Daisuke Ikeda, Dmitri Ivanov, Kazumasa Kawata, Eiji Kido, Jon Paul Lundquist, et al. "Telescope Array anisotropy summary." In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0548.

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Звіти організацій з теми "Cosmic ray; detector; anisotropy"

1

Collier, Michael. Assembly Manual for the Berkeley Lab Cosmic Ray Detector. Office of Scientific and Technical Information (OSTI), December 2002. http://dx.doi.org/10.2172/809887.

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2

Twitty, Colleen, and Howard Matis. Guide to using the Berkeley Lab Cosmic Ray Detector. Office of Scientific and Technical Information (OSTI), June 2000. http://dx.doi.org/10.2172/767637.

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3

Twitty, Colleen, Fred Bieser, and Howard Matis. Tips to assemble the Berkeley Lab Cosmic Ray Detector. Office of Scientific and Technical Information (OSTI), June 2000. http://dx.doi.org/10.2172/768482.

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4

Cristinziani, Markus. Search for Antimatter with the AMS Cosmic Ray Detector. Office of Scientific and Technical Information (OSTI), March 2003. http://dx.doi.org/10.2172/812975.

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5

Beall, Erik B. Cosmic ray muon charge ratio in the MINOS far detector. Office of Scientific and Technical Information (OSTI), December 2005. http://dx.doi.org/10.2172/892438.

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6

Ospanov, Rustem, and Karol Lang. Alignment of the Near Detector scintillator modules using cosmic ray muons. Office of Scientific and Technical Information (OSTI), May 2008. http://dx.doi.org/10.2172/933210.

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7

Plunkett, Robert, and Jennifer Thomas. Proposal for a Cosmic Ray Veto Shield for the MINOS Far Detector. Office of Scientific and Technical Information (OSTI), June 2002. http://dx.doi.org/10.2172/1155722.

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8

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

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9

Fukazawa, Y. Development of Low-noise Double-sided Silicon Strip Detector for Cosmic Soft Gamma-ray Compton Camera. Office of Scientific and Technical Information (OSTI), April 2005. http://dx.doi.org/10.2172/839892.

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10

Morgan, J. F., T. B. Gosnell, S. J. Luke, D. E. Archer, R. T. Lochner, I. M. Frank, S. G. Prussin, B. J. Quiter, and D. H. Chivers. Development of a Detector to Measure the Angular Dependence of the Cosmic Ray Induced Neutron Background Flux at Ground Level. Office of Scientific and Technical Information (OSTI), January 2002. http://dx.doi.org/10.2172/15003244.

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