Three-minute Sunspot Oscillations Driven by Magnetic Reconnection in a Light Bridge

We report a different type of three-minute chromospheric oscillation above a sunspot in association with a small-scale impulsive event in a light bridge (LB). During our observations, we found a transient brightening in the LB. The brightening was composed of elementary bursts that may be a manifest...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astrophysical journal. Letters 2017-12, Vol.850 (2), p.L33
Hauptverfasser: Song, Donguk, Chae, Jongchul, Kwak, Hannah, Kano, Ryouhei, Yurchyshyn, Vasyl, Moon, Yong-Jae, Lim, Eun-Kyung, Lee, Jeongwoo
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 2
container_start_page L33
container_title Astrophysical journal. Letters
container_volume 850
creator Song, Donguk
Chae, Jongchul
Kwak, Hannah
Kano, Ryouhei
Yurchyshyn, Vasyl
Moon, Yong-Jae
Lim, Eun-Kyung
Lee, Jeongwoo
description We report a different type of three-minute chromospheric oscillation above a sunspot in association with a small-scale impulsive event in a light bridge (LB). During our observations, we found a transient brightening in the LB. The brightening was composed of elementary bursts that may be a manifestation of fast repetitive magnetic reconnections in the LB. Interestingly, the oscillations in the nearby sunspot umbra were impulsively excited when the intensity of the brightening reached its peak. The initial period of the oscillations was about 2.3 minutes and then gradually increased to 3.0 minutes with time. In addition, we found that the amplitude of the excited oscillations was twice the amplitude of oscillations before the brightening. Based on our results, we propose that magnetic reconnection occurring in an LB can excite oscillations in the nearby sunspot umbra.
doi_str_mv 10.3847/2041-8213/aa9a36
format Article
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_journals_2365662807</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365662807</sourcerecordid><originalsourceid>FETCH-LOGICAL-c447t-1f268324625cf72b58e4ff3fed29fe44f5310586b190db3afed1420e11481b093</originalsourceid><addsrcrecordid>eNp9kM9LwzAUx4MoOKd3jwHBk3X51TQ96vwJlYGb55C2yZbRpTVphf33tlTmRTy9x3uf73vwAeASo1sqWDIjiOFIEExnSqWK8iMwOYyODz2KT8FZCFuECOJYTMBytfFaRzvrulbDZedCU7dwEQpbVaq1tQvwwdsv7WC-h29q7XRrC_iui9o5XQwAtA4qmNn1poX33pZrfQ5OjKqCvvipU_Dx9Liav0TZ4vl1fpdFBWNJG2FDuKCEcRIXJiF5LDQzhhpdktRoxkxMMYoFz3GKypyqfoEZQRpjJnCOUjoFV-PdxtefnQ6t3Nadd_1LSSiPOScCJT2FRqrwdQheG9l4u1N-LzGSgzo5uJGDJzmq6yM3Y8TWze_Nf_DrP3DVbCspYiSJzCiVTWnoN6eue-E</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365662807</pqid></control><display><type>article</type><title>Three-minute Sunspot Oscillations Driven by Magnetic Reconnection in a Light Bridge</title><source>IOP Publishing Free Content</source><creator>Song, Donguk ; Chae, Jongchul ; Kwak, Hannah ; Kano, Ryouhei ; Yurchyshyn, Vasyl ; Moon, Yong-Jae ; Lim, Eun-Kyung ; Lee, Jeongwoo</creator><creatorcontrib>Song, Donguk ; Chae, Jongchul ; Kwak, Hannah ; Kano, Ryouhei ; Yurchyshyn, Vasyl ; Moon, Yong-Jae ; Lim, Eun-Kyung ; Lee, Jeongwoo</creatorcontrib><description>We report a different type of three-minute chromospheric oscillation above a sunspot in association with a small-scale impulsive event in a light bridge (LB). During our observations, we found a transient brightening in the LB. The brightening was composed of elementary bursts that may be a manifestation of fast repetitive magnetic reconnections in the LB. Interestingly, the oscillations in the nearby sunspot umbra were impulsively excited when the intensity of the brightening reached its peak. The initial period of the oscillations was about 2.3 minutes and then gradually increased to 3.0 minutes with time. In addition, we found that the amplitude of the excited oscillations was twice the amplitude of oscillations before the brightening. Based on our results, we propose that magnetic reconnection occurring in an LB can excite oscillations in the nearby sunspot umbra.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.3847/2041-8213/aa9a36</identifier><language>eng</language><publisher>Austin: The American Astronomical Society</publisher><subject>Amplitudes ; Brightening ; Magnetic reconnection ; Oscillations ; Sun: chromosphere ; Sun: transition region ; Sun: UV radiation ; Sunspots</subject><ispartof>Astrophysical journal. Letters, 2017-12, Vol.850 (2), p.L33</ispartof><rights>2017. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Dec 01, 2017</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c447t-1f268324625cf72b58e4ff3fed29fe44f5310586b190db3afed1420e11481b093</citedby><cites>FETCH-LOGICAL-c447t-1f268324625cf72b58e4ff3fed29fe44f5310586b190db3afed1420e11481b093</cites><orcidid>0000-0002-2093-085X ; 0000-0002-5865-7924 ; 0000-0001-9982-2175 ; 0000-0001-8619-9345 ; 0000-0001-6216-6944 ; 0000-0002-7737-740X ; 0000-0002-7073-868X ; 0000-0002-7358-9827</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/aa9a36/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>314,778,782,27911,27912,38855,38877,53827,53854</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/aa9a36$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc></links><search><creatorcontrib>Song, Donguk</creatorcontrib><creatorcontrib>Chae, Jongchul</creatorcontrib><creatorcontrib>Kwak, Hannah</creatorcontrib><creatorcontrib>Kano, Ryouhei</creatorcontrib><creatorcontrib>Yurchyshyn, Vasyl</creatorcontrib><creatorcontrib>Moon, Yong-Jae</creatorcontrib><creatorcontrib>Lim, Eun-Kyung</creatorcontrib><creatorcontrib>Lee, Jeongwoo</creatorcontrib><title>Three-minute Sunspot Oscillations Driven by Magnetic Reconnection in a Light Bridge</title><title>Astrophysical journal. Letters</title><addtitle>APJL</addtitle><addtitle>Astrophys. J. Lett</addtitle><description>We report a different type of three-minute chromospheric oscillation above a sunspot in association with a small-scale impulsive event in a light bridge (LB). During our observations, we found a transient brightening in the LB. The brightening was composed of elementary bursts that may be a manifestation of fast repetitive magnetic reconnections in the LB. Interestingly, the oscillations in the nearby sunspot umbra were impulsively excited when the intensity of the brightening reached its peak. The initial period of the oscillations was about 2.3 minutes and then gradually increased to 3.0 minutes with time. In addition, we found that the amplitude of the excited oscillations was twice the amplitude of oscillations before the brightening. Based on our results, we propose that magnetic reconnection occurring in an LB can excite oscillations in the nearby sunspot umbra.</description><subject>Amplitudes</subject><subject>Brightening</subject><subject>Magnetic reconnection</subject><subject>Oscillations</subject><subject>Sun: chromosphere</subject><subject>Sun: transition region</subject><subject>Sun: UV radiation</subject><subject>Sunspots</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp9kM9LwzAUx4MoOKd3jwHBk3X51TQ96vwJlYGb55C2yZbRpTVphf33tlTmRTy9x3uf73vwAeASo1sqWDIjiOFIEExnSqWK8iMwOYyODz2KT8FZCFuECOJYTMBytfFaRzvrulbDZedCU7dwEQpbVaq1tQvwwdsv7WC-h29q7XRrC_iui9o5XQwAtA4qmNn1poX33pZrfQ5OjKqCvvipU_Dx9Liav0TZ4vl1fpdFBWNJG2FDuKCEcRIXJiF5LDQzhhpdktRoxkxMMYoFz3GKypyqfoEZQRpjJnCOUjoFV-PdxtefnQ6t3Nadd_1LSSiPOScCJT2FRqrwdQheG9l4u1N-LzGSgzo5uJGDJzmq6yM3Y8TWze_Nf_DrP3DVbCspYiSJzCiVTWnoN6eue-E</recordid><startdate>20171201</startdate><enddate>20171201</enddate><creator>Song, Donguk</creator><creator>Chae, Jongchul</creator><creator>Kwak, Hannah</creator><creator>Kano, Ryouhei</creator><creator>Yurchyshyn, Vasyl</creator><creator>Moon, Yong-Jae</creator><creator>Lim, Eun-Kyung</creator><creator>Lee, Jeongwoo</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-2093-085X</orcidid><orcidid>https://orcid.org/0000-0002-5865-7924</orcidid><orcidid>https://orcid.org/0000-0001-9982-2175</orcidid><orcidid>https://orcid.org/0000-0001-8619-9345</orcidid><orcidid>https://orcid.org/0000-0001-6216-6944</orcidid><orcidid>https://orcid.org/0000-0002-7737-740X</orcidid><orcidid>https://orcid.org/0000-0002-7073-868X</orcidid><orcidid>https://orcid.org/0000-0002-7358-9827</orcidid></search><sort><creationdate>20171201</creationdate><title>Three-minute Sunspot Oscillations Driven by Magnetic Reconnection in a Light Bridge</title><author>Song, Donguk ; Chae, Jongchul ; Kwak, Hannah ; Kano, Ryouhei ; Yurchyshyn, Vasyl ; Moon, Yong-Jae ; Lim, Eun-Kyung ; Lee, Jeongwoo</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c447t-1f268324625cf72b58e4ff3fed29fe44f5310586b190db3afed1420e11481b093</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>Amplitudes</topic><topic>Brightening</topic><topic>Magnetic reconnection</topic><topic>Oscillations</topic><topic>Sun: chromosphere</topic><topic>Sun: transition region</topic><topic>Sun: UV radiation</topic><topic>Sunspots</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Song, Donguk</creatorcontrib><creatorcontrib>Chae, Jongchul</creatorcontrib><creatorcontrib>Kwak, Hannah</creatorcontrib><creatorcontrib>Kano, Ryouhei</creatorcontrib><creatorcontrib>Yurchyshyn, Vasyl</creatorcontrib><creatorcontrib>Moon, Yong-Jae</creatorcontrib><creatorcontrib>Lim, Eun-Kyung</creatorcontrib><creatorcontrib>Lee, Jeongwoo</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Song, Donguk</au><au>Chae, Jongchul</au><au>Kwak, Hannah</au><au>Kano, Ryouhei</au><au>Yurchyshyn, Vasyl</au><au>Moon, Yong-Jae</au><au>Lim, Eun-Kyung</au><au>Lee, Jeongwoo</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Three-minute Sunspot Oscillations Driven by Magnetic Reconnection in a Light Bridge</atitle><jtitle>Astrophysical journal. Letters</jtitle><stitle>APJL</stitle><addtitle>Astrophys. J. Lett</addtitle><date>2017-12-01</date><risdate>2017</risdate><volume>850</volume><issue>2</issue><spage>L33</spage><pages>L33-</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>We report a different type of three-minute chromospheric oscillation above a sunspot in association with a small-scale impulsive event in a light bridge (LB). During our observations, we found a transient brightening in the LB. The brightening was composed of elementary bursts that may be a manifestation of fast repetitive magnetic reconnections in the LB. Interestingly, the oscillations in the nearby sunspot umbra were impulsively excited when the intensity of the brightening reached its peak. The initial period of the oscillations was about 2.3 minutes and then gradually increased to 3.0 minutes with time. In addition, we found that the amplitude of the excited oscillations was twice the amplitude of oscillations before the brightening. Based on our results, we propose that magnetic reconnection occurring in an LB can excite oscillations in the nearby sunspot umbra.</abstract><cop>Austin</cop><pub>The American Astronomical Society</pub><doi>10.3847/2041-8213/aa9a36</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0002-2093-085X</orcidid><orcidid>https://orcid.org/0000-0002-5865-7924</orcidid><orcidid>https://orcid.org/0000-0001-9982-2175</orcidid><orcidid>https://orcid.org/0000-0001-8619-9345</orcidid><orcidid>https://orcid.org/0000-0001-6216-6944</orcidid><orcidid>https://orcid.org/0000-0002-7737-740X</orcidid><orcidid>https://orcid.org/0000-0002-7073-868X</orcidid><orcidid>https://orcid.org/0000-0002-7358-9827</orcidid><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 2041-8205
ispartof Astrophysical journal. Letters, 2017-12, Vol.850 (2), p.L33
issn 2041-8205
2041-8213
language eng
recordid cdi_proquest_journals_2365662807
source IOP Publishing Free Content
subjects Amplitudes
Brightening
Magnetic reconnection
Oscillations
Sun: chromosphere
Sun: transition region
Sun: UV radiation
Sunspots
title Three-minute Sunspot Oscillations Driven by Magnetic Reconnection in a Light Bridge
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-16T02%3A24%3A38IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Three-minute%20Sunspot%20Oscillations%20Driven%20by%20Magnetic%20Reconnection%20in%20a%20Light%20Bridge&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=Song,%20Donguk&rft.date=2017-12-01&rft.volume=850&rft.issue=2&rft.spage=L33&rft.pages=L33-&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.3847/2041-8213/aa9a36&rft_dat=%3Cproquest_O3W%3E2365662807%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2365662807&rft_id=info:pmid/&rfr_iscdi=true