Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array
The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the showe...
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| Veröffentlicht in: | JETP letters 2019, Vol.109 (9), p.559-563 |
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| creator | Glushkov, A. V. Saburov, A. V. |
| description | The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of (1–30) × 10
17
eV changes from middle nuclei to a purely proton composition. |
| doi_str_mv | 10.1134/S0021364019090091 |
| format | Article |
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17
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17
eV changes from middle nuclei to a purely proton composition.</description><subject>Arrays</subject><subject>Astrophysics and Cosmology</subject><subject>Atomic</subject><subject>Biological and Medical Physics</subject><subject>Biophysics</subject><subject>Composition</subject><subject>Cosmic ray showers</subject><subject>Cosmic rays</subject><subject>Detectors</subject><subject>Flux density</subject><subject>Molecular</subject><subject>Muons</subject><subject>Nuclei (nuclear physics)</subject><subject>Optical and Plasma Physics</subject><subject>Particle and Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Information Technology</subject><subject>Solid State Physics</subject><subject>Spintronics</subject><issn>0021-3640</issn><issn>1090-6487</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1UMtOwzAQtBBIlMIHcLPEOeB1nDg-Rm15SK2QKCBxihzXbtOSuNgOqFe-nIQicUCcdnd2ZlY7CJ0DuQSI2dWcEApxyggIIggRcIAG0HVRyjJ-iAb9Our3x-jE-zUhAFnMB-hzJr3HI1tvra9CZRtsTTf6ulL4Qe48_qjCCk8a7ZaV9liW9l1jIMCxfsa5UtYtqmaJg8VhpfFYBomNs_X3NGs7u7EOWgXrfG_coy9y0wa_wZN8jnPn5O4UHRn56vXZTx2ip-vJ4-g2mt7f3I3yaaQgBYiMkXGiCRMsI6LMFpSz7k1aEsq5UFm2EKVSHcoTJjMBhsokVjFNTWlAJgLiIbrY-26dfWu1D8Xatq7pThaUJpxywrKeBXuWctZ7p02xdVUt3a4AUvRRF3-i7jR0r_Edt1lq9-v8v-gLe4R9xA</recordid><startdate>2019</startdate><enddate>2019</enddate><creator>Glushkov, A. V.</creator><creator>Saburov, A. V.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>2019</creationdate><title>Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array</title><author>Glushkov, A. V. ; Saburov, A. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c1611-ffa35e0494809b8d2740912b02779c88d9bccd27754a891f2a53c326fbf1a5913</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Arrays</topic><topic>Astrophysics and Cosmology</topic><topic>Atomic</topic><topic>Biological and Medical Physics</topic><topic>Biophysics</topic><topic>Composition</topic><topic>Cosmic ray showers</topic><topic>Cosmic rays</topic><topic>Detectors</topic><topic>Flux density</topic><topic>Molecular</topic><topic>Muons</topic><topic>Nuclei (nuclear physics)</topic><topic>Optical and Plasma Physics</topic><topic>Particle and Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Information Technology</topic><topic>Solid State Physics</topic><topic>Spintronics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Glushkov, A. V.</creatorcontrib><creatorcontrib>Saburov, A. V.</creatorcontrib><collection>CrossRef</collection><jtitle>JETP letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Glushkov, A. V.</au><au>Saburov, A. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array</atitle><jtitle>JETP letters</jtitle><stitle>Jetp Lett</stitle><date>2019</date><risdate>2019</risdate><volume>109</volume><issue>9</issue><spage>559</spage><epage>563</epage><pages>559-563</pages><issn>0021-3640</issn><eissn>1090-6487</eissn><abstract>The lateral distribution of muons in extensive air showers with energies above 1017 eV detected by underground scintillation detectors with a threshold of 1.0 GeV at the Yakutsk array in 1986–2016 has been analyzed. The experimental data on the muon flux density at a distance of 300 m from the shower axis have been compared to the calculations within various models of hadron interactions at ultrahigh energies. The experimental data are in the best agreement with the QGSJet01 and QGSJet II-04 models. The mass composition of cosmic rays in the energy range of (1–30) × 10
17
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| ispartof | JETP letters, 2019, Vol.109 (9), p.559-563 |
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| language | eng |
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| source | SpringerNature Journals |
| subjects | Arrays Astrophysics and Cosmology Atomic Biological and Medical Physics Biophysics Composition Cosmic ray showers Cosmic rays Detectors Flux density Molecular Muons Nuclei (nuclear physics) Optical and Plasma Physics Particle and Nuclear Physics Physics Physics and Astronomy Quantum Information Technology Solid State Physics Spintronics |
| title | Mass Composition of Cosmic Rays with Energies above 1017 eV According to the Data from the Muon Detectors of the Yakutsk EAS Array |
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