Solar Wind Origin in Coronal Funnels
The origin of the solar wind in solar coronal holes has long been unclear. We establish that the solar wind starts flowing out of the corona at heights above the photosphere between 5 megameters and 20 megameters in magnetic funnels. This result is obtained by a correlation of the Doppler-velocity a...
Gespeichert in:
| Veröffentlicht in: | Science (American Association for the Advancement of Science) 2005-04, Vol.308 (5721), p.519-523 |
|---|---|
| Hauptverfasser: | , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 523 |
|---|---|
| container_issue | 5721 |
| container_start_page | 519 |
| container_title | Science (American Association for the Advancement of Science) |
| container_volume | 308 |
| creator | Tu, Chuan-Yi Zhou, Cheng Marsch, Eckart Xia, Li-Dong Zhao, Liang Wang, Jing-Xiu Wilhelm, Klaus |
| description | The origin of the solar wind in solar coronal holes has long been unclear. We establish that the solar wind starts flowing out of the corona at heights above the photosphere between 5 megameters and 20 megameters in magnetic funnels. This result is obtained by a correlation of the Doppler-velocity and radiance maps of spectral lines emitted by various ions with the force-free magnetic field as extrapolated from photospheric magnetograms to different altitudes. Specifically, we find that Ne⁷⁺ ions mostly radiate around 20 megameters, where they have outflow speeds of about 10 kilometers per second, whereas C³⁺ ions with no average flow speed mainly radiate around 5 megameters. Based on these results, a model for understanding the solar wind origin is suggested. |
| doi_str_mv | 10.1126/science.1109447 |
| format | Article |
| fullrecord | <record><control><sourceid>gale_proqu</sourceid><recordid>TN_cdi_proquest_miscellaneous_743453974</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><galeid>A132192938</galeid><jstor_id>3841297</jstor_id><sourcerecordid>A132192938</sourcerecordid><originalsourceid>FETCH-LOGICAL-c897t-8f4dce9a6bc3f8285412ebb80bf15d8fe48d6ccb94d955422baa903ee644565d3</originalsourceid><addsrcrecordid>eNqN081v0zAUAHALgVgpnLkgqPgUh2z-jn0cFSuTKnoog6PlOE6UKrU3O5Hgv8dRI6aiaq1iyU78ey-R8x4ALxE8Rwjzi2ga64xNN1BSmj8Ck7RgmcSQPAYTCAnPBMzZGXgW4wbCtCfJU3CGmKBp8Al4v_atDrNfjStnq9DUjZulMffBO93OrnrnbBufgyeVbqN9Mc5TcHP19cf8W7ZcLa7nl8vMCJl3mahoaazUvDCkElgwirAtCgGLCrFSVJaKkhtTSFpKxijGhdYSEms5pYyzkkzBp13e2-Dvehs7tW2isW2rnfV9VDkllBGZpin4-KDkec4lFvwoHAxGDB-HiAqSDvAoRDmHEjKR4Nv_4Mb3IR3rkIxwDBFkCb3boVq3VjWu8l3QZsioLlH6MoklGVJlB1RtnQ269c5WTXq8588P-HSVdtuYgwGf9wKS6ezvrtZ9jOp6_f10u_p5uv2yONmKxfKhAxmt8W1ra6tSVc5X-_5i503wMQZbqdvQbHX4oxBUQyepsZPU2Ekp4vX49_pia8t7P7ZOAh9GoKPRbRW0M028dzznNOckuVc7t4mdD__2iUjdIYf3vNltV9orXYeU4madamOoNclTKZG_zzgvQA</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>213620105</pqid></control><display><type>article</type><title>Solar Wind Origin in Coronal Funnels</title><source>JSTOR Archive Collection A-Z Listing</source><source>American Association for the Advancement of Science</source><creator>Tu, Chuan-Yi ; Zhou, Cheng ; Marsch, Eckart ; Xia, Li-Dong ; Zhao, Liang ; Wang, Jing-Xiu ; Wilhelm, Klaus</creator><creatorcontrib>Tu, Chuan-Yi ; Zhou, Cheng ; Marsch, Eckart ; Xia, Li-Dong ; Zhao, Liang ; Wang, Jing-Xiu ; Wilhelm, Klaus</creatorcontrib><description>The origin of the solar wind in solar coronal holes has long been unclear. We establish that the solar wind starts flowing out of the corona at heights above the photosphere between 5 megameters and 20 megameters in magnetic funnels. This result is obtained by a correlation of the Doppler-velocity and radiance maps of spectral lines emitted by various ions with the force-free magnetic field as extrapolated from photospheric magnetograms to different altitudes. Specifically, we find that Ne⁷⁺ ions mostly radiate around 20 megameters, where they have outflow speeds of about 10 kilometers per second, whereas C³⁺ ions with no average flow speed mainly radiate around 5 megameters. Based on these results, a model for understanding the solar wind origin is suggested.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1109447</identifier><identifier>PMID: 15845846</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Analysis ; Astronomy ; Chromosphere ; Corona. Coronal loops, streamers, and holes ; Coronal mass ejections ; Correlations ; Data Analysis ; Doppler effect ; Earth, ocean, space ; Exact sciences and technology ; Interplanetary space ; Magnetic fields ; Mathematical extrapolation ; Observations ; Particle radiation, solar wind ; Physics ; Radiance ; Radiation ; Rectangles ; Solar energy ; Solar physics ; Solar system ; Solar wind ; Solar wind plasma ; Spectrometer ; Spectrometers ; Sumer ; Wind</subject><ispartof>Science (American Association for the Advancement of Science), 2005-04, Vol.308 (5721), p.519-523</ispartof><rights>Copyright 2005 American Association for the Advancement of Science</rights><rights>2005 INIST-CNRS</rights><rights>COPYRIGHT 2005 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Apr 22, 2005</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c897t-8f4dce9a6bc3f8285412ebb80bf15d8fe48d6ccb94d955422baa903ee644565d3</citedby><cites>FETCH-LOGICAL-c897t-8f4dce9a6bc3f8285412ebb80bf15d8fe48d6ccb94d955422baa903ee644565d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/3841297$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/3841297$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>315,782,786,805,2886,2887,27931,27932,58024,58257</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=16764763$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/15845846$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Tu, Chuan-Yi</creatorcontrib><creatorcontrib>Zhou, Cheng</creatorcontrib><creatorcontrib>Marsch, Eckart</creatorcontrib><creatorcontrib>Xia, Li-Dong</creatorcontrib><creatorcontrib>Zhao, Liang</creatorcontrib><creatorcontrib>Wang, Jing-Xiu</creatorcontrib><creatorcontrib>Wilhelm, Klaus</creatorcontrib><title>Solar Wind Origin in Coronal Funnels</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>The origin of the solar wind in solar coronal holes has long been unclear. We establish that the solar wind starts flowing out of the corona at heights above the photosphere between 5 megameters and 20 megameters in magnetic funnels. This result is obtained by a correlation of the Doppler-velocity and radiance maps of spectral lines emitted by various ions with the force-free magnetic field as extrapolated from photospheric magnetograms to different altitudes. Specifically, we find that Ne⁷⁺ ions mostly radiate around 20 megameters, where they have outflow speeds of about 10 kilometers per second, whereas C³⁺ ions with no average flow speed mainly radiate around 5 megameters. Based on these results, a model for understanding the solar wind origin is suggested.</description><subject>Analysis</subject><subject>Astronomy</subject><subject>Chromosphere</subject><subject>Corona. Coronal loops, streamers, and holes</subject><subject>Coronal mass ejections</subject><subject>Correlations</subject><subject>Data Analysis</subject><subject>Doppler effect</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Interplanetary space</subject><subject>Magnetic fields</subject><subject>Mathematical extrapolation</subject><subject>Observations</subject><subject>Particle radiation, solar wind</subject><subject>Physics</subject><subject>Radiance</subject><subject>Radiation</subject><subject>Rectangles</subject><subject>Solar energy</subject><subject>Solar physics</subject><subject>Solar system</subject><subject>Solar wind</subject><subject>Solar wind plasma</subject><subject>Spectrometer</subject><subject>Spectrometers</subject><subject>Sumer</subject><subject>Wind</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2005</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNqN081v0zAUAHALgVgpnLkgqPgUh2z-jn0cFSuTKnoog6PlOE6UKrU3O5Hgv8dRI6aiaq1iyU78ey-R8x4ALxE8Rwjzi2ga64xNN1BSmj8Ck7RgmcSQPAYTCAnPBMzZGXgW4wbCtCfJU3CGmKBp8Al4v_atDrNfjStnq9DUjZulMffBO93OrnrnbBufgyeVbqN9Mc5TcHP19cf8W7ZcLa7nl8vMCJl3mahoaazUvDCkElgwirAtCgGLCrFSVJaKkhtTSFpKxijGhdYSEms5pYyzkkzBp13e2-Dvehs7tW2isW2rnfV9VDkllBGZpin4-KDkec4lFvwoHAxGDB-HiAqSDvAoRDmHEjKR4Nv_4Mb3IR3rkIxwDBFkCb3boVq3VjWu8l3QZsioLlH6MoklGVJlB1RtnQ269c5WTXq8588P-HSVdtuYgwGf9wKS6ezvrtZ9jOp6_f10u_p5uv2yONmKxfKhAxmt8W1ra6tSVc5X-_5i503wMQZbqdvQbHX4oxBUQyepsZPU2Ekp4vX49_pia8t7P7ZOAh9GoKPRbRW0M028dzznNOckuVc7t4mdD__2iUjdIYf3vNltV9orXYeU4madamOoNclTKZG_zzgvQA</recordid><startdate>20050422</startdate><enddate>20050422</enddate><creator>Tu, Chuan-Yi</creator><creator>Zhou, Cheng</creator><creator>Marsch, Eckart</creator><creator>Xia, Li-Dong</creator><creator>Zhao, Liang</creator><creator>Wang, Jing-Xiu</creator><creator>Wilhelm, Klaus</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>FBQ</scope><scope>IQODW</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8GL</scope><scope>IBG</scope><scope>IOV</scope><scope>ISN</scope><scope>0-V</scope><scope>3V.</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88B</scope><scope>88E</scope><scope>88I</scope><scope>8AF</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ALSLI</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>CJNVE</scope><scope>D1I</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9-</scope><scope>K9.</scope><scope>KB.</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>LK8</scope><scope>L~C</scope><scope>L~D</scope><scope>M0K</scope><scope>M0P</scope><scope>M0R</scope><scope>M0S</scope><scope>M1P</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEDU</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope><scope>7X8</scope></search><sort><creationdate>20050422</creationdate><title>Solar Wind Origin in Coronal Funnels</title><author>Tu, Chuan-Yi ; Zhou, Cheng ; Marsch, Eckart ; Xia, Li-Dong ; Zhao, Liang ; Wang, Jing-Xiu ; Wilhelm, Klaus</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c897t-8f4dce9a6bc3f8285412ebb80bf15d8fe48d6ccb94d955422baa903ee644565d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2005</creationdate><topic>Analysis</topic><topic>Astronomy</topic><topic>Chromosphere</topic><topic>Corona. Coronal loops, streamers, and holes</topic><topic>Coronal mass ejections</topic><topic>Correlations</topic><topic>Data Analysis</topic><topic>Doppler effect</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Interplanetary space</topic><topic>Magnetic fields</topic><topic>Mathematical extrapolation</topic><topic>Observations</topic><topic>Particle radiation, solar wind</topic><topic>Physics</topic><topic>Radiance</topic><topic>Radiation</topic><topic>Rectangles</topic><topic>Solar energy</topic><topic>Solar physics</topic><topic>Solar system</topic><topic>Solar wind</topic><topic>Solar wind plasma</topic><topic>Spectrometer</topic><topic>Spectrometers</topic><topic>Sumer</topic><topic>Wind</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Tu, Chuan-Yi</creatorcontrib><creatorcontrib>Zhou, Cheng</creatorcontrib><creatorcontrib>Marsch, Eckart</creatorcontrib><creatorcontrib>Xia, Li-Dong</creatorcontrib><creatorcontrib>Zhao, Liang</creatorcontrib><creatorcontrib>Wang, Jing-Xiu</creatorcontrib><creatorcontrib>Wilhelm, Klaus</creatorcontrib><collection>AGRIS</collection><collection>Pascal-Francis</collection><collection>PubMed</collection><collection>CrossRef</collection><collection>Gale In Context: High School</collection><collection>Gale In Context: Biography</collection><collection>Gale In Context: Opposing Viewpoints</collection><collection>Gale In Context: Canada</collection><collection>ProQuest Social Sciences Premium Collection</collection><collection>ProQuest Central (Corporate)</collection><collection>Aluminium Industry Abstracts</collection><collection>Animal Behavior Abstracts</collection><collection>Bacteriology Abstracts (Microbiology B)</collection><collection>Calcium & Calcified Tissue Abstracts</collection><collection>Ceramic Abstracts</collection><collection>Chemoreception Abstracts</collection><collection>Computer and Information Systems Abstracts</collection><collection>Corrosion Abstracts</collection><collection>Ecology Abstracts</collection><collection>Electronics & Communications Abstracts</collection><collection>Engineered Materials Abstracts</collection><collection>Entomology Abstracts (Full archive)</collection><collection>Industrial and Applied Microbiology Abstracts (Microbiology A)</collection><collection>Materials Business File</collection><collection>Mechanical & Transportation Engineering Abstracts</collection><collection>Neurosciences Abstracts</collection><collection>Nucleic Acids Abstracts</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Virology and AIDS Abstracts</collection><collection>Agricultural Science Collection</collection><collection>Health & Medical Collection</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Biology Database (Alumni Edition)</collection><collection>Education Database (Alumni Edition)</collection><collection>Medical Database (Alumni Edition)</collection><collection>Science Database (Alumni Edition)</collection><collection>STEM Database</collection><collection>METADEX</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Natural Science Collection</collection><collection>Hospital Premium Collection</collection><collection>Hospital Premium Collection (Alumni Edition)</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>Research Library (Alumni Edition)</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Social Science Premium Collection</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>Agricultural & Environmental Science Collection</collection><collection>ProQuest Central Essentials</collection><collection>Biological Science Collection</collection><collection>eLibrary</collection><collection>ProQuest Central</collection><collection>Technology Collection (ProQuest)</collection><collection>Natural Science Collection (ProQuest)</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>Environmental Sciences and Pollution Management</collection><collection>ProQuest One Community College</collection><collection>Education Collection</collection><collection>ProQuest Materials Science Collection</collection><collection>ProQuest Central Korea</collection><collection>ANTE: Abstracts in New Technology & Engineering</collection><collection>Engineering Research Database</collection><collection>Health Research Premium Collection</collection><collection>Health Research Premium Collection (Alumni)</collection><collection>ProQuest Central Student</collection><collection>Research Library Prep</collection><collection>Aerospace Database</collection><collection>Copper Technical Reference Library</collection><collection>AIDS and Cancer Research Abstracts</collection><collection>SciTech Premium Collection</collection><collection>Materials Research Database</collection><collection>ProQuest Computer Science Collection</collection><collection>Consumer Health Database (Alumni Edition)</collection><collection>ProQuest Health & Medical Complete (Alumni)</collection><collection>Materials Science Database</collection><collection>Civil Engineering Abstracts</collection><collection>ProQuest Engineering Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>ProQuest Biological Science Collection</collection><collection>Computer and Information Systems Abstracts Academic</collection><collection>Computer and Information Systems Abstracts Professional</collection><collection>Agricultural Science Database</collection><collection>Education Database</collection><collection>Consumer Health Database</collection><collection>Health & Medical Collection (Alumni Edition)</collection><collection>Medical Database</collection><collection>Research Library</collection><collection>Science Database (ProQuest)</collection><collection>Algology Mycology and Protozoology Abstracts (Microbiology C)</collection><collection>Biological Science Database</collection><collection>Engineering Database</collection><collection>Research Library (Corporate)</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Biotechnology and BioEngineering Abstracts</collection><collection>Environmental Science Database</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>Materials Science Collection</collection><collection>ProQuest One Education</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><collection>Environmental Science Collection</collection><collection>ProQuest Central Basic</collection><collection>University of Michigan</collection><collection>Genetics Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>MEDLINE - Academic</collection><jtitle>Science (American Association for the Advancement of Science)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Tu, Chuan-Yi</au><au>Zhou, Cheng</au><au>Marsch, Eckart</au><au>Xia, Li-Dong</au><au>Zhao, Liang</au><au>Wang, Jing-Xiu</au><au>Wilhelm, Klaus</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Solar Wind Origin in Coronal Funnels</atitle><jtitle>Science (American Association for the Advancement of Science)</jtitle><addtitle>Science</addtitle><date>2005-04-22</date><risdate>2005</risdate><volume>308</volume><issue>5721</issue><spage>519</spage><epage>523</epage><pages>519-523</pages><issn>0036-8075</issn><eissn>1095-9203</eissn><coden>SCIEAS</coden><abstract>The origin of the solar wind in solar coronal holes has long been unclear. We establish that the solar wind starts flowing out of the corona at heights above the photosphere between 5 megameters and 20 megameters in magnetic funnels. This result is obtained by a correlation of the Doppler-velocity and radiance maps of spectral lines emitted by various ions with the force-free magnetic field as extrapolated from photospheric magnetograms to different altitudes. Specifically, we find that Ne⁷⁺ ions mostly radiate around 20 megameters, where they have outflow speeds of about 10 kilometers per second, whereas C³⁺ ions with no average flow speed mainly radiate around 5 megameters. Based on these results, a model for understanding the solar wind origin is suggested.</abstract><cop>Washington, DC</cop><pub>American Association for the Advancement of Science</pub><pmid>15845846</pmid><doi>10.1126/science.1109447</doi><tpages>5</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0036-8075 |
| ispartof | Science (American Association for the Advancement of Science), 2005-04, Vol.308 (5721), p.519-523 |
| issn | 0036-8075 1095-9203 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_743453974 |
| source | JSTOR Archive Collection A-Z Listing; American Association for the Advancement of Science |
| subjects | Analysis Astronomy Chromosphere Corona. Coronal loops, streamers, and holes Coronal mass ejections Correlations Data Analysis Doppler effect Earth, ocean, space Exact sciences and technology Interplanetary space Magnetic fields Mathematical extrapolation Observations Particle radiation, solar wind Physics Radiance Radiation Rectangles Solar energy Solar physics Solar system Solar wind Solar wind plasma Spectrometer Spectrometers Sumer Wind |
| title | Solar Wind Origin in Coronal Funnels |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-05T03%3A03%3A49IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-gale_proqu&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Solar%20Wind%20Origin%20in%20Coronal%20Funnels&rft.jtitle=Science%20(American%20Association%20for%20the%20Advancement%20of%20Science)&rft.au=Tu,%20Chuan-Yi&rft.date=2005-04-22&rft.volume=308&rft.issue=5721&rft.spage=519&rft.epage=523&rft.pages=519-523&rft.issn=0036-8075&rft.eissn=1095-9203&rft.coden=SCIEAS&rft_id=info:doi/10.1126/science.1109447&rft_dat=%3Cgale_proqu%3EA132192938%3C/gale_proqu%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=213620105&rft_id=info:pmid/15845846&rft_galeid=A132192938&rft_jstor_id=3841297&rfr_iscdi=true |