Correlation between the solar magnetic field strength and the millimeter brightness temperature
Central European Astrophysical Bulletin, 44, (2020) 2, 1-11 Images of the Sun at millimeter wavelengths obtained by ALMA show a significant correspondence with the magnetograms. In this paper, we investigate this correspondence by comparing ALMA full-disk solar image taken at 1.2 mm with a SDO/HMI m...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| 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 | |
| container_start_page | |
| container_title | |
| container_volume | |
| creator | Skokić, I Sudar, D Brajša, R |
| description | Central European Astrophysical Bulletin, 44, (2020) 2, 1-11 Images of the Sun at millimeter wavelengths obtained by ALMA show a
significant correspondence with the magnetograms. In this paper, we investigate
this correspondence by comparing ALMA full-disk solar image taken at 1.2 mm
with a SDO/HMI magnetogram and analyze their correlation. It is found that
chromospheric network and active regions show a positive correlation where
brightness temperature is increasing with the line-of-sight magnetic field
strength, while sunspots have a negative correlation. Quiet Sun regions do not
show any dependence of the brightness temperature with the magnetic field.
Thermal bremsstrahlung is given as the best explanation for the observed
correlations. |
| doi_str_mv | 10.48550/arxiv.2203.11747 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2203_11747</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2203_11747</sourcerecordid><originalsourceid>FETCH-LOGICAL-a677-9a3b82b59e49efff85f1e9a3ab86c000a08f7bb026f0df9922e6439bef9f86843</originalsourceid><addsrcrecordid>eNotz8lqxDAQBFBd5hBm8gE5RT9gR5Y36RhMNhjIZe6mNe62BbI8tJXt75M4ORUURcET4qZQeWXqWt0Bf_r3XGtV5kXRVu2V6LuFGQMkv0TpMH0gRpkmlOsSgOUMY8Tkz5I8hkGuiTGOaZIQh201-xD8jAlZOvbjlCKuq0w4X5AhvTEexI4grHj9n3txenw4dc_Z8fXppbs_ZtC0bWahdEa72mJlkYhMTQX-lOBMc1ZKgTLUOqd0Q2oga7XGpiqtQ7JkGlOVe3H7d7sJ-wv7Gfir_5X2m7T8Bo80UNo</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Correlation between the solar magnetic field strength and the millimeter brightness temperature</title><source>arXiv.org</source><creator>Skokić, I ; Sudar, D ; Brajša, R</creator><creatorcontrib>Skokić, I ; Sudar, D ; Brajša, R</creatorcontrib><description>Central European Astrophysical Bulletin, 44, (2020) 2, 1-11 Images of the Sun at millimeter wavelengths obtained by ALMA show a
significant correspondence with the magnetograms. In this paper, we investigate
this correspondence by comparing ALMA full-disk solar image taken at 1.2 mm
with a SDO/HMI magnetogram and analyze their correlation. It is found that
chromospheric network and active regions show a positive correlation where
brightness temperature is increasing with the line-of-sight magnetic field
strength, while sunspots have a negative correlation. Quiet Sun regions do not
show any dependence of the brightness temperature with the magnetic field.
Thermal bremsstrahlung is given as the best explanation for the observed
correlations.</description><identifier>DOI: 10.48550/arxiv.2203.11747</identifier><language>eng</language><subject>Physics - Solar and Stellar Astrophysics</subject><creationdate>2022-03</creationdate><rights>http://creativecommons.org/licenses/by/4.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2203.11747$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2203.11747$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Skokić, I</creatorcontrib><creatorcontrib>Sudar, D</creatorcontrib><creatorcontrib>Brajša, R</creatorcontrib><title>Correlation between the solar magnetic field strength and the millimeter brightness temperature</title><description>Central European Astrophysical Bulletin, 44, (2020) 2, 1-11 Images of the Sun at millimeter wavelengths obtained by ALMA show a
significant correspondence with the magnetograms. In this paper, we investigate
this correspondence by comparing ALMA full-disk solar image taken at 1.2 mm
with a SDO/HMI magnetogram and analyze their correlation. It is found that
chromospheric network and active regions show a positive correlation where
brightness temperature is increasing with the line-of-sight magnetic field
strength, while sunspots have a negative correlation. Quiet Sun regions do not
show any dependence of the brightness temperature with the magnetic field.
Thermal bremsstrahlung is given as the best explanation for the observed
correlations.</description><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotz8lqxDAQBFBd5hBm8gE5RT9gR5Y36RhMNhjIZe6mNe62BbI8tJXt75M4ORUURcET4qZQeWXqWt0Bf_r3XGtV5kXRVu2V6LuFGQMkv0TpMH0gRpkmlOsSgOUMY8Tkz5I8hkGuiTGOaZIQh201-xD8jAlZOvbjlCKuq0w4X5AhvTEexI4grHj9n3txenw4dc_Z8fXppbs_ZtC0bWahdEa72mJlkYhMTQX-lOBMc1ZKgTLUOqd0Q2oga7XGpiqtQ7JkGlOVe3H7d7sJ-wv7Gfir_5X2m7T8Bo80UNo</recordid><startdate>20220322</startdate><enddate>20220322</enddate><creator>Skokić, I</creator><creator>Sudar, D</creator><creator>Brajša, R</creator><scope>GOX</scope></search><sort><creationdate>20220322</creationdate><title>Correlation between the solar magnetic field strength and the millimeter brightness temperature</title><author>Skokić, I ; Sudar, D ; Brajša, R</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a677-9a3b82b59e49efff85f1e9a3ab86c000a08f7bb026f0df9922e6439bef9f86843</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Skokić, I</creatorcontrib><creatorcontrib>Sudar, D</creatorcontrib><creatorcontrib>Brajša, R</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Skokić, I</au><au>Sudar, D</au><au>Brajša, R</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Correlation between the solar magnetic field strength and the millimeter brightness temperature</atitle><date>2022-03-22</date><risdate>2022</risdate><abstract>Central European Astrophysical Bulletin, 44, (2020) 2, 1-11 Images of the Sun at millimeter wavelengths obtained by ALMA show a
significant correspondence with the magnetograms. In this paper, we investigate
this correspondence by comparing ALMA full-disk solar image taken at 1.2 mm
with a SDO/HMI magnetogram and analyze their correlation. It is found that
chromospheric network and active regions show a positive correlation where
brightness temperature is increasing with the line-of-sight magnetic field
strength, while sunspots have a negative correlation. Quiet Sun regions do not
show any dependence of the brightness temperature with the magnetic field.
Thermal bremsstrahlung is given as the best explanation for the observed
correlations.</abstract><doi>10.48550/arxiv.2203.11747</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.2203.11747 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_2203_11747 |
| source | arXiv.org |
| subjects | Physics - Solar and Stellar Astrophysics |
| title | Correlation between the solar magnetic field strength and the millimeter brightness temperature |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-01T13%3A40%3A38IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Correlation%20between%20the%20solar%20magnetic%20field%20strength%20and%20the%20millimeter%20brightness%20temperature&rft.au=Skoki%C4%87,%20I&rft.date=2022-03-22&rft_id=info:doi/10.48550/arxiv.2203.11747&rft_dat=%3Carxiv_GOX%3E2203_11747%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |