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Dust acoustic dromions in a magnetized dusty plasma with superthermal electrons and ions
An investigation of dust acoustic (DA) dromions in a magnetized dusty plasma consisting of inertial dust fluid, kappa‐type distributed electrons, and ions is presented. Using reductive perturbation technique, we have derived coupled nonlinear evolution equations of (2 + 1) dimensions (called Davey‐S...
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Published in: | Journal of geophysical research. Space physics 2016-06, Vol.121 (6), p.5944-5958 |
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container_issue | 6 |
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container_title | Journal of geophysical research. Space physics |
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creator | Saini, N. S. Ghai, Yashika Kohli, Ripin |
description | An investigation of dust acoustic (DA) dromions in a magnetized dusty plasma consisting of inertial dust fluid, kappa‐type distributed electrons, and ions is presented. Using reductive perturbation technique, we have derived coupled nonlinear evolution equations of (2 + 1) dimensions (called Davey‐Stewartson (DS‐I) equations). Hirota bilinear method has been employed to derive the analytical solution of DS‐I equations. The solutions of such equations are exponentially localized and are called dromions. The combined effects of various physical parameters such as superthermality of charged particles, strength of magnetic field, and dust concentration have been studied on the existence regions and propagation properties of DA dromions in context with observations of POLAR satellite in the presence of superthermal particles in polar cap boundary layer region of Earth's atmosphere.
Key Points
The strength of magnetic field and superthermality of charged particles significantly influence the characteristics of DA dromions
The parametric domain for existence of dromions is significantly modified by the variation in superthermality of charged particles
Three‐dimensional dromions having very high amplitude are observed |
doi_str_mv | 10.1002/2015JA022138 |
format | article |
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Key Points
The strength of magnetic field and superthermality of charged particles significantly influence the characteristics of DA dromions
The parametric domain for existence of dromions is significantly modified by the variation in superthermality of charged particles
Three‐dimensional dromions having very high amplitude are observed</description><identifier>ISSN: 2169-9380</identifier><identifier>EISSN: 2169-9402</identifier><identifier>DOI: 10.1002/2015JA022138</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Boundary layers ; Charged particles ; Davey‐Stewartson equation ; dromions ; Dust ; dust acoustic ; Dusty plasmas ; Earth atmosphere ; Electrons ; Evolution ; Inertial ; Ions ; kappa distribution ; Magnetic fields ; Mathematical analysis ; Nonlinear equations ; Nonlinear evolution equations ; Perturbation methods ; Physical properties ; Plasma ; Polar caps ; Satellite observation ; Strength</subject><ispartof>Journal of geophysical research. Space physics, 2016-06, Vol.121 (6), p.5944-5958</ispartof><rights>2016. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4012-898fe3722929f195fa57ef4801cff30e4cc0be675a397d0b27c9029bba3cfc483</citedby><cites>FETCH-LOGICAL-c4012-898fe3722929f195fa57ef4801cff30e4cc0be675a397d0b27c9029bba3cfc483</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Saini, N. S.</creatorcontrib><creatorcontrib>Ghai, Yashika</creatorcontrib><creatorcontrib>Kohli, Ripin</creatorcontrib><title>Dust acoustic dromions in a magnetized dusty plasma with superthermal electrons and ions</title><title>Journal of geophysical research. Space physics</title><description>An investigation of dust acoustic (DA) dromions in a magnetized dusty plasma consisting of inertial dust fluid, kappa‐type distributed electrons, and ions is presented. Using reductive perturbation technique, we have derived coupled nonlinear evolution equations of (2 + 1) dimensions (called Davey‐Stewartson (DS‐I) equations). Hirota bilinear method has been employed to derive the analytical solution of DS‐I equations. The solutions of such equations are exponentially localized and are called dromions. The combined effects of various physical parameters such as superthermality of charged particles, strength of magnetic field, and dust concentration have been studied on the existence regions and propagation properties of DA dromions in context with observations of POLAR satellite in the presence of superthermal particles in polar cap boundary layer region of Earth's atmosphere.
Key Points
The strength of magnetic field and superthermality of charged particles significantly influence the characteristics of DA dromions
The parametric domain for existence of dromions is significantly modified by the variation in superthermality of charged particles
Three‐dimensional dromions having very high amplitude are observed</description><subject>Boundary layers</subject><subject>Charged particles</subject><subject>Davey‐Stewartson equation</subject><subject>dromions</subject><subject>Dust</subject><subject>dust acoustic</subject><subject>Dusty plasmas</subject><subject>Earth atmosphere</subject><subject>Electrons</subject><subject>Evolution</subject><subject>Inertial</subject><subject>Ions</subject><subject>kappa distribution</subject><subject>Magnetic fields</subject><subject>Mathematical analysis</subject><subject>Nonlinear equations</subject><subject>Nonlinear evolution equations</subject><subject>Perturbation methods</subject><subject>Physical properties</subject><subject>Plasma</subject><subject>Polar caps</subject><subject>Satellite observation</subject><subject>Strength</subject><issn>2169-9380</issn><issn>2169-9402</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><recordid>eNqNkU1LAzEQhhdRsNTe_AEBLx5cnSSbTXIsVaulIIiCtyWbTeyW_TLZpdRfb0oVxENxLjPMPPMyH1F0juEaA5AbApgtpkAIpuIoGhGcylgmQI5_YirgNJp4v4ZgIqQwG0Vvt4PvkdJtcKVGhWvrsm08KhukUK3eG9OXn6ZARahvUVcpXyu0KfsV8kNnXL8yrlYVMpXRvds1qqZAO4Wz6MSqypvJtx9Hr_d3L7OHePk0f5xNl7FOAJNYSGEN5YRIIi2WzCrGjU0EYG0tBZNoDblJOVNU8gJywrUEIvNcUW11Iug4utzrdq79GIzvs7r02lSVakxYKsOCshSYJOwfKAgOKUmSgF78Qdft4JqwSBbuzMPkHKeHqKCVMC4oxYG62lPatd47Y7POlbVy2wxDtntd9vt1Aad7fFNWZnuQzRbz5ykLoxD6BTL8mAc</recordid><startdate>201606</startdate><enddate>201606</enddate><creator>Saini, N. S.</creator><creator>Ghai, Yashika</creator><creator>Kohli, Ripin</creator><general>Blackwell Publishing Ltd</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>201606</creationdate><title>Dust acoustic dromions in a magnetized dusty plasma with superthermal electrons and ions</title><author>Saini, N. S. ; Ghai, Yashika ; Kohli, Ripin</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4012-898fe3722929f195fa57ef4801cff30e4cc0be675a397d0b27c9029bba3cfc483</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Boundary layers</topic><topic>Charged particles</topic><topic>Davey‐Stewartson equation</topic><topic>dromions</topic><topic>Dust</topic><topic>dust acoustic</topic><topic>Dusty plasmas</topic><topic>Earth atmosphere</topic><topic>Electrons</topic><topic>Evolution</topic><topic>Inertial</topic><topic>Ions</topic><topic>kappa distribution</topic><topic>Magnetic fields</topic><topic>Mathematical analysis</topic><topic>Nonlinear equations</topic><topic>Nonlinear evolution equations</topic><topic>Perturbation methods</topic><topic>Physical properties</topic><topic>Plasma</topic><topic>Polar caps</topic><topic>Satellite observation</topic><topic>Strength</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Saini, N. S.</creatorcontrib><creatorcontrib>Ghai, Yashika</creatorcontrib><creatorcontrib>Kohli, Ripin</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>Journal of geophysical research. Space physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Saini, N. S.</au><au>Ghai, Yashika</au><au>Kohli, Ripin</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Dust acoustic dromions in a magnetized dusty plasma with superthermal electrons and ions</atitle><jtitle>Journal of geophysical research. Space physics</jtitle><date>2016-06</date><risdate>2016</risdate><volume>121</volume><issue>6</issue><spage>5944</spage><epage>5958</epage><pages>5944-5958</pages><issn>2169-9380</issn><eissn>2169-9402</eissn><abstract>An investigation of dust acoustic (DA) dromions in a magnetized dusty plasma consisting of inertial dust fluid, kappa‐type distributed electrons, and ions is presented. Using reductive perturbation technique, we have derived coupled nonlinear evolution equations of (2 + 1) dimensions (called Davey‐Stewartson (DS‐I) equations). Hirota bilinear method has been employed to derive the analytical solution of DS‐I equations. The solutions of such equations are exponentially localized and are called dromions. The combined effects of various physical parameters such as superthermality of charged particles, strength of magnetic field, and dust concentration have been studied on the existence regions and propagation properties of DA dromions in context with observations of POLAR satellite in the presence of superthermal particles in polar cap boundary layer region of Earth's atmosphere.
Key Points
The strength of magnetic field and superthermality of charged particles significantly influence the characteristics of DA dromions
The parametric domain for existence of dromions is significantly modified by the variation in superthermality of charged particles
Three‐dimensional dromions having very high amplitude are observed</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1002/2015JA022138</doi><tpages>15</tpages></addata></record> |
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language | eng |
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source | Wiley |
subjects | Boundary layers Charged particles Davey‐Stewartson equation dromions Dust dust acoustic Dusty plasmas Earth atmosphere Electrons Evolution Inertial Ions kappa distribution Magnetic fields Mathematical analysis Nonlinear equations Nonlinear evolution equations Perturbation methods Physical properties Plasma Polar caps Satellite observation Strength |
title | Dust acoustic dromions in a magnetized dusty plasma with superthermal electrons and ions |
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