Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001
The results of solar microwave observations in the Radio Astronomical Observatory NIRFI “Zimenki” are examined. Data analysis shows the presence of periodic component, that arose prior to burst connected to CMEs onset, and its absence after burst. Obtained data are compared with the dynamics of the...
Gespeichert in:
Veröffentlicht in: | Proceedings of the International Astronomical Union 2004-09, Vol.2004 (IAUS226), p.235-237 |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | 237 |
---|---|
container_issue | IAUS226 |
container_start_page | 235 |
container_title | Proceedings of the International Astronomical Union |
container_volume | 2004 |
creator | Sheiner, Olga A. Fridman, Vladimir M. |
description | The results of solar microwave observations in the Radio Astronomical Observatory NIRFI “Zimenki” are examined. Data analysis shows the presence of periodic component, that arose prior to burst connected to CMEs onset, and its absence after burst. Obtained data are compared with the dynamics of the development of activity on the solar disk. Results can be considered as the illustration of the dynamics of wave motions in the periods of flare activity.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html |
doi_str_mv | 10.1017/S1743921305000633 |
format | Article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_19655134</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>10_1017_S1743921305000633</cupid><sourcerecordid>1401573391</sourcerecordid><originalsourceid>FETCH-LOGICAL-c320t-107bf7e59599e63117ee2442122214a0b68215db8c86e192a4b818999c8d42e63</originalsourceid><addsrcrecordid>eNp1UMtOwzAQtBBIlMIHcLM4cCLgtfPyEUXlIRW1qOUcOcmmuEriYicg_h5XrUACcdrV7sxoZgg5B3YNDJKbBSShkBwEixhjsRAHZLQ9BZJzOPzeQRyTE-fWjIVxKqIRKZ4H5XQwR6tNpUuamXZjOux6R01NF6ZRlj7p0poP9Y500mrntOno3GKJWOluRZevSLOnCZ11DnvqfyDprOxNgfaKcsbglBzVqnF4tp9j8nI3WWYPwXR2_5jdToNScNYHwJKiTjCSkZQYC4AEkYchB-4ThIoVccohqoq0TGMEyVVYpJBKKcu0CrlnjMnlTndjzduArs-92xKbRnVoBpeDjKMIROiBF7-AazPYznvLOY-8tBRbNdiBfHbnLNb5xupW2c8cWL6tPP9TueeIPUe1hdXVCn-U_2d9Ab1zfv0</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>225192936</pqid></control><display><type>article</type><title>Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001</title><source>Cambridge Journals</source><creator>Sheiner, Olga A. ; Fridman, Vladimir M.</creator><creatorcontrib>Sheiner, Olga A. ; Fridman, Vladimir M.</creatorcontrib><description>The results of solar microwave observations in the Radio Astronomical Observatory NIRFI “Zimenki” are examined. Data analysis shows the presence of periodic component, that arose prior to burst connected to CMEs onset, and its absence after burst. Obtained data are compared with the dynamics of the development of activity on the solar disk. Results can be considered as the illustration of the dynamics of wave motions in the periods of flare activity.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921305000633</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Astronomy ; Contributed Papers</subject><ispartof>Proceedings of the International Astronomical Union, 2004-09, Vol.2004 (IAUS226), p.235-237</ispartof><rights>2005 International Astronomical Union</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c320t-107bf7e59599e63117ee2442122214a0b68215db8c86e192a4b818999c8d42e63</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.cambridge.org/core/product/identifier/S1743921305000633/type/journal_article$$EHTML$$P50$$Gcambridge$$H</linktohtml><link.rule.ids>164,315,781,785,27929,27930,55633</link.rule.ids></links><search><creatorcontrib>Sheiner, Olga A.</creatorcontrib><creatorcontrib>Fridman, Vladimir M.</creatorcontrib><title>Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001</title><title>Proceedings of the International Astronomical Union</title><addtitle>Proc. IAU</addtitle><description>The results of solar microwave observations in the Radio Astronomical Observatory NIRFI “Zimenki” are examined. Data analysis shows the presence of periodic component, that arose prior to burst connected to CMEs onset, and its absence after burst. Obtained data are compared with the dynamics of the development of activity on the solar disk. Results can be considered as the illustration of the dynamics of wave motions in the periods of flare activity.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html</description><subject>Astronomy</subject><subject>Contributed Papers</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</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>eNp1UMtOwzAQtBBIlMIHcLM4cCLgtfPyEUXlIRW1qOUcOcmmuEriYicg_h5XrUACcdrV7sxoZgg5B3YNDJKbBSShkBwEixhjsRAHZLQ9BZJzOPzeQRyTE-fWjIVxKqIRKZ4H5XQwR6tNpUuamXZjOux6R01NF6ZRlj7p0poP9Y500mrntOno3GKJWOluRZevSLOnCZ11DnvqfyDprOxNgfaKcsbglBzVqnF4tp9j8nI3WWYPwXR2_5jdToNScNYHwJKiTjCSkZQYC4AEkYchB-4ThIoVccohqoq0TGMEyVVYpJBKKcu0CrlnjMnlTndjzduArs-92xKbRnVoBpeDjKMIROiBF7-AazPYznvLOY-8tBRbNdiBfHbnLNb5xupW2c8cWL6tPP9TueeIPUe1hdXVCn-U_2d9Ab1zfv0</recordid><startdate>20040901</startdate><enddate>20040901</enddate><creator>Sheiner, Olga A.</creator><creator>Fridman, Vladimir M.</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><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20040901</creationdate><title>Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001</title><author>Sheiner, Olga A. ; Fridman, Vladimir M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c320t-107bf7e59599e63117ee2442122214a0b68215db8c86e192a4b818999c8d42e63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2004</creationdate><topic>Astronomy</topic><topic>Contributed Papers</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sheiner, Olga A.</creatorcontrib><creatorcontrib>Fridman, Vladimir M.</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><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Proceedings of the International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sheiner, Olga A.</au><au>Fridman, Vladimir M.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001</atitle><jtitle>Proceedings of the International Astronomical Union</jtitle><addtitle>Proc. IAU</addtitle><date>2004-09-01</date><risdate>2004</risdate><volume>2004</volume><issue>IAUS226</issue><spage>235</spage><epage>237</epage><pages>235-237</pages><issn>1743-9213</issn><eissn>1743-9221</eissn><abstract>The results of solar microwave observations in the Radio Astronomical Observatory NIRFI “Zimenki” are examined. Data analysis shows the presence of periodic component, that arose prior to burst connected to CMEs onset, and its absence after burst. Obtained data are compared with the dynamics of the development of activity on the solar disk. Results can be considered as the illustration of the dynamics of wave motions in the periods of flare activity.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921305000633</doi><tpages>3</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1743-9213 |
ispartof | Proceedings of the International Astronomical Union, 2004-09, Vol.2004 (IAUS226), p.235-237 |
issn | 1743-9213 1743-9221 |
language | eng |
recordid | cdi_proquest_miscellaneous_19655134 |
source | Cambridge Journals |
subjects | Astronomy Contributed Papers |
title | Quasi-Periodic Components of Solar Microwave Emission Preceeding The CME Onset on 19 October, 2001 |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-15T06%3A41%3A09IST&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=Quasi-Periodic%20Components%20of%20Solar%20Microwave%20Emission%20Preceeding%20The%20CME%20Onset%20on%2019%20October,%202001&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.au=Sheiner,%20Olga%20A.&rft.date=2004-09-01&rft.volume=2004&rft.issue=IAUS226&rft.spage=235&rft.epage=237&rft.pages=235-237&rft.issn=1743-9213&rft.eissn=1743-9221&rft_id=info:doi/10.1017/S1743921305000633&rft_dat=%3Cproquest_cross%3E1401573391%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=225192936&rft_id=info:pmid/&rft_cupid=10_1017_S1743921305000633&rfr_iscdi=true |