Loading…

Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions

The flux of energetic particles originating from the Sun fluctuates during the solar cycles. It depends on the number and properties of Active Regions (ARs) present in a single day and associated solar activities, such as solar flares and coronal mass ejections (CMEs). Observational records of the S...

Full description

Saved in:
Bibliographic Details
Published in:arXiv.org 2023-03
Main Authors: Marroquin, Russell D, Sadykov, Viacheslav, Kosovichev, Alexander, Kitiashvili, Irina N, Oria, Vincent, Nita, Gelu M, Illarionov, Egor, O'Keefe, Patrick M, Fraila Francis, Chun-Jie, Chong, Kosovich, Paul, Aatiya Ali
Format: Article
Language:English
Subjects:
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by
cites
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Marroquin, Russell D
Sadykov, Viacheslav
Kosovichev, Alexander
Kitiashvili, Irina N
Oria, Vincent
Nita, Gelu M
Illarionov, Egor
O'Keefe, Patrick M
Fraila Francis
Chun-Jie, Chong
Kosovich, Paul
Aatiya Ali
description The flux of energetic particles originating from the Sun fluctuates during the solar cycles. It depends on the number and properties of Active Regions (ARs) present in a single day and associated solar activities, such as solar flares and coronal mass ejections (CMEs). Observational records of the Space Weather Prediction Center (SWPC NOAA) enable the creation of time-indexed databases containing information about ARs and particle flux enhancements, most widely known as Solar Energetic Particle events (SEPs). In this work, we utilize the data available for Solar Cycles 21-24, and the initial phase of Cycle 25 to perform a statistical analysis of the correlation between SEPs and properties of ARs inferred from the McIntosh and Hale classifications. We find that the complexity of the magnetic field, longitudinal location, area, and penumbra type of the largest sunspot of ARs are most correlated with the production of SEPs. It is found that most SEPs (\(\approx\)60\%, or 108 out of 181 considered events) were generated from an AR classified with the 'k' McIntosh subclass as the second component, and these ARs are more likely to produce SEPs if they fall in a Hale class containing \(\delta\) component. The resulting database containing information about SEP events and ARs is publicly available and can be used for the development of Machine Learning (ML) models to predict the occurrence of SEPs.
doi_str_mv 10.48550/arxiv.2303.06100
format article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2786308395</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2786308395</sourcerecordid><originalsourceid>FETCH-LOGICAL-a950-5382a36bc6615ab6bbeb20943e3055011a55332fd69c0339d1ba64f6440c5bb23</originalsourceid><addsrcrecordid>eNotj81qwzAQhEWh0JDmAXoT9Gx3pbUU-xhM-gOBhib3INnr1MFYqSSn7dtX0JyGnWG_3WHsQUBelErBk_E__SWXCJiDFgA3bCYRRVYWUt6xRQgnAJB6KZXCGTvuool9iH1jBr6LU_vLXcfjJ_HaeU9DCt3ILcVvopHv3GA8X4_kj5RW-Nb4JAMFbsaWb707UzLSmBirJvYX4h90TIRwz247MwRaXHXO9s_rff2abd5f3urVJjOVgkxhKQ1q22gtlLHaWrISqgIJIXUTwqSnUXatrhpArFphjS46XRTQKGslztnjP_bs3ddEIR5ObvJjuniQy1IjlFgp_APAVlhs</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2786308395</pqid></control><display><type>article</type><title>Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions</title><source>Publicly Available Content (ProQuest)</source><creator>Marroquin, Russell D ; Sadykov, Viacheslav ; Kosovichev, Alexander ; Kitiashvili, Irina N ; Oria, Vincent ; Nita, Gelu M ; Illarionov, Egor ; O'Keefe, Patrick M ; Fraila Francis ; Chun-Jie, Chong ; Kosovich, Paul ; Aatiya Ali</creator><creatorcontrib>Marroquin, Russell D ; Sadykov, Viacheslav ; Kosovichev, Alexander ; Kitiashvili, Irina N ; Oria, Vincent ; Nita, Gelu M ; Illarionov, Egor ; O'Keefe, Patrick M ; Fraila Francis ; Chun-Jie, Chong ; Kosovich, Paul ; Aatiya Ali</creatorcontrib><description>The flux of energetic particles originating from the Sun fluctuates during the solar cycles. It depends on the number and properties of Active Regions (ARs) present in a single day and associated solar activities, such as solar flares and coronal mass ejections (CMEs). Observational records of the Space Weather Prediction Center (SWPC NOAA) enable the creation of time-indexed databases containing information about ARs and particle flux enhancements, most widely known as Solar Energetic Particle events (SEPs). In this work, we utilize the data available for Solar Cycles 21-24, and the initial phase of Cycle 25 to perform a statistical analysis of the correlation between SEPs and properties of ARs inferred from the McIntosh and Hale classifications. We find that the complexity of the magnetic field, longitudinal location, area, and penumbra type of the largest sunspot of ARs are most correlated with the production of SEPs. It is found that most SEPs (\(\approx\)60\%, or 108 out of 181 considered events) were generated from an AR classified with the 'k' McIntosh subclass as the second component, and these ARs are more likely to produce SEPs if they fall in a Hale class containing \(\delta\) component. The resulting database containing information about SEP events and ARs is publicly available and can be used for the development of Machine Learning (ML) models to predict the occurrence of SEPs.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2303.06100</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Coronal mass ejection ; Energetic particles ; Machine learning ; Solar corona ; Solar cycle ; Solar flares ; Space weather ; Statistical analysis ; Sunspots ; Weather forecasting ; Western Hemisphere</subject><ispartof>arXiv.org, 2023-03</ispartof><rights>2023. 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><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2786308395?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>780,784,25753,27925,37012,44590</link.rule.ids></links><search><creatorcontrib>Marroquin, Russell D</creatorcontrib><creatorcontrib>Sadykov, Viacheslav</creatorcontrib><creatorcontrib>Kosovichev, Alexander</creatorcontrib><creatorcontrib>Kitiashvili, Irina N</creatorcontrib><creatorcontrib>Oria, Vincent</creatorcontrib><creatorcontrib>Nita, Gelu M</creatorcontrib><creatorcontrib>Illarionov, Egor</creatorcontrib><creatorcontrib>O'Keefe, Patrick M</creatorcontrib><creatorcontrib>Fraila Francis</creatorcontrib><creatorcontrib>Chun-Jie, Chong</creatorcontrib><creatorcontrib>Kosovich, Paul</creatorcontrib><creatorcontrib>Aatiya Ali</creatorcontrib><title>Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions</title><title>arXiv.org</title><description>The flux of energetic particles originating from the Sun fluctuates during the solar cycles. It depends on the number and properties of Active Regions (ARs) present in a single day and associated solar activities, such as solar flares and coronal mass ejections (CMEs). Observational records of the Space Weather Prediction Center (SWPC NOAA) enable the creation of time-indexed databases containing information about ARs and particle flux enhancements, most widely known as Solar Energetic Particle events (SEPs). In this work, we utilize the data available for Solar Cycles 21-24, and the initial phase of Cycle 25 to perform a statistical analysis of the correlation between SEPs and properties of ARs inferred from the McIntosh and Hale classifications. We find that the complexity of the magnetic field, longitudinal location, area, and penumbra type of the largest sunspot of ARs are most correlated with the production of SEPs. It is found that most SEPs (\(\approx\)60\%, or 108 out of 181 considered events) were generated from an AR classified with the 'k' McIntosh subclass as the second component, and these ARs are more likely to produce SEPs if they fall in a Hale class containing \(\delta\) component. The resulting database containing information about SEP events and ARs is publicly available and can be used for the development of Machine Learning (ML) models to predict the occurrence of SEPs.</description><subject>Coronal mass ejection</subject><subject>Energetic particles</subject><subject>Machine learning</subject><subject>Solar corona</subject><subject>Solar cycle</subject><subject>Solar flares</subject><subject>Space weather</subject><subject>Statistical analysis</subject><subject>Sunspots</subject><subject>Weather forecasting</subject><subject>Western Hemisphere</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNotj81qwzAQhEWh0JDmAXoT9Gx3pbUU-xhM-gOBhib3INnr1MFYqSSn7dtX0JyGnWG_3WHsQUBelErBk_E__SWXCJiDFgA3bCYRRVYWUt6xRQgnAJB6KZXCGTvuool9iH1jBr6LU_vLXcfjJ_HaeU9DCt3ILcVvopHv3GA8X4_kj5RW-Nb4JAMFbsaWb707UzLSmBirJvYX4h90TIRwz247MwRaXHXO9s_rff2abd5f3urVJjOVgkxhKQ1q22gtlLHaWrISqgIJIXUTwqSnUXatrhpArFphjS46XRTQKGslztnjP_bs3ddEIR5ObvJjuniQy1IjlFgp_APAVlhs</recordid><startdate>20230322</startdate><enddate>20230322</enddate><creator>Marroquin, Russell D</creator><creator>Sadykov, Viacheslav</creator><creator>Kosovichev, Alexander</creator><creator>Kitiashvili, Irina N</creator><creator>Oria, Vincent</creator><creator>Nita, Gelu M</creator><creator>Illarionov, Egor</creator><creator>O'Keefe, Patrick M</creator><creator>Fraila Francis</creator><creator>Chun-Jie, Chong</creator><creator>Kosovich, Paul</creator><creator>Aatiya Ali</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20230322</creationdate><title>Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions</title><author>Marroquin, Russell D ; Sadykov, Viacheslav ; Kosovichev, Alexander ; Kitiashvili, Irina N ; Oria, Vincent ; Nita, Gelu M ; Illarionov, Egor ; O'Keefe, Patrick M ; Fraila Francis ; Chun-Jie, Chong ; Kosovich, Paul ; Aatiya Ali</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a950-5382a36bc6615ab6bbeb20943e3055011a55332fd69c0339d1ba64f6440c5bb23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Coronal mass ejection</topic><topic>Energetic particles</topic><topic>Machine learning</topic><topic>Solar corona</topic><topic>Solar cycle</topic><topic>Solar flares</topic><topic>Space weather</topic><topic>Statistical analysis</topic><topic>Sunspots</topic><topic>Weather forecasting</topic><topic>Western Hemisphere</topic><toplevel>online_resources</toplevel><creatorcontrib>Marroquin, Russell D</creatorcontrib><creatorcontrib>Sadykov, Viacheslav</creatorcontrib><creatorcontrib>Kosovichev, Alexander</creatorcontrib><creatorcontrib>Kitiashvili, Irina N</creatorcontrib><creatorcontrib>Oria, Vincent</creatorcontrib><creatorcontrib>Nita, Gelu M</creatorcontrib><creatorcontrib>Illarionov, Egor</creatorcontrib><creatorcontrib>O'Keefe, Patrick M</creatorcontrib><creatorcontrib>Fraila Francis</creatorcontrib><creatorcontrib>Chun-Jie, Chong</creatorcontrib><creatorcontrib>Kosovich, Paul</creatorcontrib><creatorcontrib>Aatiya Ali</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content (ProQuest)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Marroquin, Russell D</au><au>Sadykov, Viacheslav</au><au>Kosovichev, Alexander</au><au>Kitiashvili, Irina N</au><au>Oria, Vincent</au><au>Nita, Gelu M</au><au>Illarionov, Egor</au><au>O'Keefe, Patrick M</au><au>Fraila Francis</au><au>Chun-Jie, Chong</au><au>Kosovich, Paul</au><au>Aatiya Ali</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions</atitle><jtitle>arXiv.org</jtitle><date>2023-03-22</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>The flux of energetic particles originating from the Sun fluctuates during the solar cycles. It depends on the number and properties of Active Regions (ARs) present in a single day and associated solar activities, such as solar flares and coronal mass ejections (CMEs). Observational records of the Space Weather Prediction Center (SWPC NOAA) enable the creation of time-indexed databases containing information about ARs and particle flux enhancements, most widely known as Solar Energetic Particle events (SEPs). In this work, we utilize the data available for Solar Cycles 21-24, and the initial phase of Cycle 25 to perform a statistical analysis of the correlation between SEPs and properties of ARs inferred from the McIntosh and Hale classifications. We find that the complexity of the magnetic field, longitudinal location, area, and penumbra type of the largest sunspot of ARs are most correlated with the production of SEPs. It is found that most SEPs (\(\approx\)60\%, or 108 out of 181 considered events) were generated from an AR classified with the 'k' McIntosh subclass as the second component, and these ARs are more likely to produce SEPs if they fall in a Hale class containing \(\delta\) component. The resulting database containing information about SEP events and ARs is publicly available and can be used for the development of Machine Learning (ML) models to predict the occurrence of SEPs.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2303.06100</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2023-03
issn 2331-8422
language eng
recordid cdi_proquest_journals_2786308395
source Publicly Available Content (ProQuest)
subjects Coronal mass ejection
Energetic particles
Machine learning
Solar corona
Solar cycle
Solar flares
Space weather
Statistical analysis
Sunspots
Weather forecasting
Western Hemisphere
title Statistical Study of the Correlation between Solar Energetic Particles and Properties of Active Regions
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-01T19%3A52%3A59IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Statistical%20Study%20of%20the%20Correlation%20between%20Solar%20Energetic%20Particles%20and%20Properties%20of%20Active%20Regions&rft.jtitle=arXiv.org&rft.au=Marroquin,%20Russell%20D&rft.date=2023-03-22&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2303.06100&rft_dat=%3Cproquest%3E2786308395%3C/proquest%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-a950-5382a36bc6615ab6bbeb20943e3055011a55332fd69c0339d1ba64f6440c5bb23%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2786308395&rft_id=info:pmid/&rfr_iscdi=true