Finding the dispersion of low-frequency waves in cosmic plasma from the results of multi-satellite measurements

An improved method of analysis of low-frequency wave processes in the interplanetary plasma using the results of multi-satellite measurements is presented. The new method develops the phase difference method and is distinguished by the fact that it allows one to analyze wavelengths several times sho...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Cosmic research 2008-04, Vol.46 (2), p.97-108
1. Verfasser: Romanov, S. A.
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 108
container_issue 2
container_start_page 97
container_title Cosmic research
container_volume 46
creator Romanov, S. A.
description An improved method of analysis of low-frequency wave processes in the interplanetary plasma using the results of multi-satellite measurements is presented. The new method develops the phase difference method and is distinguished by the fact that it allows one to analyze wavelengths several times shorter than the mean separation between spacecraft that perform the measurements. Its capabilities and the feasibility of analyzing events in different regions where spacecraft plasma measurements are undertaken are demonstrated using several examples of dispersion functions obtained by this method from the results of processing the magnetic field measurements on four spacecraft of the Cluster mission. The remarkable role played by ion-cyclotron oscillations in the outer magnetosphere cusp region is demonstrated, which manifests itself in wave generation and nonlinear structure formation.
doi_str_mv 10.1134/S0010952508020019
format Article
fullrecord <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_907982443</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2410112711</sourcerecordid><originalsourceid>FETCH-LOGICAL-c347t-9b1c40b4d6845ee9101c54ffb1a5943686474c4e160a6e1d875ac9d4d30495623</originalsourceid><addsrcrecordid>eNp1kU1LAzEQhoMoWD9-gLfgxdPqZDf7kaMUq0LBg3pe0uxsTdlNambX0n9vagVB8TQD8zzDDC9jFwKuhcjkzTOAAJWnOVSQxl4dsIkooEoyKPNDNtmNk938mJ0QrQBAlVkxYX5mXWPdkg9vyBtLawxkveO-5Z3fJG3A9xGd2fKN_kDi1nHjqbeGrztNveZt8P2XG5DGbqCd2MfGJqQH7Do7IO9R0xiwRzfQGTtqdUd4_l1P2evs7mX6kMyf7h-nt_PEZLIcErUQRsJCNkUlc0QlQJhctu1C6FzJrKgKWUojMb6oCxRNVebaqEY2GUiVF2l2yq72e9fBxw9oqHtLJh6kHfqRagWlqlIps0he_iJXfgwuHldXpSqqFEoRIbGHTPBEAdt6HWyvw7YWUO8CqP8EEJ1071Bk3RLDz-L_pU9oSofd</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>879682071</pqid></control><display><type>article</type><title>Finding the dispersion of low-frequency waves in cosmic plasma from the results of multi-satellite measurements</title><source>Springer Nature - Complete Springer Journals</source><creator>Romanov, S. A.</creator><creatorcontrib>Romanov, S. A.</creatorcontrib><description>An improved method of analysis of low-frequency wave processes in the interplanetary plasma using the results of multi-satellite measurements is presented. The new method develops the phase difference method and is distinguished by the fact that it allows one to analyze wavelengths several times shorter than the mean separation between spacecraft that perform the measurements. Its capabilities and the feasibility of analyzing events in different regions where spacecraft plasma measurements are undertaken are demonstrated using several examples of dispersion functions obtained by this method from the results of processing the magnetic field measurements on four spacecraft of the Cluster mission. The remarkable role played by ion-cyclotron oscillations in the outer magnetosphere cusp region is demonstrated, which manifests itself in wave generation and nonlinear structure formation.</description><identifier>ISSN: 0010-9525</identifier><identifier>EISSN: 1608-3075</identifier><identifier>DOI: 10.1134/S0010952508020019</identifier><language>eng</language><publisher>Dordrecht: SP MAIK Nauka/Interperiodica</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Physics ; Physics and Astronomy ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics</subject><ispartof>Cosmic research, 2008-04, Vol.46 (2), p.97-108</ispartof><rights>MAIK Nauka 2008</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c347t-9b1c40b4d6845ee9101c54ffb1a5943686474c4e160a6e1d875ac9d4d30495623</citedby><cites>FETCH-LOGICAL-c347t-9b1c40b4d6845ee9101c54ffb1a5943686474c4e160a6e1d875ac9d4d30495623</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S0010952508020019$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0010952508020019$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,777,781,27905,27906,41469,42538,51300</link.rule.ids></links><search><creatorcontrib>Romanov, S. A.</creatorcontrib><title>Finding the dispersion of low-frequency waves in cosmic plasma from the results of multi-satellite measurements</title><title>Cosmic research</title><addtitle>Cosmic Res</addtitle><description>An improved method of analysis of low-frequency wave processes in the interplanetary plasma using the results of multi-satellite measurements is presented. The new method develops the phase difference method and is distinguished by the fact that it allows one to analyze wavelengths several times shorter than the mean separation between spacecraft that perform the measurements. Its capabilities and the feasibility of analyzing events in different regions where spacecraft plasma measurements are undertaken are demonstrated using several examples of dispersion functions obtained by this method from the results of processing the magnetic field measurements on four spacecraft of the Cluster mission. The remarkable role played by ion-cyclotron oscillations in the outer magnetosphere cusp region is demonstrated, which manifests itself in wave generation and nonlinear structure formation.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><issn>0010-9525</issn><issn>1608-3075</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNp1kU1LAzEQhoMoWD9-gLfgxdPqZDf7kaMUq0LBg3pe0uxsTdlNambX0n9vagVB8TQD8zzDDC9jFwKuhcjkzTOAAJWnOVSQxl4dsIkooEoyKPNDNtmNk938mJ0QrQBAlVkxYX5mXWPdkg9vyBtLawxkveO-5Z3fJG3A9xGd2fKN_kDi1nHjqbeGrztNveZt8P2XG5DGbqCd2MfGJqQH7Do7IO9R0xiwRzfQGTtqdUd4_l1P2evs7mX6kMyf7h-nt_PEZLIcErUQRsJCNkUlc0QlQJhctu1C6FzJrKgKWUojMb6oCxRNVebaqEY2GUiVF2l2yq72e9fBxw9oqHtLJh6kHfqRagWlqlIps0he_iJXfgwuHldXpSqqFEoRIbGHTPBEAdt6HWyvw7YWUO8CqP8EEJ1071Bk3RLDz-L_pU9oSofd</recordid><startdate>200804</startdate><enddate>200804</enddate><creator>Romanov, S. A.</creator><general>SP MAIK Nauka/Interperiodica</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope></search><sort><creationdate>200804</creationdate><title>Finding the dispersion of low-frequency waves in cosmic plasma from the results of multi-satellite measurements</title><author>Romanov, S. A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c347t-9b1c40b4d6845ee9101c54ffb1a5943686474c4e160a6e1d875ac9d4d30495623</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2008</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Romanov, S. A.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Cosmic research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Romanov, S. A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Finding the dispersion of low-frequency waves in cosmic plasma from the results of multi-satellite measurements</atitle><jtitle>Cosmic research</jtitle><stitle>Cosmic Res</stitle><date>2008-04</date><risdate>2008</risdate><volume>46</volume><issue>2</issue><spage>97</spage><epage>108</epage><pages>97-108</pages><issn>0010-9525</issn><eissn>1608-3075</eissn><abstract>An improved method of analysis of low-frequency wave processes in the interplanetary plasma using the results of multi-satellite measurements is presented. The new method develops the phase difference method and is distinguished by the fact that it allows one to analyze wavelengths several times shorter than the mean separation between spacecraft that perform the measurements. Its capabilities and the feasibility of analyzing events in different regions where spacecraft plasma measurements are undertaken are demonstrated using several examples of dispersion functions obtained by this method from the results of processing the magnetic field measurements on four spacecraft of the Cluster mission. The remarkable role played by ion-cyclotron oscillations in the outer magnetosphere cusp region is demonstrated, which manifests itself in wave generation and nonlinear structure formation.</abstract><cop>Dordrecht</cop><pub>SP MAIK Nauka/Interperiodica</pub><doi>10.1134/S0010952508020019</doi><tpages>12</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0010-9525
ispartof Cosmic research, 2008-04, Vol.46 (2), p.97-108
issn 0010-9525
1608-3075
language eng
recordid cdi_proquest_miscellaneous_907982443
source Springer Nature - Complete Springer Journals
subjects Astronomy
Astrophysics and Astroparticles
Astrophysics and Cosmology
Physics
Physics and Astronomy
Space Exploration and Astronautics
Space Sciences (including Extraterrestrial Physics
title Finding the dispersion of low-frequency waves in cosmic plasma from the results of multi-satellite measurements
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-20T18%3A48%3A40IST&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=Finding%20the%20dispersion%20of%20low-frequency%20waves%20in%20cosmic%20plasma%20from%20the%20results%20of%20multi-satellite%20measurements&rft.jtitle=Cosmic%20research&rft.au=Romanov,%20S.%20A.&rft.date=2008-04&rft.volume=46&rft.issue=2&rft.spage=97&rft.epage=108&rft.pages=97-108&rft.issn=0010-9525&rft.eissn=1608-3075&rft_id=info:doi/10.1134/S0010952508020019&rft_dat=%3Cproquest_cross%3E2410112711%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=879682071&rft_id=info:pmid/&rfr_iscdi=true