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Study of characteristics of Forbush decreases detected in 2006 – 2011 by means of muon hodoscope URAGAN
Results of the study of variations of cosmic ray muon flux at the Earth surface during Forbush decreases (FD) registered in 2006 – 2011 by means of muon hodoscope URAGAN both for the integral counting rate and for different angular intervals are presented. Dependences of the amplitude of the decreas...
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Published in: | Journal of physics. Conference series 2013-01, Vol.409 (1), p.12189-4 |
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creator | Barbashina, N S Astapov, I I Borog, V V Dmitrieva, A N Kokoulin, R P Kompaniets, K G Mishutina, Yu N Petrukhin, A A Shutenko, V V Sit'ko, O A Yakovleva, E I Yashin, I I |
description | Results of the study of variations of cosmic ray muon flux at the Earth surface during Forbush decreases (FD) registered in 2006 – 2011 by means of muon hodoscope URAGAN both for the integral counting rate and for different angular intervals are presented. Dependences of the amplitude of the decrease of cosmic ray muon intensity on the energy of primary particles in the energy region above 10 GeV during different phases of the FD were obtained. On the basis of the analysis of spatial-angular distribution of muon flux, values of the horizontal projections of the local anisotropy vector were calculated and their dynamics was studied. Energy, angular and temporal characteristics of Forbush decreases determined from cosmic ray muon data are compared with basic parameters characterizing conditions of near-Earth space before and during FD. |
doi_str_mv | 10.1088/1742-6596/409/1/012189 |
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Energy, angular and temporal characteristics of Forbush decreases determined from cosmic ray muon data are compared with basic parameters characterizing conditions of near-Earth space before and during FD.</description><subject>Angular distribution</subject><subject>Anisotropy</subject><subject>Cosmic rays</subject><subject>Earth surface</subject><subject>Flux</subject><subject>Forbush decreases</subject><subject>Hodoscopes</subject><subject>Horizontal</subject><subject>Mathematical analysis</subject><subject>Muons</subject><subject>Physics</subject><issn>1742-6596</issn><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNpdkcFOwzAMhisEEmPwCigSFy6lcdKmzXGaYCBNIME4R2nqap3WZiTtYTfegTfkSUgZQghf_Mv-bFm_o-gS6A3QokggT1ksMimSlMoEEgoMCnkUTX4bx3_0aXTm_YZSHiKfRM1LP1R7Ymti1tpp06NrfN8YP5burCsHvyYVGofaow-qx8BUpOkIo1SQz_ePIABIuSct6u57rh1sR9a2st7YHZLX59li9ngendR66_HiJ0-j1d3tan4fL58WD_PZMjZcpH0cttJSM1pmyEWmEWqoOFDIakAqTVXLIq1KKEGWHAtOhcS0YAazSjAdatPo-rB25-zbgL5XbeMNbre6Qzt4BTmntBC5kAG9-odu7OC6cJxiWZ6zYGfBAyUOlHHWe4e12rmm1W6vgKrxAWr0Vo3eqjChQB0ewL8ATPh3Ug</recordid><startdate>20130101</startdate><enddate>20130101</enddate><creator>Barbashina, N S</creator><creator>Astapov, I I</creator><creator>Borog, V V</creator><creator>Dmitrieva, A N</creator><creator>Kokoulin, R P</creator><creator>Kompaniets, K G</creator><creator>Mishutina, Yu N</creator><creator>Petrukhin, A A</creator><creator>Shutenko, V V</creator><creator>Sit'ko, O A</creator><creator>Yakovleva, E I</creator><creator>Yashin, I I</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PHGZM</scope><scope>PHGZT</scope><scope>PIMPY</scope><scope>PKEHL</scope><scope>PQEST</scope><scope>PQGLB</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>7U5</scope><scope>8BQ</scope><scope>JG9</scope></search><sort><creationdate>20130101</creationdate><title>Study of characteristics of Forbush decreases detected in 2006 – 2011 by means of muon hodoscope URAGAN</title><author>Barbashina, N S ; 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subjects | Angular distribution Anisotropy Cosmic rays Earth surface Flux Forbush decreases Hodoscopes Horizontal Mathematical analysis Muons Physics |
title | Study of characteristics of Forbush decreases detected in 2006 – 2011 by means of muon hodoscope URAGAN |
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