Duration of wave disturbances generated by solar terminator in magneto-conjugate areas

We consider a possible explanation of long duration of travelling wave packets (TWPs) generated by solar terminator (ST). We suggest a hypothesis about consecutive detecting of MHD-nature disturbances, generated by ST in magneto-conjugate area first and in observation area next. Registration beginni...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Edemskiy, I. K., Yasyukevich, Y. V.
Format: Tagungsbericht
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 4
container_issue
container_start_page 1
container_title
container_volume
creator Edemskiy, I. K.
Yasyukevich, Y. V.
description We consider a possible explanation of long duration of travelling wave packets (TWPs) generated by solar terminator (ST). We suggest a hypothesis about consecutive detecting of MHD-nature disturbances, generated by ST in magneto-conjugate area first and in observation area next. Registration beginning time depends on latitude. In summer in Japan TWP registration starts with ST arriving in magneto-conjugate region - about 2-3 hours depending on latitude before ST arrives to the observation point. Dynamic spectra show clearly additive character of registered disturbances. ST appearance over the registration point accompanies amplitude increment on TWP frequencies in spectrum.
doi_str_mv 10.1109/URSIGASS.2011.6051003
format Conference Proceeding
fullrecord <record><control><sourceid>ieee_6IE</sourceid><recordid>TN_cdi_ieee_primary_6051003</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><ieee_id>6051003</ieee_id><sourcerecordid>6051003</sourcerecordid><originalsourceid>FETCH-LOGICAL-i90t-5afd8a74b23e48404e6f0069c27e362eaed7e4694b65c56d3cd075dfa3f25ab33</originalsourceid><addsrcrecordid>eNotUNtKAzEUjEhBW_sFIuQHtua-zWOpWgsFwVZfy9nN2ZLSzUqSKv17V9x5GYYZhmEIeeBsxjmzjx_v2_Vqsd3OBON8ZpjmjMkrMuZKKPUn1fUgNOelHpGxYMxaKZWyN2Sa0pH1MMZyLm_J59M5QvZdoF1Df-AbqfMpn2MFocZEDxiw99HR6kJTd4JIM8bWB8hdpD7QFg4Bc1fUXTieD32SQkRId2TUwCnhdOAJ2b0875avxeZttV4uNoW3LBcaGjeHUlVCoporptA0_TRbixKlEQjoSlTGqsroWhsna8dK7RqQjdBQSTkh9_-1HhH3X9G3EC_74RP5C_YNVdY</addsrcrecordid><sourcetype>Publisher</sourcetype><iscdi>true</iscdi><recordtype>conference_proceeding</recordtype></control><display><type>conference_proceeding</type><title>Duration of wave disturbances generated by solar terminator in magneto-conjugate areas</title><source>IEEE Electronic Library (IEL) Conference Proceedings</source><creator>Edemskiy, I. K. ; Yasyukevich, Y. V.</creator><creatorcontrib>Edemskiy, I. K. ; Yasyukevich, Y. V.</creatorcontrib><description>We consider a possible explanation of long duration of travelling wave packets (TWPs) generated by solar terminator (ST). We suggest a hypothesis about consecutive detecting of MHD-nature disturbances, generated by ST in magneto-conjugate area first and in observation area next. Registration beginning time depends on latitude. In summer in Japan TWP registration starts with ST arriving in magneto-conjugate region - about 2-3 hours depending on latitude before ST arrives to the observation point. Dynamic spectra show clearly additive character of registered disturbances. ST appearance over the registration point accompanies amplitude increment on TWP frequencies in spectrum.</description><identifier>ISBN: 1424451175</identifier><identifier>ISBN: 9781424451173</identifier><identifier>EISBN: 1424460514</identifier><identifier>EISBN: 1424451183</identifier><identifier>EISBN: 9781424460519</identifier><identifier>EISBN: 9781424451180</identifier><identifier>DOI: 10.1109/URSIGASS.2011.6051003</identifier><identifier>LCCN: 2009933449</identifier><language>eng</language><publisher>IEEE</publisher><subject>Additives ; Geometry ; Global Positioning System ; Green products ; Magnetic resonance imaging ; Magnetoacoustic effects ; Magnetohydrodynamics</subject><ispartof>2011 XXXth URSI General Assembly and Scientific Symposium, 2011, p.1-4</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/6051003$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>309,310,780,784,789,790,2058,27925,54920</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/6051003$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc></links><search><creatorcontrib>Edemskiy, I. K.</creatorcontrib><creatorcontrib>Yasyukevich, Y. V.</creatorcontrib><title>Duration of wave disturbances generated by solar terminator in magneto-conjugate areas</title><title>2011 XXXth URSI General Assembly and Scientific Symposium</title><addtitle>URSIGASS</addtitle><description>We consider a possible explanation of long duration of travelling wave packets (TWPs) generated by solar terminator (ST). We suggest a hypothesis about consecutive detecting of MHD-nature disturbances, generated by ST in magneto-conjugate area first and in observation area next. Registration beginning time depends on latitude. In summer in Japan TWP registration starts with ST arriving in magneto-conjugate region - about 2-3 hours depending on latitude before ST arrives to the observation point. Dynamic spectra show clearly additive character of registered disturbances. ST appearance over the registration point accompanies amplitude increment on TWP frequencies in spectrum.</description><subject>Additives</subject><subject>Geometry</subject><subject>Global Positioning System</subject><subject>Green products</subject><subject>Magnetic resonance imaging</subject><subject>Magnetoacoustic effects</subject><subject>Magnetohydrodynamics</subject><isbn>1424451175</isbn><isbn>9781424451173</isbn><isbn>1424460514</isbn><isbn>1424451183</isbn><isbn>9781424460519</isbn><isbn>9781424451180</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2011</creationdate><recordtype>conference_proceeding</recordtype><sourceid>6IE</sourceid><sourceid>RIE</sourceid><recordid>eNotUNtKAzEUjEhBW_sFIuQHtua-zWOpWgsFwVZfy9nN2ZLSzUqSKv17V9x5GYYZhmEIeeBsxjmzjx_v2_Vqsd3OBON8ZpjmjMkrMuZKKPUn1fUgNOelHpGxYMxaKZWyN2Sa0pH1MMZyLm_J59M5QvZdoF1Df-AbqfMpn2MFocZEDxiw99HR6kJTd4JIM8bWB8hdpD7QFg4Bc1fUXTieD32SQkRId2TUwCnhdOAJ2b0875avxeZttV4uNoW3LBcaGjeHUlVCoporptA0_TRbixKlEQjoSlTGqsroWhsna8dK7RqQjdBQSTkh9_-1HhH3X9G3EC_74RP5C_YNVdY</recordid><startdate>201108</startdate><enddate>201108</enddate><creator>Edemskiy, I. K.</creator><creator>Yasyukevich, Y. V.</creator><general>IEEE</general><scope>6IE</scope><scope>6IL</scope><scope>CBEJK</scope><scope>RIE</scope><scope>RIL</scope></search><sort><creationdate>201108</creationdate><title>Duration of wave disturbances generated by solar terminator in magneto-conjugate areas</title><author>Edemskiy, I. K. ; Yasyukevich, Y. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i90t-5afd8a74b23e48404e6f0069c27e362eaed7e4694b65c56d3cd075dfa3f25ab33</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2011</creationdate><topic>Additives</topic><topic>Geometry</topic><topic>Global Positioning System</topic><topic>Green products</topic><topic>Magnetic resonance imaging</topic><topic>Magnetoacoustic effects</topic><topic>Magnetohydrodynamics</topic><toplevel>online_resources</toplevel><creatorcontrib>Edemskiy, I. K.</creatorcontrib><creatorcontrib>Yasyukevich, Y. V.</creatorcontrib><collection>IEEE Electronic Library (IEL) Conference Proceedings</collection><collection>IEEE Proceedings Order Plan All Online (POP All Online) 1998-present by volume</collection><collection>IEEE Xplore All Conference Proceedings</collection><collection>IEEE Electronic Library Online</collection><collection>IEEE Proceedings Order Plans (POP All) 1998-Present</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Edemskiy, I. K.</au><au>Yasyukevich, Y. V.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Duration of wave disturbances generated by solar terminator in magneto-conjugate areas</atitle><btitle>2011 XXXth URSI General Assembly and Scientific Symposium</btitle><stitle>URSIGASS</stitle><date>2011-08</date><risdate>2011</risdate><spage>1</spage><epage>4</epage><pages>1-4</pages><isbn>1424451175</isbn><isbn>9781424451173</isbn><eisbn>1424460514</eisbn><eisbn>1424451183</eisbn><eisbn>9781424460519</eisbn><eisbn>9781424451180</eisbn><abstract>We consider a possible explanation of long duration of travelling wave packets (TWPs) generated by solar terminator (ST). We suggest a hypothesis about consecutive detecting of MHD-nature disturbances, generated by ST in magneto-conjugate area first and in observation area next. Registration beginning time depends on latitude. In summer in Japan TWP registration starts with ST arriving in magneto-conjugate region - about 2-3 hours depending on latitude before ST arrives to the observation point. Dynamic spectra show clearly additive character of registered disturbances. ST appearance over the registration point accompanies amplitude increment on TWP frequencies in spectrum.</abstract><pub>IEEE</pub><doi>10.1109/URSIGASS.2011.6051003</doi><tpages>4</tpages></addata></record>
fulltext fulltext_linktorsrc
identifier ISBN: 1424451175
ispartof 2011 XXXth URSI General Assembly and Scientific Symposium, 2011, p.1-4
issn
language eng
recordid cdi_ieee_primary_6051003
source IEEE Electronic Library (IEL) Conference Proceedings
subjects Additives
Geometry
Global Positioning System
Green products
Magnetic resonance imaging
Magnetoacoustic effects
Magnetohydrodynamics
title Duration of wave disturbances generated by solar terminator in magneto-conjugate areas
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T08%3A47%3A06IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-ieee_6IE&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=proceeding&rft.atitle=Duration%20of%20wave%20disturbances%20generated%20by%20solar%20terminator%20in%20magneto-conjugate%20areas&rft.btitle=2011%20XXXth%20URSI%20General%20Assembly%20and%20Scientific%20Symposium&rft.au=Edemskiy,%20I.%20K.&rft.date=2011-08&rft.spage=1&rft.epage=4&rft.pages=1-4&rft.isbn=1424451175&rft.isbn_list=9781424451173&rft_id=info:doi/10.1109/URSIGASS.2011.6051003&rft_dat=%3Cieee_6IE%3E6051003%3C/ieee_6IE%3E%3Curl%3E%3C/url%3E&rft.eisbn=1424460514&rft.eisbn_list=1424451183&rft.eisbn_list=9781424460519&rft.eisbn_list=9781424451180&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rft_ieee_id=6051003&rfr_iscdi=true