Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams
— This study gives a comparison of characteristics of small-scale ion flux fluctuations based on measurements of the SPEKTR-R spacecraft in slow and fast solar wind streams. Fast quasi-stationary streams and fast disturbed streams, associated with transient phenomena in the solar corona, are conside...
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| Veröffentlicht in: | Cosmic research 2019-11, Vol.57 (6), p.434-442 |
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| container_title | Cosmic research |
| container_volume | 57 |
| creator | Riazantseva, M. O. Rakhmanova, L. S. Zastenker, G. N. Yermolaev, Yu. I. Lodkina, I. G. Chesalin, L. S. |
| description | —
This study gives a comparison of characteristics of small-scale ion flux fluctuations based on measurements of the
SPEKTR-R
spacecraft in slow and fast solar wind streams. Fast quasi-stationary streams and fast disturbed streams, associated with transient phenomena in the solar corona, are considered separately. The use of high-time-resolution data from the Bright Monitor of Solar Wind (BMSW) instrument makes it possible to analyze plasma fluctuations in a wide range of scales, including small scales, where kinetic effects can make a significant contribution. It is shown in the study that the nature of small-scale fluctuations can significantly differ in fast streams with the same mean solar wind velocity but having a different nature. |
| doi_str_mv | 10.1134/S0010952519060078 |
| format | Article |
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This study gives a comparison of characteristics of small-scale ion flux fluctuations based on measurements of the
SPEKTR-R
spacecraft in slow and fast solar wind streams. Fast quasi-stationary streams and fast disturbed streams, associated with transient phenomena in the solar corona, are considered separately. The use of high-time-resolution data from the Bright Monitor of Solar Wind (BMSW) instrument makes it possible to analyze plasma fluctuations in a wide range of scales, including small scales, where kinetic effects can make a significant contribution. It is shown in the study that the nature of small-scale fluctuations can significantly differ in fast streams with the same mean solar wind velocity but having a different nature.</description><identifier>ISSN: 0010-9525</identifier><identifier>EISSN: 1608-3075</identifier><identifier>DOI: 10.1134/S0010952519060078</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Astronomy ; Astrophysics and Astroparticles ; Astrophysics and Cosmology ; Corona ; Fluctuations ; Ion flux ; Physics ; Physics and Astronomy ; Solar corona ; Solar wind ; Solar wind velocity ; Space Exploration and Astronautics ; Space Sciences (including Extraterrestrial Physics ; Spacecraft ; Streams ; Wind speed ; Wind velocities</subject><ispartof>Cosmic research, 2019-11, Vol.57 (6), p.434-442</ispartof><rights>Pleiades Publishing, Ltd. 2019</rights><rights>2019© Pleiades Publishing, Ltd. 2019</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-b248a377e367e72656b8cdda19ac727ebb914741173dc51c64affee664d4aa1a3</citedby><cites>FETCH-LOGICAL-c316t-b248a377e367e72656b8cdda19ac727ebb914741173dc51c64affee664d4aa1a3</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/S0010952519060078$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S0010952519060078$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,776,780,27901,27902,41464,42533,51294</link.rule.ids></links><search><creatorcontrib>Riazantseva, M. O.</creatorcontrib><creatorcontrib>Rakhmanova, L. S.</creatorcontrib><creatorcontrib>Zastenker, G. N.</creatorcontrib><creatorcontrib>Yermolaev, Yu. I.</creatorcontrib><creatorcontrib>Lodkina, I. G.</creatorcontrib><creatorcontrib>Chesalin, L. S.</creatorcontrib><title>Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams</title><title>Cosmic research</title><addtitle>Cosmic Res</addtitle><description>—
This study gives a comparison of characteristics of small-scale ion flux fluctuations based on measurements of the
SPEKTR-R
spacecraft in slow and fast solar wind streams. Fast quasi-stationary streams and fast disturbed streams, associated with transient phenomena in the solar corona, are considered separately. The use of high-time-resolution data from the Bright Monitor of Solar Wind (BMSW) instrument makes it possible to analyze plasma fluctuations in a wide range of scales, including small scales, where kinetic effects can make a significant contribution. It is shown in the study that the nature of small-scale fluctuations can significantly differ in fast streams with the same mean solar wind velocity but having a different nature.</description><subject>Astronomy</subject><subject>Astrophysics and Astroparticles</subject><subject>Astrophysics and Cosmology</subject><subject>Corona</subject><subject>Fluctuations</subject><subject>Ion flux</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Solar corona</subject><subject>Solar wind</subject><subject>Solar wind velocity</subject><subject>Space Exploration and Astronautics</subject><subject>Space Sciences (including Extraterrestrial Physics</subject><subject>Spacecraft</subject><subject>Streams</subject><subject>Wind speed</subject><subject>Wind velocities</subject><issn>0010-9525</issn><issn>1608-3075</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp1kEFLxDAQhYMouK7-AG8Bz9WZJk2aoyyuCgsKVTyWaZpKl2y7Ji3iv7dlBQ_iaXi8972Bx9glwjWikDcFAILJ0gwNKACdH7EFKsgTATo7ZovZTmb_lJ3FuAUAo4VasFWxI--TwpJ3_NlT3BFf-9EOIw1t30XednxNceDU1bzw_Scvek-Bv7WzHoKjXTxnJw356C5-7pK9ru9eVg_J5un-cXW7SaxANSRVKnMSWjuhtNOpylSV27omNGR1ql1VGZRaImpR2wytktQ0zikla0mEJJbs6tC7D_3H6OJQbvsxdNPLMhXSoFEGzJTCQ8qGPsbgmnIf2h2FrxKhnLcq_2w1MemBiVO2e3fht_l_6BsRQmmX</recordid><startdate>20191101</startdate><enddate>20191101</enddate><creator>Riazantseva, M. O.</creator><creator>Rakhmanova, L. S.</creator><creator>Zastenker, G. N.</creator><creator>Yermolaev, Yu. I.</creator><creator>Lodkina, I. G.</creator><creator>Chesalin, L. S.</creator><general>Pleiades Publishing</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>20191101</creationdate><title>Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams</title><author>Riazantseva, M. O. ; Rakhmanova, L. S. ; Zastenker, G. N. ; Yermolaev, Yu. I. ; Lodkina, I. G. ; Chesalin, L. S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-b248a377e367e72656b8cdda19ac727ebb914741173dc51c64affee664d4aa1a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Astronomy</topic><topic>Astrophysics and Astroparticles</topic><topic>Astrophysics and Cosmology</topic><topic>Corona</topic><topic>Fluctuations</topic><topic>Ion flux</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Solar corona</topic><topic>Solar wind</topic><topic>Solar wind velocity</topic><topic>Space Exploration and Astronautics</topic><topic>Space Sciences (including Extraterrestrial Physics</topic><topic>Spacecraft</topic><topic>Streams</topic><topic>Wind speed</topic><topic>Wind velocities</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Riazantseva, M. O.</creatorcontrib><creatorcontrib>Rakhmanova, L. S.</creatorcontrib><creatorcontrib>Zastenker, G. N.</creatorcontrib><creatorcontrib>Yermolaev, Yu. I.</creatorcontrib><creatorcontrib>Lodkina, I. G.</creatorcontrib><creatorcontrib>Chesalin, L. S.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & 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>Riazantseva, M. O.</au><au>Rakhmanova, L. S.</au><au>Zastenker, G. N.</au><au>Yermolaev, Yu. I.</au><au>Lodkina, I. G.</au><au>Chesalin, L. S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams</atitle><jtitle>Cosmic research</jtitle><stitle>Cosmic Res</stitle><date>2019-11-01</date><risdate>2019</risdate><volume>57</volume><issue>6</issue><spage>434</spage><epage>442</epage><pages>434-442</pages><issn>0010-9525</issn><eissn>1608-3075</eissn><abstract>—
This study gives a comparison of characteristics of small-scale ion flux fluctuations based on measurements of the
SPEKTR-R
spacecraft in slow and fast solar wind streams. Fast quasi-stationary streams and fast disturbed streams, associated with transient phenomena in the solar corona, are considered separately. The use of high-time-resolution data from the Bright Monitor of Solar Wind (BMSW) instrument makes it possible to analyze plasma fluctuations in a wide range of scales, including small scales, where kinetic effects can make a significant contribution. It is shown in the study that the nature of small-scale fluctuations can significantly differ in fast streams with the same mean solar wind velocity but having a different nature.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S0010952519060078</doi><tpages>9</tpages></addata></record> |
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| ispartof | Cosmic research, 2019-11, Vol.57 (6), p.434-442 |
| issn | 0010-9525 1608-3075 |
| language | eng |
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| source | Springer Online Journals |
| subjects | Astronomy Astrophysics and Astroparticles Astrophysics and Cosmology Corona Fluctuations Ion flux Physics Physics and Astronomy Solar corona Solar wind Solar wind velocity Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacecraft Streams Wind speed Wind velocities |
| title | Small-Scale Plasma Fluctuations in Fast and Slow Solar Wind Streams |
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