Numerical simulations of type-III solar radio bursts
The first numerical simulations are presented for type-III solar radio bursts in the inhomogeneous solar corona and interplanetary space, that include microscale quasilinear and nonlinear processes, intermediate-scale driven ambient density fluctuations, and large scale evolution of electron beams,...
Gespeichert in:
| Veröffentlicht in: | Physical review letters 2006-04, Vol.96 (14), p.145005-145005, Article 145005 |
|---|---|
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 145005 |
|---|---|
| container_issue | 14 |
| container_start_page | 145005 |
| container_title | Physical review letters |
| container_volume | 96 |
| creator | Li, B Robinson, P A Cairns, I H |
| description | The first numerical simulations are presented for type-III solar radio bursts in the inhomogeneous solar corona and interplanetary space, that include microscale quasilinear and nonlinear processes, intermediate-scale driven ambient density fluctuations, and large scale evolution of electron beams, Langmuir and ion sound waves, and fundamental and harmonic electromagnetic emission. Bidirectional coronal emission is asymmetric between the upward and downward directions, and harmonic emission dominates fundamental emission. In interplanetary space, fundamental and/or harmonic emission can be important. Langmuir and ion sound waves are bursty and the statistics of Langmuir wave energy agree well with the predictions of stochastic growth theory. |
| doi_str_mv | 10.1103/PhysRevLett.96.145005 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_20775167</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>67998964</sourcerecordid><originalsourceid>FETCH-LOGICAL-c335t-8950148c53d013a3bd4e5300af27570f18881319fdeb25e6df6e78203f0b7a383</originalsourceid><addsrcrecordid>eNpNkF1LwzAUhoMobk5_glIQvOs8p2ma5FKGH4OhInod0jRllbaZSSrs31vpQK_em-c9h_ch5BJhiQj09nW7D2_2e2NjXMpiiTkDYEdkjsBlyhHzYzIHoJhKAD4jZyF8AgBmhTglMyw4ZiD4nOTPQ2d9Y3SbhKYbWh0b14fE1Unc72y6Xq-T4FrtE6-rxiXl4EMM5-Sk1m2wF4dckI-H-_fVU7p5eVyv7japoZTFVEgGmAvDaAVINS2r3DIKoOuMMw41CiGQoqwrW2bMFlVdWC4yoDWUXFNBF-R6uutCbFQwTbRma1zfWxNVBpyzcchI3UzUzruvwYaouiYY27a6t24IquBSClnkI8gm0HgXgre12vmm036vENSvVPVPqpKFmqSOvavDg6HsbPXXOlikPyBpc8s</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>67998964</pqid></control><display><type>article</type><title>Numerical simulations of type-III solar radio bursts</title><source>American Physical Society Journals</source><creator>Li, B ; Robinson, P A ; Cairns, I H</creator><creatorcontrib>Li, B ; Robinson, P A ; Cairns, I H</creatorcontrib><description>The first numerical simulations are presented for type-III solar radio bursts in the inhomogeneous solar corona and interplanetary space, that include microscale quasilinear and nonlinear processes, intermediate-scale driven ambient density fluctuations, and large scale evolution of electron beams, Langmuir and ion sound waves, and fundamental and harmonic electromagnetic emission. Bidirectional coronal emission is asymmetric between the upward and downward directions, and harmonic emission dominates fundamental emission. In interplanetary space, fundamental and/or harmonic emission can be important. Langmuir and ion sound waves are bursty and the statistics of Langmuir wave energy agree well with the predictions of stochastic growth theory.</description><identifier>ISSN: 0031-9007</identifier><identifier>EISSN: 1079-7114</identifier><identifier>DOI: 10.1103/PhysRevLett.96.145005</identifier><identifier>PMID: 16712087</identifier><language>eng</language><publisher>United States</publisher><subject>ASYMMETRY ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; ELECTRON BEAMS ; EMISSION ; EVOLUTION ; FLUCTUATIONS ; INTERPLANETARY SPACE ; ION WAVES ; LANGMUIR FREQUENCY ; NONLINEAR PROBLEMS ; NUMERICAL ANALYSIS ; PLASMA ; SIMULATION ; SOLAR CORONA ; SOLAR RADIO BURSTS ; SOUND WAVES ; STATISTICS</subject><ispartof>Physical review letters, 2006-04, Vol.96 (14), p.145005-145005, Article 145005</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c335t-8950148c53d013a3bd4e5300af27570f18881319fdeb25e6df6e78203f0b7a383</citedby><cites>FETCH-LOGICAL-c335t-8950148c53d013a3bd4e5300af27570f18881319fdeb25e6df6e78203f0b7a383</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,2863,2864,27901,27902</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/16712087$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/20775167$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Li, B</creatorcontrib><creatorcontrib>Robinson, P A</creatorcontrib><creatorcontrib>Cairns, I H</creatorcontrib><title>Numerical simulations of type-III solar radio bursts</title><title>Physical review letters</title><addtitle>Phys Rev Lett</addtitle><description>The first numerical simulations are presented for type-III solar radio bursts in the inhomogeneous solar corona and interplanetary space, that include microscale quasilinear and nonlinear processes, intermediate-scale driven ambient density fluctuations, and large scale evolution of electron beams, Langmuir and ion sound waves, and fundamental and harmonic electromagnetic emission. Bidirectional coronal emission is asymmetric between the upward and downward directions, and harmonic emission dominates fundamental emission. In interplanetary space, fundamental and/or harmonic emission can be important. Langmuir and ion sound waves are bursty and the statistics of Langmuir wave energy agree well with the predictions of stochastic growth theory.</description><subject>ASYMMETRY</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>ELECTRON BEAMS</subject><subject>EMISSION</subject><subject>EVOLUTION</subject><subject>FLUCTUATIONS</subject><subject>INTERPLANETARY SPACE</subject><subject>ION WAVES</subject><subject>LANGMUIR FREQUENCY</subject><subject>NONLINEAR PROBLEMS</subject><subject>NUMERICAL ANALYSIS</subject><subject>PLASMA</subject><subject>SIMULATION</subject><subject>SOLAR CORONA</subject><subject>SOLAR RADIO BURSTS</subject><subject>SOUND WAVES</subject><subject>STATISTICS</subject><issn>0031-9007</issn><issn>1079-7114</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNpNkF1LwzAUhoMobk5_glIQvOs8p2ma5FKGH4OhInod0jRllbaZSSrs31vpQK_em-c9h_ch5BJhiQj09nW7D2_2e2NjXMpiiTkDYEdkjsBlyhHzYzIHoJhKAD4jZyF8AgBmhTglMyw4ZiD4nOTPQ2d9Y3SbhKYbWh0b14fE1Unc72y6Xq-T4FrtE6-rxiXl4EMM5-Sk1m2wF4dckI-H-_fVU7p5eVyv7japoZTFVEgGmAvDaAVINS2r3DIKoOuMMw41CiGQoqwrW2bMFlVdWC4yoDWUXFNBF-R6uutCbFQwTbRma1zfWxNVBpyzcchI3UzUzruvwYaouiYY27a6t24IquBSClnkI8gm0HgXgre12vmm036vENSvVPVPqpKFmqSOvavDg6HsbPXXOlikPyBpc8s</recordid><startdate>20060414</startdate><enddate>20060414</enddate><creator>Li, B</creator><creator>Robinson, P A</creator><creator>Cairns, I H</creator><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7X8</scope><scope>OTOTI</scope></search><sort><creationdate>20060414</creationdate><title>Numerical simulations of type-III solar radio bursts</title><author>Li, B ; Robinson, P A ; Cairns, I H</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c335t-8950148c53d013a3bd4e5300af27570f18881319fdeb25e6df6e78203f0b7a383</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2006</creationdate><topic>ASYMMETRY</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>ELECTRON BEAMS</topic><topic>EMISSION</topic><topic>EVOLUTION</topic><topic>FLUCTUATIONS</topic><topic>INTERPLANETARY SPACE</topic><topic>ION WAVES</topic><topic>LANGMUIR FREQUENCY</topic><topic>NONLINEAR PROBLEMS</topic><topic>NUMERICAL ANALYSIS</topic><topic>PLASMA</topic><topic>SIMULATION</topic><topic>SOLAR CORONA</topic><topic>SOLAR RADIO BURSTS</topic><topic>SOUND WAVES</topic><topic>STATISTICS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Li, B</creatorcontrib><creatorcontrib>Robinson, P A</creatorcontrib><creatorcontrib>Cairns, I H</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Li, B</au><au>Robinson, P A</au><au>Cairns, I H</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Numerical simulations of type-III solar radio bursts</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2006-04-14</date><risdate>2006</risdate><volume>96</volume><issue>14</issue><spage>145005</spage><epage>145005</epage><pages>145005-145005</pages><artnum>145005</artnum><issn>0031-9007</issn><eissn>1079-7114</eissn><abstract>The first numerical simulations are presented for type-III solar radio bursts in the inhomogeneous solar corona and interplanetary space, that include microscale quasilinear and nonlinear processes, intermediate-scale driven ambient density fluctuations, and large scale evolution of electron beams, Langmuir and ion sound waves, and fundamental and harmonic electromagnetic emission. Bidirectional coronal emission is asymmetric between the upward and downward directions, and harmonic emission dominates fundamental emission. In interplanetary space, fundamental and/or harmonic emission can be important. Langmuir and ion sound waves are bursty and the statistics of Langmuir wave energy agree well with the predictions of stochastic growth theory.</abstract><cop>United States</cop><pmid>16712087</pmid><doi>10.1103/PhysRevLett.96.145005</doi><tpages>1</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2006-04, Vol.96 (14), p.145005-145005, Article 145005 |
| issn | 0031-9007 1079-7114 |
| language | eng |
| recordid | cdi_osti_scitechconnect_20775167 |
| source | American Physical Society Journals |
| subjects | ASYMMETRY CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ELECTRON BEAMS EMISSION EVOLUTION FLUCTUATIONS INTERPLANETARY SPACE ION WAVES LANGMUIR FREQUENCY NONLINEAR PROBLEMS NUMERICAL ANALYSIS PLASMA SIMULATION SOLAR CORONA SOLAR RADIO BURSTS SOUND WAVES STATISTICS |
| title | Numerical simulations of type-III solar radio bursts |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-05T23%3A04%3A43IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Numerical%20simulations%20of%20type-III%20solar%20radio%20bursts&rft.jtitle=Physical%20review%20letters&rft.au=Li,%20B&rft.date=2006-04-14&rft.volume=96&rft.issue=14&rft.spage=145005&rft.epage=145005&rft.pages=145005-145005&rft.artnum=145005&rft.issn=0031-9007&rft.eissn=1079-7114&rft_id=info:doi/10.1103/PhysRevLett.96.145005&rft_dat=%3Cproquest_osti_%3E67998964%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=67998964&rft_id=info:pmid/16712087&rfr_iscdi=true |