Maximum Depth of Development of EASes with Energies above 1016 eV, Measured in Individual Events by Cherenkov Tracking Detectors
The Cherenkov radiation of extensive air showers (EASes) is studied using a system of optical tracking detectors based on a camera obscura as part of the Yakutsk EAS complex. These detectors allow photons to be counted from a certain height in the atmosphere and thus reconstruction of longitudinal d...
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| Veröffentlicht in: | Bulletin of the Russian Academy of Sciences. Physics 2019-08, Vol.83 (8), p.1032-1034 |
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| container_title | Bulletin of the Russian Academy of Sciences. Physics |
| container_volume | 83 |
| creator | Mokhnachevskaya, V. P. Sleptsov, I. E. Knurenko, S. P. Saburov, A. V. Egorov, Yu. A. Petrov, Z. E. |
| description | The Cherenkov radiation of extensive air showers (EASes) is studied using a system of optical tracking detectors based on a
camera obscura
as part of the Yakutsk EAS complex. These detectors allow photons to be counted from a certain height in the atmosphere and thus reconstruction of longitudinal development of a shower. Good coincidence is observed between EAS cascade curve parameter
X
max
measured in this way and by modeling. Preliminary results on the cosmic ray mass composition are obtained for energies above 10
16
eV. |
| doi_str_mv | 10.3103/S106287381908029X |
| format | Article |
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camera obscura
as part of the Yakutsk EAS complex. These detectors allow photons to be counted from a certain height in the atmosphere and thus reconstruction of longitudinal development of a shower. Good coincidence is observed between EAS cascade curve parameter
X
max
measured in this way and by modeling. Preliminary results on the cosmic ray mass composition are obtained for energies above 10
16
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camera obscura
as part of the Yakutsk EAS complex. These detectors allow photons to be counted from a certain height in the atmosphere and thus reconstruction of longitudinal development of a shower. Good coincidence is observed between EAS cascade curve parameter
X
max
measured in this way and by modeling. Preliminary results on the cosmic ray mass composition are obtained for energies above 10
16
eV.</description><subject>Atmospheric models</subject><subject>Cosmic ray showers</subject><subject>Cosmic rays</subject><subject>Detectors</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Nuclear Physics</subject><subject>Optical tracking</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Sensors</subject><issn>1062-8738</issn><issn>1934-9432</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1UMtKw0AUDaJgrX6AuwG3RueRSTLLUqMWWly0Sndhktxpp20eziTR7vx0p1RwIa7uuZwXHM-7JviOEczu5wSHNI5YTASOMRXLE29ABAt8ETB66rCj_QN_7l1Yu8GYc0H5wPuayU9ddiV6gKZdo1o50MOubkqo2sObjOZg0Yd2ZFKBWWn3yazuARFMQgRvt2gG0nYGCqQrNKkK3euikzuU9C7ComyPxmswUG3rHi2MzLe6WrmWFvK2NvbSO1NyZ-Hq5w6918dkMX72py9Pk_Fo6ueEsKUvFAcsM8HDkKig4CojPGegeKAkIVxyFUUqjDIe0zDGmYoLEkoaSBlEEjgDNvRujrmNqd87sG26qTtTucqUUiGCKOYxcypyVOWmttaAShujS2n2KcHpYej0z9DOQ48e67TVCsxv8v-mb2NGf7E</recordid><startdate>20190801</startdate><enddate>20190801</enddate><creator>Mokhnachevskaya, V. P.</creator><creator>Sleptsov, I. E.</creator><creator>Knurenko, S. P.</creator><creator>Saburov, A. V.</creator><creator>Egorov, Yu. A.</creator><creator>Petrov, Z. E.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20190801</creationdate><title>Maximum Depth of Development of EASes with Energies above 1016 eV, Measured in Individual Events by Cherenkov Tracking Detectors</title><author>Mokhnachevskaya, V. P. ; Sleptsov, I. E. ; Knurenko, S. P. ; Saburov, A. V. ; Egorov, Yu. A. ; Petrov, Z. E.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c113X-9f5e0ab95661f4d5fb15c3ef54fa115a5f77f67b582680bf8d16a24aa47ae53e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Atmospheric models</topic><topic>Cosmic ray showers</topic><topic>Cosmic rays</topic><topic>Detectors</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Nuclear Physics</topic><topic>Optical tracking</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Sensors</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mokhnachevskaya, V. P.</creatorcontrib><creatorcontrib>Sleptsov, I. E.</creatorcontrib><creatorcontrib>Knurenko, S. P.</creatorcontrib><creatorcontrib>Saburov, A. V.</creatorcontrib><creatorcontrib>Egorov, Yu. A.</creatorcontrib><creatorcontrib>Petrov, Z. E.</creatorcontrib><collection>CrossRef</collection><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mokhnachevskaya, V. P.</au><au>Sleptsov, I. E.</au><au>Knurenko, S. P.</au><au>Saburov, A. V.</au><au>Egorov, Yu. A.</au><au>Petrov, Z. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Maximum Depth of Development of EASes with Energies above 1016 eV, Measured in Individual Events by Cherenkov Tracking Detectors</atitle><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle><stitle>Bull. Russ. Acad. Sci. Phys</stitle><date>2019-08-01</date><risdate>2019</risdate><volume>83</volume><issue>8</issue><spage>1032</spage><epage>1034</epage><pages>1032-1034</pages><issn>1062-8738</issn><eissn>1934-9432</eissn><abstract>The Cherenkov radiation of extensive air showers (EASes) is studied using a system of optical tracking detectors based on a
camera obscura
as part of the Yakutsk EAS complex. These detectors allow photons to be counted from a certain height in the atmosphere and thus reconstruction of longitudinal development of a shower. Good coincidence is observed between EAS cascade curve parameter
X
max
measured in this way and by modeling. Preliminary results on the cosmic ray mass composition are obtained for energies above 10
16
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| language | eng |
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| subjects | Atmospheric models Cosmic ray showers Cosmic rays Detectors Hadrons Heavy Ions Nuclear Physics Optical tracking Physics Physics and Astronomy Sensors |
| title | Maximum Depth of Development of EASes with Energies above 1016 eV, Measured in Individual Events by Cherenkov Tracking Detectors |
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