Polarization properties of the June 21, 2001 solar corona
Five series of coronal images have been obtained by V.Kulijanishvili during the total solar eclipse of the June 21, 2001, in Zambia, Lusaka. A photographic mirror-lens coronagraph-polarimeter (D=100 mm, F=1000 mm) was used. The absolute brightness, polarization and direction of polarization of the i...
Gespeichert in:
| Veröffentlicht in: | Proceedings of the International Astronomical Union 2006-03, Vol.2 (S233), p.255-256 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 256 |
|---|---|
| container_issue | S233 |
| container_start_page | 255 |
| container_title | Proceedings of the International Astronomical Union |
| container_volume | 2 |
| creator | Kapanadze, N. G. Kulijanishvili, V. I. Hady, Ahmed A. |
| description | Five series of coronal images have been obtained by V.Kulijanishvili during the total solar eclipse of the June 21, 2001, in Zambia, Lusaka. A photographic mirror-lens coronagraph-polarimeter (D=100 mm, F=1000 mm) was used. The absolute brightness, polarization and direction of polarization of the inner corona were measured. Standard techniques are used for the separation of the F- and K-coronas and for determination of coronal electron densities and temperatures. The background skylight polarization and intensity are calculated. |
| doi_str_mv | 10.1017/S1743921306001979 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_journals_225185560</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>10_1017_S1743921306001979</cupid><sourcerecordid>1401572211</sourcerecordid><originalsourceid>FETCH-LOGICAL-c231t-7e20c1f2b4a697732c898b9460b4e55d21af2d6279873317ff96062f76b39b303</originalsourceid><addsrcrecordid>eNp1kE9LxDAQxYMouK5-AG_Bs9XMpEmaoyz-ZUFBPZekTbTLblOT9qCf3pZd9CCeZhh-783jEXIK7AIYqMtnUDnXCJxJxkArvUdm0ynTiLD_swM_JEcprRjLZcHFjOinsDax-TJ9E1raxdC52Dcu0eBp_-7ow9A6inBOcbSlaYJpFWJozTE58Gad3MluzsnrzfXL4i5bPt7eL66WWYUc-kw5ZBV4tLmRWimOVaELq3PJbO6EqBGMx1qi0oXiHJT3WjKJXknLteWMz8nZ1ncM9zG41JerMMR2fFkiCiiEkBMEW6iKIaXofNnFZmPiZwmsnAoq_xQ0avhOYzY2NvWb-3X-X_UNt-5j3g</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>225185560</pqid></control><display><type>article</type><title>Polarization properties of the June 21, 2001 solar corona</title><source>Cambridge University Press Journals Complete</source><creator>Kapanadze, N. G. ; Kulijanishvili, V. I. ; Hady, Ahmed A.</creator><creatorcontrib>Kapanadze, N. G. ; Kulijanishvili, V. I. ; Hady, Ahmed A.</creatorcontrib><description>Five series of coronal images have been obtained by V.Kulijanishvili during the total solar eclipse of the June 21, 2001, in Zambia, Lusaka. A photographic mirror-lens coronagraph-polarimeter (D=100 mm, F=1000 mm) was used. The absolute brightness, polarization and direction of polarization of the inner corona were measured. Standard techniques are used for the separation of the F- and K-coronas and for determination of coronal electron densities and temperatures. The background skylight polarization and intensity are calculated.</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921306001979</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Contributed Papers ; Corona ; Electrons ; Solar eclipses ; Solar physics</subject><ispartof>Proceedings of the International Astronomical Union, 2006-03, Vol.2 (S233), p.255-256</ispartof><rights>2006 International Astronomical Union</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c231t-7e20c1f2b4a697732c898b9460b4e55d21af2d6279873317ff96062f76b39b303</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.cambridge.org/core/product/identifier/S1743921306001979/type/journal_article$$EHTML$$P50$$Gcambridge$$H</linktohtml><link.rule.ids>164,314,776,780,27903,27904,55607</link.rule.ids></links><search><creatorcontrib>Kapanadze, N. G.</creatorcontrib><creatorcontrib>Kulijanishvili, V. I.</creatorcontrib><creatorcontrib>Hady, Ahmed A.</creatorcontrib><title>Polarization properties of the June 21, 2001 solar corona</title><title>Proceedings of the International Astronomical Union</title><addtitle>Proc. IAU</addtitle><description>Five series of coronal images have been obtained by V.Kulijanishvili during the total solar eclipse of the June 21, 2001, in Zambia, Lusaka. A photographic mirror-lens coronagraph-polarimeter (D=100 mm, F=1000 mm) was used. The absolute brightness, polarization and direction of polarization of the inner corona were measured. Standard techniques are used for the separation of the F- and K-coronas and for determination of coronal electron densities and temperatures. The background skylight polarization and intensity are calculated.</description><subject>Contributed Papers</subject><subject>Corona</subject><subject>Electrons</subject><subject>Solar eclipses</subject><subject>Solar physics</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GNUQQ</sourceid><recordid>eNp1kE9LxDAQxYMouK5-AG_Bs9XMpEmaoyz-ZUFBPZekTbTLblOT9qCf3pZd9CCeZhh-783jEXIK7AIYqMtnUDnXCJxJxkArvUdm0ynTiLD_swM_JEcprRjLZcHFjOinsDax-TJ9E1raxdC52Dcu0eBp_-7ow9A6inBOcbSlaYJpFWJozTE58Gad3MluzsnrzfXL4i5bPt7eL66WWYUc-kw5ZBV4tLmRWimOVaELq3PJbO6EqBGMx1qi0oXiHJT3WjKJXknLteWMz8nZ1ncM9zG41JerMMR2fFkiCiiEkBMEW6iKIaXofNnFZmPiZwmsnAoq_xQ0avhOYzY2NvWb-3X-X_UNt-5j3g</recordid><startdate>200603</startdate><enddate>200603</enddate><creator>Kapanadze, N. G.</creator><creator>Kulijanishvili, V. I.</creator><creator>Hady, Ahmed A.</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope></search><sort><creationdate>200603</creationdate><title>Polarization properties of the June 21, 2001 solar corona</title><author>Kapanadze, N. G. ; Kulijanishvili, V. I. ; Hady, Ahmed A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c231t-7e20c1f2b4a697732c898b9460b4e55d21af2d6279873317ff96062f76b39b303</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>Contributed Papers</topic><topic>Corona</topic><topic>Electrons</topic><topic>Solar eclipses</topic><topic>Solar physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kapanadze, N. G.</creatorcontrib><creatorcontrib>Kulijanishvili, V. I.</creatorcontrib><creatorcontrib>Hady, Ahmed A.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</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>ProQuest Central Basic</collection><jtitle>Proceedings of the International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kapanadze, N. G.</au><au>Kulijanishvili, V. I.</au><au>Hady, Ahmed A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Polarization properties of the June 21, 2001 solar corona</atitle><jtitle>Proceedings of the International Astronomical Union</jtitle><addtitle>Proc. IAU</addtitle><date>2006-03</date><risdate>2006</risdate><volume>2</volume><issue>S233</issue><spage>255</spage><epage>256</epage><pages>255-256</pages><issn>1743-9213</issn><eissn>1743-9221</eissn><abstract>Five series of coronal images have been obtained by V.Kulijanishvili during the total solar eclipse of the June 21, 2001, in Zambia, Lusaka. A photographic mirror-lens coronagraph-polarimeter (D=100 mm, F=1000 mm) was used. The absolute brightness, polarization and direction of polarization of the inner corona were measured. Standard techniques are used for the separation of the F- and K-coronas and for determination of coronal electron densities and temperatures. The background skylight polarization and intensity are calculated.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921306001979</doi><tpages>2</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 1743-9213 |
| ispartof | Proceedings of the International Astronomical Union, 2006-03, Vol.2 (S233), p.255-256 |
| issn | 1743-9213 1743-9221 |
| language | eng |
| recordid | cdi_proquest_journals_225185560 |
| source | Cambridge University Press Journals Complete |
| subjects | Contributed Papers Corona Electrons Solar eclipses Solar physics |
| title | Polarization properties of the June 21, 2001 solar corona |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-22T13%3A24%3A51IST&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=Polarization%20properties%20of%20the%20June%2021,%202001%20solar%20corona&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.au=Kapanadze,%20N.%20G.&rft.date=2006-03&rft.volume=2&rft.issue=S233&rft.spage=255&rft.epage=256&rft.pages=255-256&rft.issn=1743-9213&rft.eissn=1743-9221&rft_id=info:doi/10.1017/S1743921306001979&rft_dat=%3Cproquest_cross%3E1401572211%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=225185560&rft_id=info:pmid/&rft_cupid=10_1017_S1743921306001979&rfr_iscdi=true |