Searching for preferential arrival directions of ultrahigh-energy cosmic rays on the Moscow State University EAS array
There is evidence for possible clustering in the arrival directions of extensive air showers (EASs). A program for analyzing EAS arrival directions has been developed to investigate this problem and the database of the Moscow State University EAS array for 1982–1989 has been analyzed. The distributi...
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Veröffentlicht in: | Moscow University physics bulletin 2007-10, Vol.62 (5), p.320-323 |
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container_title | Moscow University physics bulletin |
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creator | Kalmykov, N. N. Kulikov, G. V. Silaev, Aleksei A. Silaev, A. A. Sulakov, V. P. |
description | There is evidence for possible clustering in the arrival directions of extensive air showers (EASs). A program for analyzing EAS arrival directions has been developed to investigate this problem and the database of the Moscow State University EAS array for 1982–1989 has been analyzed. The distributions in equatorial coordinates have been derived for cosmic rays with energies E ≥ 2 × 1015 eV and zenith angles |
doi_str_mv | 10.3103/S0027134907050116 |
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N. ; Kulikov, G. V. ; Silaev, Aleksei A. ; Silaev, A. A. ; Sulakov, V. P.</creator><creatorcontrib>Kalmykov, N. N. ; Kulikov, G. V. ; Silaev, Aleksei A. ; Silaev, A. A. ; Sulakov, V. P.</creatorcontrib><description>There is evidence for possible clustering in the arrival directions of extensive air showers (EASs). A program for analyzing EAS arrival directions has been developed to investigate this problem and the database of the Moscow State University EAS array for 1982–1989 has been analyzed. The distributions in equatorial coordinates have been derived for cosmic rays with energies E ≥ 2 × 1015 eV and zenith angles <40°. The uniformity of the derived distributions is verified using various statistical tests.</description><identifier>ISSN: 0027-1349</identifier><identifier>EISSN: 1934-8460</identifier><identifier>DOI: 10.3103/S0027134907050116</identifier><language>eng</language><publisher>New York: Springer Nature B.V</publisher><subject>Arrays ; Clustering ; Cosmic ray showers ; Cosmic rays ; Statistical tests</subject><ispartof>Moscow University physics bulletin, 2007-10, Vol.62 (5), p.320-323</ispartof><rights>Allerton Press, Inc. 2007.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>315,781,785,27929,27930</link.rule.ids></links><search><creatorcontrib>Kalmykov, N. N.</creatorcontrib><creatorcontrib>Kulikov, G. V.</creatorcontrib><creatorcontrib>Silaev, Aleksei A.</creatorcontrib><creatorcontrib>Silaev, A. A.</creatorcontrib><creatorcontrib>Sulakov, V. P.</creatorcontrib><title>Searching for preferential arrival directions of ultrahigh-energy cosmic rays on the Moscow State University EAS array</title><title>Moscow University physics bulletin</title><description>There is evidence for possible clustering in the arrival directions of extensive air showers (EASs). A program for analyzing EAS arrival directions has been developed to investigate this problem and the database of the Moscow State University EAS array for 1982–1989 has been analyzed. The distributions in equatorial coordinates have been derived for cosmic rays with energies E ≥ 2 × 1015 eV and zenith angles <40°. The uniformity of the derived distributions is verified using various statistical tests.</description><subject>Arrays</subject><subject>Clustering</subject><subject>Cosmic ray showers</subject><subject>Cosmic rays</subject><subject>Statistical tests</subject><issn>0027-1349</issn><issn>1934-8460</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><recordid>eNplkMtOwzAURC0EEqXwAewssQ5c20mcLKuqPKQiFinryPWjcdXG5dotyt-TCnasZnFGM9Ih5J7Bo2AgnhoALpnIa5BQAGPlBZmwWuRZlZdwSSZnnJ35NbmJcQtQlFzUE3JqrELd-X5DXUB6QOss2j55taMK0Z_GNB6tTj70kQZHj7uEqvObLrO9xc1AdYh7rymqYeQ9TZ2l7yHq8E2bpJKln70_WYw-DXQxa86rarglV07tor37yylZPS9W89ds-fHyNp8tMy2hypjLnVEKirWudLnmIIt1AdoU0mme25orDQZKY3ldWJNbXbmqZlI65Qx3YMSUPPzOHjB8HW1M7TYcsR8fW16WeZVLUVdji_22NIYYRwPtAf1e4dAyaM922392xQ-Vr289</recordid><startdate>200710</startdate><enddate>200710</enddate><creator>Kalmykov, N. N.</creator><creator>Kulikov, G. 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N.</creatorcontrib><creatorcontrib>Kulikov, G. V.</creatorcontrib><creatorcontrib>Silaev, Aleksei A.</creatorcontrib><creatorcontrib>Silaev, A. A.</creatorcontrib><creatorcontrib>Sulakov, V. P.</creatorcontrib><collection>CrossRef</collection><jtitle>Moscow University physics bulletin</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kalmykov, N. N.</au><au>Kulikov, G. V.</au><au>Silaev, Aleksei A.</au><au>Silaev, A. A.</au><au>Sulakov, V. P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Searching for preferential arrival directions of ultrahigh-energy cosmic rays on the Moscow State University EAS array</atitle><jtitle>Moscow University physics bulletin</jtitle><date>2007-10</date><risdate>2007</risdate><volume>62</volume><issue>5</issue><spage>320</spage><epage>323</epage><pages>320-323</pages><issn>0027-1349</issn><eissn>1934-8460</eissn><abstract>There is evidence for possible clustering in the arrival directions of extensive air showers (EASs). A program for analyzing EAS arrival directions has been developed to investigate this problem and the database of the Moscow State University EAS array for 1982–1989 has been analyzed. The distributions in equatorial coordinates have been derived for cosmic rays with energies E ≥ 2 × 1015 eV and zenith angles <40°. The uniformity of the derived distributions is verified using various statistical tests.</abstract><cop>New York</cop><pub>Springer Nature B.V</pub><doi>10.3103/S0027134907050116</doi><tpages>4</tpages></addata></record> |
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subjects | Arrays Clustering Cosmic ray showers Cosmic rays Statistical tests |
title | Searching for preferential arrival directions of ultrahigh-energy cosmic rays on the Moscow State University EAS array |
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