Relationship between magnetic rigidity cutoff and chaotic behavior in cosmic ray time series using visibility graph and network analysis techniques
Cosmic rays are highly energetic particles originating from astrophysical events outside the Solar System. In this study, we analyze the time series of cosmic ray flux measured by neutron detectors at 16 monitoring stations distributed worldwide. By applying visibility graph analysis, we explore the...
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| Veröffentlicht in: | Chaos (Woodbury, N.Y.) N.Y.), 2024-02, Vol.34 (2) |
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| creator | Sierra-Porta, D. |
| description | Cosmic rays are highly energetic particles originating from astrophysical events outside the Solar System. In this study, we analyze the time series of cosmic ray flux measured by neutron detectors at 16 monitoring stations distributed worldwide. By applying visibility graph analysis, we explore the relationship between the magnetic rigidity cutoff (
R
c) and the fractality exhibited from topology of the cosmic ray time series. Our results reveal a significant association between the magnetic rigidity cutoff and the fractality of the cosmic ray time series. Specifically, the analysis of visibility graphs and network properties demonstrates that the magnetic rigidity is inversely related to the magnetic rigidity cutoff. The identified relationship between magnetic rigidity and fractality provides insights into the chaotic nature of cosmic ray variations and their potential uses for predictability. |
| doi_str_mv | 10.1063/5.0167156 |
| format | Article |
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R
c) and the fractality exhibited from topology of the cosmic ray time series. Our results reveal a significant association between the magnetic rigidity cutoff and the fractality of the cosmic ray time series. Specifically, the analysis of visibility graphs and network properties demonstrates that the magnetic rigidity is inversely related to the magnetic rigidity cutoff. The identified relationship between magnetic rigidity and fractality provides insights into the chaotic nature of cosmic ray variations and their potential uses for predictability.</description><identifier>ISSN: 1054-1500</identifier><identifier>EISSN: 1089-7682</identifier><identifier>DOI: 10.1063/5.0167156</identifier><identifier>PMID: 38363955</identifier><identifier>CODEN: CHAOEH</identifier><language>eng</language><publisher>United States: American Institute of Physics</publisher><subject>Cosmic rays ; Energetic particles ; Magnetic properties ; Magnetic rigidity ; Network analysis ; Neutron counters ; Rigidity ; Time series ; Topology ; Visibility</subject><ispartof>Chaos (Woodbury, N.Y.), 2024-02, Vol.34 (2)</ispartof><rights>Author(s)</rights><rights>2024 Author(s). Published under an exclusive license by AIP Publishing.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c343t-92b8e46e6bb1a14a2ece1b3e65a02ae49719af1722657854183563e763f6081f3</cites><orcidid>0000-0003-3461-1347</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,794,4512,27924,27925</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/38363955$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Sierra-Porta, D.</creatorcontrib><title>Relationship between magnetic rigidity cutoff and chaotic behavior in cosmic ray time series using visibility graph and network analysis techniques</title><title>Chaos (Woodbury, N.Y.)</title><addtitle>Chaos</addtitle><description>Cosmic rays are highly energetic particles originating from astrophysical events outside the Solar System. In this study, we analyze the time series of cosmic ray flux measured by neutron detectors at 16 monitoring stations distributed worldwide. By applying visibility graph analysis, we explore the relationship between the magnetic rigidity cutoff (
R
c) and the fractality exhibited from topology of the cosmic ray time series. Our results reveal a significant association between the magnetic rigidity cutoff and the fractality of the cosmic ray time series. Specifically, the analysis of visibility graphs and network properties demonstrates that the magnetic rigidity is inversely related to the magnetic rigidity cutoff. The identified relationship between magnetic rigidity and fractality provides insights into the chaotic nature of cosmic ray variations and their potential uses for predictability.</description><subject>Cosmic rays</subject><subject>Energetic particles</subject><subject>Magnetic properties</subject><subject>Magnetic rigidity</subject><subject>Network analysis</subject><subject>Neutron counters</subject><subject>Rigidity</subject><subject>Time series</subject><subject>Topology</subject><subject>Visibility</subject><issn>1054-1500</issn><issn>1089-7682</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><recordid>eNp9kU2L1EAQhhtR3A89-AekwYsrZO2PdKdzlMUvWBBEz6HTU5nUmqTHrs4u8zv8wyYzowcPnuqFeniq4GXshRTXUlj91lwLaStp7CN2LoWri8o69XjNpiykEeKMXRDdCSGk0uYpO9NOW10bc85-fYXBZ4wT9bjjLeQHgImPfjtBxsATbnGDec_DnGPXcT9teOh9XHct9P4eY-I48RBpXHG_5xlH4AQJgfhMOG35PRK2OKyabfK7_mBZ_A8x_ViyH_aExDOEfsKfM9Az9qTzA8Hz07xk3z-8_3bzqbj98vHzzbvbIuhS56JWrYPSgm1b6WXpFQSQrQZrvFAeyrqSte9kpZQ1lTOldNpYDZXVnRVOdvqSvT56dymud3MzIgUYBj9BnKlRtXKqrIVyC_rqH_Quzml5_UBZVYlK1At1daRCikQJumaXcPRp30jRrE01pjk1tbAvT8a5HWHzl_xTzQK8OQIUMB8q-o_tN3q5nOo</recordid><startdate>202402</startdate><enddate>202402</enddate><creator>Sierra-Porta, D.</creator><general>American Institute of Physics</general><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7X8</scope><orcidid>https://orcid.org/0000-0003-3461-1347</orcidid></search><sort><creationdate>202402</creationdate><title>Relationship between magnetic rigidity cutoff and chaotic behavior in cosmic ray time series using visibility graph and network analysis techniques</title><author>Sierra-Porta, D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c343t-92b8e46e6bb1a14a2ece1b3e65a02ae49719af1722657854183563e763f6081f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Cosmic rays</topic><topic>Energetic particles</topic><topic>Magnetic properties</topic><topic>Magnetic rigidity</topic><topic>Network analysis</topic><topic>Neutron counters</topic><topic>Rigidity</topic><topic>Time series</topic><topic>Topology</topic><topic>Visibility</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sierra-Porta, D.</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><jtitle>Chaos (Woodbury, N.Y.)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sierra-Porta, D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Relationship between magnetic rigidity cutoff and chaotic behavior in cosmic ray time series using visibility graph and network analysis techniques</atitle><jtitle>Chaos (Woodbury, N.Y.)</jtitle><addtitle>Chaos</addtitle><date>2024-02</date><risdate>2024</risdate><volume>34</volume><issue>2</issue><issn>1054-1500</issn><eissn>1089-7682</eissn><coden>CHAOEH</coden><abstract>Cosmic rays are highly energetic particles originating from astrophysical events outside the Solar System. In this study, we analyze the time series of cosmic ray flux measured by neutron detectors at 16 monitoring stations distributed worldwide. By applying visibility graph analysis, we explore the relationship between the magnetic rigidity cutoff (
R
c) and the fractality exhibited from topology of the cosmic ray time series. Our results reveal a significant association between the magnetic rigidity cutoff and the fractality of the cosmic ray time series. Specifically, the analysis of visibility graphs and network properties demonstrates that the magnetic rigidity is inversely related to the magnetic rigidity cutoff. The identified relationship between magnetic rigidity and fractality provides insights into the chaotic nature of cosmic ray variations and their potential uses for predictability.</abstract><cop>United States</cop><pub>American Institute of Physics</pub><pmid>38363955</pmid><doi>10.1063/5.0167156</doi><tpages>7</tpages><orcidid>https://orcid.org/0000-0003-3461-1347</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
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| ispartof | Chaos (Woodbury, N.Y.), 2024-02, Vol.34 (2) |
| issn | 1054-1500 1089-7682 |
| language | eng |
| recordid | cdi_proquest_journals_2926270709 |
| source | AIP Journals Complete |
| subjects | Cosmic rays Energetic particles Magnetic properties Magnetic rigidity Network analysis Neutron counters Rigidity Time series Topology Visibility |
| title | Relationship between magnetic rigidity cutoff and chaotic behavior in cosmic ray time series using visibility graph and network analysis techniques |
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