Loading…

GLE73 Event (October 28, 2021) in Solar Cosmic Rays

Results are presented from analyzing the GLE73 event in terms of solar cosmic rays. The GLE73 event raised the count by 2–6% at polar stations of the World Neutron Monitor Network. A direct solution to the inverse problem is found, along with and the energy spectra of solar cosmic rays at the bounda...

Full description

Saved in:
Bibliographic Details
Published in:Bulletin of the Russian Academy of Sciences. Physics 2022-12, Vol.86 (12), p.1542-1548
Main Authors: Balabin, Yu. V., Gvozdevsky, B. B., Germanenko, A. V., Maurchev, E. A., Michalko, E. A.
Format: Article
Language:English
Subjects:
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93
cites cdi_FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93
container_end_page 1548
container_issue 12
container_start_page 1542
container_title Bulletin of the Russian Academy of Sciences. Physics
container_volume 86
creator Balabin, Yu. V.
Gvozdevsky, B. B.
Germanenko, A. V.
Maurchev, E. A.
Michalko, E. A.
description Results are presented from analyzing the GLE73 event in terms of solar cosmic rays. The GLE73 event raised the count by 2–6% at polar stations of the World Neutron Monitor Network. A direct solution to the inverse problem is found, along with and the energy spectra of solar cosmic rays at the boundary of the magnetosphere are obtained and the pitch angle distribution of the flux.
doi_str_mv 10.3103/S1062873822120048
format article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_2754881014</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2754881014</sourcerecordid><originalsourceid>FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93</originalsourceid><addsrcrecordid>eNp1kEFLAzEQhYMoWKs_wFvAi4Krk5nsJnuUUqtQKFg9L7vZibS0uzWpQv-9KRU8iKcZeN97D54QlwruSAHdzxUUaA1ZRIUA2h6JgSpJZ6UmPE5_krO9firOYlwC5HmJ-UDQZDo2JMdf3G3l9cxt-4aDRHsrEVDdyEUn5_2qDnLUx_XCyZd6F8_Fia9XkS9-7lC8PY5fR0_ZdDZ5Hj1MM4dG26ygxmhq25ILTsUe2RkPORC0jhQhU0lNy4YbXzfeG43QomVqsVauaEoaiqtD7ib0H58ct9Wy_wxdqqzQ5NpaBUonSh0oF_oYA_tqExbrOuwqBdV-m-rPNsmDB09MbPfO4Tf5f9M3WbZhBg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2754881014</pqid></control><display><type>article</type><title>GLE73 Event (October 28, 2021) in Solar Cosmic Rays</title><source>Springer Nature</source><creator>Balabin, Yu. V. ; Gvozdevsky, B. B. ; Germanenko, A. V. ; Maurchev, E. A. ; Michalko, E. A.</creator><creatorcontrib>Balabin, Yu. V. ; Gvozdevsky, B. B. ; Germanenko, A. V. ; Maurchev, E. A. ; Michalko, E. A.</creatorcontrib><description>Results are presented from analyzing the GLE73 event in terms of solar cosmic rays. The GLE73 event raised the count by 2–6% at polar stations of the World Neutron Monitor Network. A direct solution to the inverse problem is found, along with and the energy spectra of solar cosmic rays at the boundary of the magnetosphere are obtained and the pitch angle distribution of the flux.</description><identifier>ISSN: 1062-8738</identifier><identifier>EISSN: 1934-9432</identifier><identifier>DOI: 10.3103/S1062873822120048</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Energy spectra ; Hadrons ; Heavy Ions ; Inverse problems ; Magnetospheres ; Nuclear Physics ; Physics ; Physics and Astronomy ; Pitch (inclination) ; Solar cosmic rays</subject><ispartof>Bulletin of the Russian Academy of Sciences. Physics, 2022-12, Vol.86 (12), p.1542-1548</ispartof><rights>The Author(s) 2022. ISSN 1062-8738, Bulletin of the Russian Academy of Sciences: Physics, 2022, Vol. 86, No. 12, pp. 1542–1548. © The Author(s), 2022. This article is an open access publication. Russian Text © The Author(s), 2022, published in Izvestiya Rossiiskoi Akademii Nauk, Seriya Fizicheskaya, 2022, Vol. 86, No. 12, pp. 1810–1816.</rights><rights>The Author(s) 2022. ISSN 1062-8738, Bulletin of the Russian Academy of Sciences: Physics, 2022, Vol. 86, No. 12, pp. 1542–1548. © The Author(s), 2022. This article is an open access publication. Russian Text © The Author(s), 2022, published in Izvestiya Rossiiskoi Akademii Nauk, Seriya Fizicheskaya, 2022, Vol. 86, No. 12, pp. 1810–1816. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93</citedby><cites>FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Balabin, Yu. V.</creatorcontrib><creatorcontrib>Gvozdevsky, B. B.</creatorcontrib><creatorcontrib>Germanenko, A. V.</creatorcontrib><creatorcontrib>Maurchev, E. A.</creatorcontrib><creatorcontrib>Michalko, E. A.</creatorcontrib><title>GLE73 Event (October 28, 2021) in Solar Cosmic Rays</title><title>Bulletin of the Russian Academy of Sciences. Physics</title><addtitle>Bull. Russ. Acad. Sci. Phys</addtitle><description>Results are presented from analyzing the GLE73 event in terms of solar cosmic rays. The GLE73 event raised the count by 2–6% at polar stations of the World Neutron Monitor Network. A direct solution to the inverse problem is found, along with and the energy spectra of solar cosmic rays at the boundary of the magnetosphere are obtained and the pitch angle distribution of the flux.</description><subject>Energy spectra</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Inverse problems</subject><subject>Magnetospheres</subject><subject>Nuclear Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Pitch (inclination)</subject><subject>Solar cosmic rays</subject><issn>1062-8738</issn><issn>1934-9432</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp1kEFLAzEQhYMoWKs_wFvAi4Krk5nsJnuUUqtQKFg9L7vZibS0uzWpQv-9KRU8iKcZeN97D54QlwruSAHdzxUUaA1ZRIUA2h6JgSpJZ6UmPE5_krO9firOYlwC5HmJ-UDQZDo2JMdf3G3l9cxt-4aDRHsrEVDdyEUn5_2qDnLUx_XCyZd6F8_Fia9XkS9-7lC8PY5fR0_ZdDZ5Hj1MM4dG26ygxmhq25ILTsUe2RkPORC0jhQhU0lNy4YbXzfeG43QomVqsVauaEoaiqtD7ib0H58ct9Wy_wxdqqzQ5NpaBUonSh0oF_oYA_tqExbrOuwqBdV-m-rPNsmDB09MbPfO4Tf5f9M3WbZhBg</recordid><startdate>20221201</startdate><enddate>20221201</enddate><creator>Balabin, Yu. V.</creator><creator>Gvozdevsky, B. B.</creator><creator>Germanenko, A. V.</creator><creator>Maurchev, E. A.</creator><creator>Michalko, E. A.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20221201</creationdate><title>GLE73 Event (October 28, 2021) in Solar Cosmic Rays</title><author>Balabin, Yu. V. ; Gvozdevsky, B. B. ; Germanenko, A. V. ; Maurchev, E. A. ; Michalko, E. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Energy spectra</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Inverse problems</topic><topic>Magnetospheres</topic><topic>Nuclear Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Pitch (inclination)</topic><topic>Solar cosmic rays</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Balabin, Yu. V.</creatorcontrib><creatorcontrib>Gvozdevsky, B. B.</creatorcontrib><creatorcontrib>Germanenko, A. V.</creatorcontrib><creatorcontrib>Maurchev, E. A.</creatorcontrib><creatorcontrib>Michalko, E. A.</creatorcontrib><collection>Springer Nature OA Free Journals</collection><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>Balabin, Yu. V.</au><au>Gvozdevsky, B. B.</au><au>Germanenko, A. V.</au><au>Maurchev, E. A.</au><au>Michalko, E. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>GLE73 Event (October 28, 2021) in Solar Cosmic Rays</atitle><jtitle>Bulletin of the Russian Academy of Sciences. Physics</jtitle><stitle>Bull. Russ. Acad. Sci. Phys</stitle><date>2022-12-01</date><risdate>2022</risdate><volume>86</volume><issue>12</issue><spage>1542</spage><epage>1548</epage><pages>1542-1548</pages><issn>1062-8738</issn><eissn>1934-9432</eissn><abstract>Results are presented from analyzing the GLE73 event in terms of solar cosmic rays. The GLE73 event raised the count by 2–6% at polar stations of the World Neutron Monitor Network. A direct solution to the inverse problem is found, along with and the energy spectra of solar cosmic rays at the boundary of the magnetosphere are obtained and the pitch angle distribution of the flux.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.3103/S1062873822120048</doi><tpages>7</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 1062-8738
ispartof Bulletin of the Russian Academy of Sciences. Physics, 2022-12, Vol.86 (12), p.1542-1548
issn 1062-8738
1934-9432
language eng
recordid cdi_proquest_journals_2754881014
source Springer Nature
subjects Energy spectra
Hadrons
Heavy Ions
Inverse problems
Magnetospheres
Nuclear Physics
Physics
Physics and Astronomy
Pitch (inclination)
Solar cosmic rays
title GLE73 Event (October 28, 2021) in Solar Cosmic Rays
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T16%3A55%3A21IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=GLE73%20Event%20(October%2028,%202021)%20in%20Solar%20Cosmic%20Rays&rft.jtitle=Bulletin%20of%20the%20Russian%20Academy%20of%20Sciences.%20Physics&rft.au=Balabin,%20Yu.%20V.&rft.date=2022-12-01&rft.volume=86&rft.issue=12&rft.spage=1542&rft.epage=1548&rft.pages=1542-1548&rft.issn=1062-8738&rft.eissn=1934-9432&rft_id=info:doi/10.3103/S1062873822120048&rft_dat=%3Cproquest_cross%3E2754881014%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c2748-63b743dd9e6e738f2ec7f05030dc3132e393bde7ebfabff7420d28e3d2a1c6b93%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2754881014&rft_id=info:pmid/&rfr_iscdi=true