Causal Attention Deep-learning Model for Solar Flare Forecasting
Solar flares originate from the sudden release of energy stored in the magnetic field of the active region on the Sun, but the trigger for flares is still uncertain. Currently, deep-learning-based solar flare prediction models have achieved good results and are widely recognized. However, these mode...
Gespeichert in:
Veröffentlicht in: | The Astrophysical journal. Supplement series 2024-10, Vol.274 (2), p.38 |
---|---|
Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | |
---|---|
container_issue | 2 |
container_start_page | 38 |
container_title | The Astrophysical journal. Supplement series |
container_volume | 274 |
creator | Zhang, Xinze Xu, Long Li, Zihan Huang, Xin |
description | Solar flares originate from the sudden release of energy stored in the magnetic field of the active region on the Sun, but the trigger for flares is still uncertain. Currently, deep-learning-based solar flare prediction models have achieved good results and are widely recognized. However, these models focus more on data correlation rather than causality. An ideal flare prediction model should probe into the causes/triggers of solar flares, and diagnose the precursors of flares rather than just correlation analysis. To extract more informative precursors of flares from magnetograms, while suppressing the interference of confounding factors, a causal attention module is introduced to disentangle causal and confounder features from the input features. To address the problem of imbalanced positive and negative samples in the data set, an adaptive data set split mechanism is proposed. It divides the data set into several balanced subsets of positive and negative samples, and dynamically adjusts the subsets according to the model’s prediction results during the training process. The experimental results demonstrate that our proposed model achieves 4.08%, 8.38%, and 2.19% higher accuracy, true skill score, and area under the receiver operating characteristic curve than the baseline model. Additionally, the class-specific heatmaps by using the gradient-weighted class activation mapping method reveal that our proposed model generally focuses on the polarity inverse line of active regions, well in line with theoretical study. |
doi_str_mv | 10.3847/1538-4365/ad7386 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_crossref_primary_10_3847_1538_4365_ad7386</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><doaj_id>oai_doaj_org_article_600d88df6b104714b5230e0901916422</doaj_id><sourcerecordid>3112853465</sourcerecordid><originalsourceid>FETCH-LOGICAL-c299t-94855c9f6cf5da6c4bde8cc21fb8e3edce82a284742e87dd6b696a2d83034b813</originalsourceid><addsrcrecordid>eNp1kL1PwzAQxS0EEqWwM0ZiJfT8GXujKhQqFTEAs-XYlypViIuTDvz3pATBxHInnd57d_cj5JLCDdeimFHJdS64kjMXCq7VEZn8jo7JBEAVOYAwp-Ss67YAUEhuJuR24fada7J532Pb17HN7hB3eYMutXW7yZ5iwCarYspeYuNSthwKZsuY0LuuHxTn5KRyTYcXP31K3pb3r4vHfP38sFrM17lnxvS5EVpKbyrlKxmc8qIMqL1ntCo1cgweNXNseEQw1EUIqlRGORY0By5KTfmUrMbcEN3W7lL97tKnja6234OYNtalvvYNWgUQtA6VKimIgopSMg4IBqihSjA2ZF2NWbsUP_bY9XYb96kdzrecUqYlF0oOKhhVPsWuS1j9bqVgD8ztAbA9ALYj88FyPVrquPvL_Ff-BQ0yf7I</addsrcrecordid><sourcetype>Open Website</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>3112853465</pqid></control><display><type>article</type><title>Causal Attention Deep-learning Model for Solar Flare Forecasting</title><source>IOP Publishing Free Content</source><source>DOAJ Directory of Open Access Journals</source><source>Alma/SFX Local Collection</source><creator>Zhang, Xinze ; Xu, Long ; Li, Zihan ; Huang, Xin</creator><creatorcontrib>Zhang, Xinze ; Xu, Long ; Li, Zihan ; Huang, Xin</creatorcontrib><description>Solar flares originate from the sudden release of energy stored in the magnetic field of the active region on the Sun, but the trigger for flares is still uncertain. Currently, deep-learning-based solar flare prediction models have achieved good results and are widely recognized. However, these models focus more on data correlation rather than causality. An ideal flare prediction model should probe into the causes/triggers of solar flares, and diagnose the precursors of flares rather than just correlation analysis. To extract more informative precursors of flares from magnetograms, while suppressing the interference of confounding factors, a causal attention module is introduced to disentangle causal and confounder features from the input features. To address the problem of imbalanced positive and negative samples in the data set, an adaptive data set split mechanism is proposed. It divides the data set into several balanced subsets of positive and negative samples, and dynamically adjusts the subsets according to the model’s prediction results during the training process. The experimental results demonstrate that our proposed model achieves 4.08%, 8.38%, and 2.19% higher accuracy, true skill score, and area under the receiver operating characteristic curve than the baseline model. Additionally, the class-specific heatmaps by using the gradient-weighted class activation mapping method reveal that our proposed model generally focuses on the polarity inverse line of active regions, well in line with theoretical study.</description><identifier>ISSN: 0067-0049</identifier><identifier>EISSN: 1538-4365</identifier><identifier>DOI: 10.3847/1538-4365/ad7386</identifier><language>eng</language><publisher>Saskatoon: The American Astronomical Society</publisher><subject>Adaptive sampling ; Correlation analysis ; Data correlation ; Datasets ; Deep learning ; Magnetic fields ; Precursors ; Prediction models ; Solar flare forecasting ; Solar flares ; Solar magnetic field ; Solar physics</subject><ispartof>The Astrophysical journal. Supplement series, 2024-10, Vol.274 (2), p.38</ispartof><rights>2024. The Author(s). Published by the American Astronomical Society.</rights><rights>2024. The Author(s). Published by the American Astronomical Society. 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><cites>FETCH-LOGICAL-c299t-94855c9f6cf5da6c4bde8cc21fb8e3edce82a284742e87dd6b696a2d83034b813</cites><orcidid>0000-0002-9286-2876 ; 0000-0002-3437-3636</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4365/ad7386/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,776,780,860,2096,27901,27902,38867,53842</link.rule.ids></links><search><creatorcontrib>Zhang, Xinze</creatorcontrib><creatorcontrib>Xu, Long</creatorcontrib><creatorcontrib>Li, Zihan</creatorcontrib><creatorcontrib>Huang, Xin</creatorcontrib><title>Causal Attention Deep-learning Model for Solar Flare Forecasting</title><title>The Astrophysical journal. Supplement series</title><addtitle>APJS</addtitle><addtitle>Astrophys. J. Suppl</addtitle><description>Solar flares originate from the sudden release of energy stored in the magnetic field of the active region on the Sun, but the trigger for flares is still uncertain. Currently, deep-learning-based solar flare prediction models have achieved good results and are widely recognized. However, these models focus more on data correlation rather than causality. An ideal flare prediction model should probe into the causes/triggers of solar flares, and diagnose the precursors of flares rather than just correlation analysis. To extract more informative precursors of flares from magnetograms, while suppressing the interference of confounding factors, a causal attention module is introduced to disentangle causal and confounder features from the input features. To address the problem of imbalanced positive and negative samples in the data set, an adaptive data set split mechanism is proposed. It divides the data set into several balanced subsets of positive and negative samples, and dynamically adjusts the subsets according to the model’s prediction results during the training process. The experimental results demonstrate that our proposed model achieves 4.08%, 8.38%, and 2.19% higher accuracy, true skill score, and area under the receiver operating characteristic curve than the baseline model. Additionally, the class-specific heatmaps by using the gradient-weighted class activation mapping method reveal that our proposed model generally focuses on the polarity inverse line of active regions, well in line with theoretical study.</description><subject>Adaptive sampling</subject><subject>Correlation analysis</subject><subject>Data correlation</subject><subject>Datasets</subject><subject>Deep learning</subject><subject>Magnetic fields</subject><subject>Precursors</subject><subject>Prediction models</subject><subject>Solar flare forecasting</subject><subject>Solar flares</subject><subject>Solar magnetic field</subject><subject>Solar physics</subject><issn>0067-0049</issn><issn>1538-4365</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><sourceid>DOA</sourceid><recordid>eNp1kL1PwzAQxS0EEqWwM0ZiJfT8GXujKhQqFTEAs-XYlypViIuTDvz3pATBxHInnd57d_cj5JLCDdeimFHJdS64kjMXCq7VEZn8jo7JBEAVOYAwp-Ss67YAUEhuJuR24fada7J532Pb17HN7hB3eYMutXW7yZ5iwCarYspeYuNSthwKZsuY0LuuHxTn5KRyTYcXP31K3pb3r4vHfP38sFrM17lnxvS5EVpKbyrlKxmc8qIMqL1ntCo1cgweNXNseEQw1EUIqlRGORY0By5KTfmUrMbcEN3W7lL97tKnja6234OYNtalvvYNWgUQtA6VKimIgopSMg4IBqihSjA2ZF2NWbsUP_bY9XYb96kdzrecUqYlF0oOKhhVPsWuS1j9bqVgD8ztAbA9ALYj88FyPVrquPvL_Ff-BQ0yf7I</recordid><startdate>20241001</startdate><enddate>20241001</enddate><creator>Zhang, Xinze</creator><creator>Xu, Long</creator><creator>Li, Zihan</creator><creator>Huang, Xin</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0002-9286-2876</orcidid><orcidid>https://orcid.org/0000-0002-3437-3636</orcidid></search><sort><creationdate>20241001</creationdate><title>Causal Attention Deep-learning Model for Solar Flare Forecasting</title><author>Zhang, Xinze ; Xu, Long ; Li, Zihan ; Huang, Xin</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c299t-94855c9f6cf5da6c4bde8cc21fb8e3edce82a284742e87dd6b696a2d83034b813</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Adaptive sampling</topic><topic>Correlation analysis</topic><topic>Data correlation</topic><topic>Datasets</topic><topic>Deep learning</topic><topic>Magnetic fields</topic><topic>Precursors</topic><topic>Prediction models</topic><topic>Solar flare forecasting</topic><topic>Solar flares</topic><topic>Solar magnetic field</topic><topic>Solar physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zhang, Xinze</creatorcontrib><creatorcontrib>Xu, Long</creatorcontrib><creatorcontrib>Li, Zihan</creatorcontrib><creatorcontrib>Huang, Xin</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>The Astrophysical journal. Supplement series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Zhang, Xinze</au><au>Xu, Long</au><au>Li, Zihan</au><au>Huang, Xin</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Causal Attention Deep-learning Model for Solar Flare Forecasting</atitle><jtitle>The Astrophysical journal. Supplement series</jtitle><stitle>APJS</stitle><addtitle>Astrophys. J. Suppl</addtitle><date>2024-10-01</date><risdate>2024</risdate><volume>274</volume><issue>2</issue><spage>38</spage><pages>38-</pages><issn>0067-0049</issn><eissn>1538-4365</eissn><abstract>Solar flares originate from the sudden release of energy stored in the magnetic field of the active region on the Sun, but the trigger for flares is still uncertain. Currently, deep-learning-based solar flare prediction models have achieved good results and are widely recognized. However, these models focus more on data correlation rather than causality. An ideal flare prediction model should probe into the causes/triggers of solar flares, and diagnose the precursors of flares rather than just correlation analysis. To extract more informative precursors of flares from magnetograms, while suppressing the interference of confounding factors, a causal attention module is introduced to disentangle causal and confounder features from the input features. To address the problem of imbalanced positive and negative samples in the data set, an adaptive data set split mechanism is proposed. It divides the data set into several balanced subsets of positive and negative samples, and dynamically adjusts the subsets according to the model’s prediction results during the training process. The experimental results demonstrate that our proposed model achieves 4.08%, 8.38%, and 2.19% higher accuracy, true skill score, and area under the receiver operating characteristic curve than the baseline model. Additionally, the class-specific heatmaps by using the gradient-weighted class activation mapping method reveal that our proposed model generally focuses on the polarity inverse line of active regions, well in line with theoretical study.</abstract><cop>Saskatoon</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4365/ad7386</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0002-9286-2876</orcidid><orcidid>https://orcid.org/0000-0002-3437-3636</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0067-0049 |
ispartof | The Astrophysical journal. Supplement series, 2024-10, Vol.274 (2), p.38 |
issn | 0067-0049 1538-4365 |
language | eng |
recordid | cdi_crossref_primary_10_3847_1538_4365_ad7386 |
source | IOP Publishing Free Content; DOAJ Directory of Open Access Journals; Alma/SFX Local Collection |
subjects | Adaptive sampling Correlation analysis Data correlation Datasets Deep learning Magnetic fields Precursors Prediction models Solar flare forecasting Solar flares Solar magnetic field Solar physics |
title | Causal Attention Deep-learning Model for Solar Flare Forecasting |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-09T12%3A34%3A32IST&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=Causal%20Attention%20Deep-learning%20Model%20for%20Solar%20Flare%20Forecasting&rft.jtitle=The%20Astrophysical%20journal.%20Supplement%20series&rft.au=Zhang,%20Xinze&rft.date=2024-10-01&rft.volume=274&rft.issue=2&rft.spage=38&rft.pages=38-&rft.issn=0067-0049&rft.eissn=1538-4365&rft_id=info:doi/10.3847/1538-4365/ad7386&rft_dat=%3Cproquest_cross%3E3112853465%3C/proquest_cross%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=3112853465&rft_id=info:pmid/&rft_doaj_id=oai_doaj_org_article_600d88df6b104714b5230e0901916422&rfr_iscdi=true |