Direct Measurement of AIA 171 Coronal Loop Transparency
Observations suggest that coronal loops should not be completely transparent. The transparency of coronal loops is rarely investigated in spite of its key role in coronal diagnostics. Here, we present an original investigation of Atmospheric Imaging Assembly 171 coronal loop transparency directly fr...
Gespeichert in:
Veröffentlicht in: | The Astrophysical journal 2022-08, Vol.934 (2), p.135 |
---|---|
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 | 135 |
container_title | The Astrophysical journal |
container_volume | 934 |
creator | li, Hongbo Feng, Hengqiang Tian, Zhanjun Zhang, Xuefei Liu, Jihong Zhao, Guoqing Zhao, Yan Cai, Hao Liang, Yuanxi Guo, Runze |
description | Observations suggest that coronal loops should not be completely transparent. The transparency of coronal loops is rarely investigated in spite of its key role in coronal diagnostics. Here, we present an original investigation of Atmospheric Imaging Assembly 171 coronal loop transparency directly from the radiation of visually intersecting coronal loops, which strongly indicates that the coronal loops may have significant opaqueness on the 171 Å radiation, and therefore should not be optical thin structures at least for some coronal lines. We suggest that this result may not only be helpful for explaining some basic observational features of coronal loops, but also in bringing new clues to the radiation-based diagnostics. |
doi_str_mv | 10.3847/1538-4357/ac7da5 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_crossref_primary_10_3847_1538_4357_ac7da5</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2697406395</sourcerecordid><originalsourceid>FETCH-LOGICAL-c263t-fdbc62014debff5ee7d9791f33dae6b66d09aff884130fd384ebaf43336dcec3</originalsourceid><addsrcrecordid>eNp9kE1LAzEQhoMoWKt3jwHx5tpkJ5tsjqVWLVS89OAtZPMBLe0mJttD_727rOhFPA0zPO8w8yB0S8kj1EzMaAV1waASM22E1dUZmvyMztGEEMIKDuLjEl3lvBvaUsoJEk_b5EyH35zOx-QOru1w8Hi-mmMqKF6EFFq9x-sQIt4k3eaok2vN6RpdeL3P7ua7TtHmeblZvBbr95fVYr4uTMmhK7xtDC8JZdY13lfOCSuFpB7Aascbzi2R2vu6ZhSIt_0nrtGeAQC3xhmYortxbUzh8-hyp3bhmPqLsiq5FIxwkFVPkZEyKeScnFcxbQ86nRQlarCjBhVqUKFGO33kYYxsQ_zd-Q9-_weu405JYKpUFCoVrYcvIbRybg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2697406395</pqid></control><display><type>article</type><title>Direct Measurement of AIA 171 Coronal Loop Transparency</title><source>IOP Publishing Free Content</source><source>DOAJ Directory of Open Access Journals</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>li, Hongbo ; Feng, Hengqiang ; Tian, Zhanjun ; Zhang, Xuefei ; Liu, Jihong ; Zhao, Guoqing ; Zhao, Yan ; Cai, Hao ; Liang, Yuanxi ; Guo, Runze</creator><creatorcontrib>li, Hongbo ; Feng, Hengqiang ; Tian, Zhanjun ; Zhang, Xuefei ; Liu, Jihong ; Zhao, Guoqing ; Zhao, Yan ; Cai, Hao ; Liang, Yuanxi ; Guo, Runze</creatorcontrib><description>Observations suggest that coronal loops should not be completely transparent. The transparency of coronal loops is rarely investigated in spite of its key role in coronal diagnostics. Here, we present an original investigation of Atmospheric Imaging Assembly 171 coronal loop transparency directly from the radiation of visually intersecting coronal loops, which strongly indicates that the coronal loops may have significant opaqueness on the 171 Å radiation, and therefore should not be optical thin structures at least for some coronal lines. We suggest that this result may not only be helpful for explaining some basic observational features of coronal loops, but also in bringing new clues to the radiation-based diagnostics.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ac7da5</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Active solar corona ; Astrophysics ; Coronal loops ; Radiation ; Solar coronal heating ; Solar coronal loops ; Transparency</subject><ispartof>The Astrophysical journal, 2022-08, Vol.934 (2), p.135</ispartof><rights>2022. The Author(s). Published by the American Astronomical Society.</rights><rights>2022. 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-c263t-fdbc62014debff5ee7d9791f33dae6b66d09aff884130fd384ebaf43336dcec3</cites><orcidid>0000-0002-0931-7552 ; 0000-0003-2632-8066 ; 0000-0003-1312-9308 ; 0000-0002-1831-1451 ; 0000-0002-3828-9837 ; 0000-0001-5649-6066</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/ac7da5/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,776,780,860,27903,27904,38869,53845</link.rule.ids></links><search><creatorcontrib>li, Hongbo</creatorcontrib><creatorcontrib>Feng, Hengqiang</creatorcontrib><creatorcontrib>Tian, Zhanjun</creatorcontrib><creatorcontrib>Zhang, Xuefei</creatorcontrib><creatorcontrib>Liu, Jihong</creatorcontrib><creatorcontrib>Zhao, Guoqing</creatorcontrib><creatorcontrib>Zhao, Yan</creatorcontrib><creatorcontrib>Cai, Hao</creatorcontrib><creatorcontrib>Liang, Yuanxi</creatorcontrib><creatorcontrib>Guo, Runze</creatorcontrib><title>Direct Measurement of AIA 171 Coronal Loop Transparency</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>Observations suggest that coronal loops should not be completely transparent. The transparency of coronal loops is rarely investigated in spite of its key role in coronal diagnostics. Here, we present an original investigation of Atmospheric Imaging Assembly 171 coronal loop transparency directly from the radiation of visually intersecting coronal loops, which strongly indicates that the coronal loops may have significant opaqueness on the 171 Å radiation, and therefore should not be optical thin structures at least for some coronal lines. We suggest that this result may not only be helpful for explaining some basic observational features of coronal loops, but also in bringing new clues to the radiation-based diagnostics.</description><subject>Active solar corona</subject><subject>Astrophysics</subject><subject>Coronal loops</subject><subject>Radiation</subject><subject>Solar coronal heating</subject><subject>Solar coronal loops</subject><subject>Transparency</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><recordid>eNp9kE1LAzEQhoMoWKt3jwHx5tpkJ5tsjqVWLVS89OAtZPMBLe0mJttD_727rOhFPA0zPO8w8yB0S8kj1EzMaAV1waASM22E1dUZmvyMztGEEMIKDuLjEl3lvBvaUsoJEk_b5EyH35zOx-QOru1w8Hi-mmMqKF6EFFq9x-sQIt4k3eaok2vN6RpdeL3P7ua7TtHmeblZvBbr95fVYr4uTMmhK7xtDC8JZdY13lfOCSuFpB7Aascbzi2R2vu6ZhSIt_0nrtGeAQC3xhmYortxbUzh8-hyp3bhmPqLsiq5FIxwkFVPkZEyKeScnFcxbQ86nRQlarCjBhVqUKFGO33kYYxsQ_zd-Q9-_weu405JYKpUFCoVrYcvIbRybg</recordid><startdate>20220801</startdate><enddate>20220801</enddate><creator>li, Hongbo</creator><creator>Feng, Hengqiang</creator><creator>Tian, Zhanjun</creator><creator>Zhang, Xuefei</creator><creator>Liu, Jihong</creator><creator>Zhao, Guoqing</creator><creator>Zhao, Yan</creator><creator>Cai, Hao</creator><creator>Liang, Yuanxi</creator><creator>Guo, Runze</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><orcidid>https://orcid.org/0000-0002-0931-7552</orcidid><orcidid>https://orcid.org/0000-0003-2632-8066</orcidid><orcidid>https://orcid.org/0000-0003-1312-9308</orcidid><orcidid>https://orcid.org/0000-0002-1831-1451</orcidid><orcidid>https://orcid.org/0000-0002-3828-9837</orcidid><orcidid>https://orcid.org/0000-0001-5649-6066</orcidid></search><sort><creationdate>20220801</creationdate><title>Direct Measurement of AIA 171 Coronal Loop Transparency</title><author>li, Hongbo ; Feng, Hengqiang ; Tian, Zhanjun ; Zhang, Xuefei ; Liu, Jihong ; Zhao, Guoqing ; Zhao, Yan ; Cai, Hao ; Liang, Yuanxi ; Guo, Runze</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c263t-fdbc62014debff5ee7d9791f33dae6b66d09aff884130fd384ebaf43336dcec3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Active solar corona</topic><topic>Astrophysics</topic><topic>Coronal loops</topic><topic>Radiation</topic><topic>Solar coronal heating</topic><topic>Solar coronal loops</topic><topic>Transparency</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>li, Hongbo</creatorcontrib><creatorcontrib>Feng, Hengqiang</creatorcontrib><creatorcontrib>Tian, Zhanjun</creatorcontrib><creatorcontrib>Zhang, Xuefei</creatorcontrib><creatorcontrib>Liu, Jihong</creatorcontrib><creatorcontrib>Zhao, Guoqing</creatorcontrib><creatorcontrib>Zhao, Yan</creatorcontrib><creatorcontrib>Cai, Hao</creatorcontrib><creatorcontrib>Liang, Yuanxi</creatorcontrib><creatorcontrib>Guo, Runze</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><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>li, Hongbo</au><au>Feng, Hengqiang</au><au>Tian, Zhanjun</au><au>Zhang, Xuefei</au><au>Liu, Jihong</au><au>Zhao, Guoqing</au><au>Zhao, Yan</au><au>Cai, Hao</au><au>Liang, Yuanxi</au><au>Guo, Runze</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Direct Measurement of AIA 171 Coronal Loop Transparency</atitle><jtitle>The Astrophysical journal</jtitle><stitle>APJ</stitle><addtitle>Astrophys. J</addtitle><date>2022-08-01</date><risdate>2022</risdate><volume>934</volume><issue>2</issue><spage>135</spage><pages>135-</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Observations suggest that coronal loops should not be completely transparent. The transparency of coronal loops is rarely investigated in spite of its key role in coronal diagnostics. Here, we present an original investigation of Atmospheric Imaging Assembly 171 coronal loop transparency directly from the radiation of visually intersecting coronal loops, which strongly indicates that the coronal loops may have significant opaqueness on the 171 Å radiation, and therefore should not be optical thin structures at least for some coronal lines. We suggest that this result may not only be helpful for explaining some basic observational features of coronal loops, but also in bringing new clues to the radiation-based diagnostics.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/ac7da5</doi><tpages>6</tpages><orcidid>https://orcid.org/0000-0002-0931-7552</orcidid><orcidid>https://orcid.org/0000-0003-2632-8066</orcidid><orcidid>https://orcid.org/0000-0003-1312-9308</orcidid><orcidid>https://orcid.org/0000-0002-1831-1451</orcidid><orcidid>https://orcid.org/0000-0002-3828-9837</orcidid><orcidid>https://orcid.org/0000-0001-5649-6066</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 0004-637X |
ispartof | The Astrophysical journal, 2022-08, Vol.934 (2), p.135 |
issn | 0004-637X 1538-4357 |
language | eng |
recordid | cdi_crossref_primary_10_3847_1538_4357_ac7da5 |
source | IOP Publishing Free Content; DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
subjects | Active solar corona Astrophysics Coronal loops Radiation Solar coronal heating Solar coronal loops Transparency |
title | Direct Measurement of AIA 171 Coronal Loop Transparency |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-24T09%3A46%3A12IST&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=Direct%20Measurement%20of%20AIA%20171%20Coronal%20Loop%20Transparency&rft.jtitle=The%20Astrophysical%20journal&rft.au=li,%20Hongbo&rft.date=2022-08-01&rft.volume=934&rft.issue=2&rft.spage=135&rft.pages=135-&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.3847/1538-4357/ac7da5&rft_dat=%3Cproquest_cross%3E2697406395%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=2697406395&rft_id=info:pmid/&rfr_iscdi=true |