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Analytical study of electromagnetic ion cyclotron wave for ring distribution with AC electric field in Saturn magnetosphere
Characteristics of electromagnetic ion cyclotron waves in Saturn inner magnetosphere has been investigated here in close proximity of equatorial plane at approximately mid of the E ring near 5Rs by using data sets released by Voyager and Cassini spacecraft. Previous encounter of these spacecraft wit...
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Published in: | Journal of physics. Conference series 2021-03, Vol.1817 (1), p.12020 |
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description | Characteristics of electromagnetic ion cyclotron waves in Saturn inner magnetosphere has been investigated here in close proximity of equatorial plane at approximately mid of the E ring near 5Rs by using data sets released by Voyager and Cassini spacecraft. Previous encounter of these spacecraft with Saturn exposed the strong signature of EMIC wave and harmonics believed to be originated within 7.5 Rs due to dominant O
+
ions and water group ions. Maxwellian ring distribution for pickup ions contributing ring around planet is opted to find unperturbed particle density. Therefore, investigating here growth of obliquely propagating EMIC wave undergoing wave particle mechanism by opting kinetic approach to establish mathematical dispersion model in view of different parameters and extended to comparative study for parallel propagation. Parametric analysis inferred that waves propagating in the oblique direction grows more as compare to parallel propagating waves for the extended value of temperature anisotropy and the angle of propagation with respect to the ambient magnetic field B (at equator) and second harmonic of ion cyclotron waves indicating that the modified ion cyclotron wave shifts the wave spectra to higher side with increase in bandwidth. Study can be carried out to analyze other instabilities to explore magnetospheric dynamics at different radial distances. |
doi_str_mv | 10.1088/1742-6596/1817/1/012020 |
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+
ions and water group ions. Maxwellian ring distribution for pickup ions contributing ring around planet is opted to find unperturbed particle density. Therefore, investigating here growth of obliquely propagating EMIC wave undergoing wave particle mechanism by opting kinetic approach to establish mathematical dispersion model in view of different parameters and extended to comparative study for parallel propagation. Parametric analysis inferred that waves propagating in the oblique direction grows more as compare to parallel propagating waves for the extended value of temperature anisotropy and the angle of propagation with respect to the ambient magnetic field B (at equator) and second harmonic of ion cyclotron waves indicating that the modified ion cyclotron wave shifts the wave spectra to higher side with increase in bandwidth. Study can be carried out to analyze other instabilities to explore magnetospheric dynamics at different radial distances.</description><identifier>ISSN: 1742-6588</identifier><identifier>EISSN: 1742-6596</identifier><identifier>DOI: 10.1088/1742-6596/1817/1/012020</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Anisotropy ; Bandwidths ; Cassini mission ; Comparative studies ; Cyclotrons ; Electric fields ; Harmonics ; Ions ; Parametric analysis ; Particle density (concentration) ; Physics ; Planetary magnetospheres ; Rings (mathematics) ; Saturn ; Spacecraft ; Wave propagation ; Wave spectra</subject><ispartof>Journal of physics. Conference series, 2021-03, Vol.1817 (1), p.12020</ispartof><rights>2021. This work is published under http://creativecommons.org/licenses/by/3.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c2490-f88cc3c14c3d453ce517e50d5b89defa52e6f8f2c3b59661af429f044fe6d9153</citedby><cites>FETCH-LOGICAL-c2490-f88cc3c14c3d453ce517e50d5b89defa52e6f8f2c3b59661af429f044fe6d9153</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.proquest.com/docview/2512938197?pq-origsite=primo$$EHTML$$P50$$Gproquest$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,25751,27922,27923,37010,44588</link.rule.ids></links><search><creatorcontrib>Shukla, Neeta Kumari</creatorcontrib><creatorcontrib>Singh, Devi</creatorcontrib><creatorcontrib>Pandey, R.S.</creatorcontrib><title>Analytical study of electromagnetic ion cyclotron wave for ring distribution with AC electric field in Saturn magnetosphere</title><title>Journal of physics. Conference series</title><description>Characteristics of electromagnetic ion cyclotron waves in Saturn inner magnetosphere has been investigated here in close proximity of equatorial plane at approximately mid of the E ring near 5Rs by using data sets released by Voyager and Cassini spacecraft. Previous encounter of these spacecraft with Saturn exposed the strong signature of EMIC wave and harmonics believed to be originated within 7.5 Rs due to dominant O
+
ions and water group ions. Maxwellian ring distribution for pickup ions contributing ring around planet is opted to find unperturbed particle density. Therefore, investigating here growth of obliquely propagating EMIC wave undergoing wave particle mechanism by opting kinetic approach to establish mathematical dispersion model in view of different parameters and extended to comparative study for parallel propagation. Parametric analysis inferred that waves propagating in the oblique direction grows more as compare to parallel propagating waves for the extended value of temperature anisotropy and the angle of propagation with respect to the ambient magnetic field B (at equator) and second harmonic of ion cyclotron waves indicating that the modified ion cyclotron wave shifts the wave spectra to higher side with increase in bandwidth. Study can be carried out to analyze other instabilities to explore magnetospheric dynamics at different radial distances.</description><subject>Anisotropy</subject><subject>Bandwidths</subject><subject>Cassini mission</subject><subject>Comparative studies</subject><subject>Cyclotrons</subject><subject>Electric fields</subject><subject>Harmonics</subject><subject>Ions</subject><subject>Parametric analysis</subject><subject>Particle density (concentration)</subject><subject>Physics</subject><subject>Planetary magnetospheres</subject><subject>Rings (mathematics)</subject><subject>Saturn</subject><subject>Spacecraft</subject><subject>Wave propagation</subject><subject>Wave spectra</subject><issn>1742-6588</issn><issn>1742-6596</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><recordid>eNo9kN9LwzAQx4MoOKd_gwGfa_OjadPHMdQJAx_U55ClyZbRNTNJHcV_3pSO5eXC3fe-d_cB4BGjZ4w4z3FVkKxkdZljjqsc5wgTRNAVmF0q15c_57fgLoQ9QjS9agb-Fp1sh2iVbGGIfTNAZ6ButYreHeS206kEreugGlTrUrKDJ_mroXEeetttYWND9HbTx1F0snEHF8uzQeo0VrcNtB38lLH3HZwsXTjutNf34MbINuiHc5yD79eXr-UqW3-8vS8X60yRokaZ4VwpqnChaFMwqjTDlWaoYRteN9pIRnRpuCGKbtKtJZamILVBRWF02dSY0Tl4mnyP3v30OkSxd2mZNFIQhklNOa6rpKomlfIuBK-NOHp7kH4QGImRtBgZipGnGEkLLCbS9B_rj3PX</recordid><startdate>20210301</startdate><enddate>20210301</enddate><creator>Shukla, Neeta Kumari</creator><creator>Singh, Devi</creator><creator>Pandey, R.S.</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope></search><sort><creationdate>20210301</creationdate><title>Analytical study of electromagnetic ion cyclotron wave for ring distribution with AC electric field in Saturn magnetosphere</title><author>Shukla, Neeta Kumari ; Singh, Devi ; Pandey, R.S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c2490-f88cc3c14c3d453ce517e50d5b89defa52e6f8f2c3b59661af429f044fe6d9153</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Anisotropy</topic><topic>Bandwidths</topic><topic>Cassini mission</topic><topic>Comparative studies</topic><topic>Cyclotrons</topic><topic>Electric fields</topic><topic>Harmonics</topic><topic>Ions</topic><topic>Parametric analysis</topic><topic>Particle density (concentration)</topic><topic>Physics</topic><topic>Planetary magnetospheres</topic><topic>Rings (mathematics)</topic><topic>Saturn</topic><topic>Spacecraft</topic><topic>Wave propagation</topic><topic>Wave spectra</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Shukla, Neeta Kumari</creatorcontrib><creatorcontrib>Singh, Devi</creatorcontrib><creatorcontrib>Pandey, R.S.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><jtitle>Journal of physics. Conference series</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Shukla, Neeta Kumari</au><au>Singh, Devi</au><au>Pandey, R.S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Analytical study of electromagnetic ion cyclotron wave for ring distribution with AC electric field in Saturn magnetosphere</atitle><jtitle>Journal of physics. Conference series</jtitle><date>2021-03-01</date><risdate>2021</risdate><volume>1817</volume><issue>1</issue><spage>12020</spage><pages>12020-</pages><issn>1742-6588</issn><eissn>1742-6596</eissn><abstract>Characteristics of electromagnetic ion cyclotron waves in Saturn inner magnetosphere has been investigated here in close proximity of equatorial plane at approximately mid of the E ring near 5Rs by using data sets released by Voyager and Cassini spacecraft. Previous encounter of these spacecraft with Saturn exposed the strong signature of EMIC wave and harmonics believed to be originated within 7.5 Rs due to dominant O
+
ions and water group ions. Maxwellian ring distribution for pickup ions contributing ring around planet is opted to find unperturbed particle density. Therefore, investigating here growth of obliquely propagating EMIC wave undergoing wave particle mechanism by opting kinetic approach to establish mathematical dispersion model in view of different parameters and extended to comparative study for parallel propagation. Parametric analysis inferred that waves propagating in the oblique direction grows more as compare to parallel propagating waves for the extended value of temperature anisotropy and the angle of propagation with respect to the ambient magnetic field B (at equator) and second harmonic of ion cyclotron waves indicating that the modified ion cyclotron wave shifts the wave spectra to higher side with increase in bandwidth. Study can be carried out to analyze other instabilities to explore magnetospheric dynamics at different radial distances.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1742-6596/1817/1/012020</doi><oa>free_for_read</oa></addata></record> |
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subjects | Anisotropy Bandwidths Cassini mission Comparative studies Cyclotrons Electric fields Harmonics Ions Parametric analysis Particle density (concentration) Physics Planetary magnetospheres Rings (mathematics) Saturn Spacecraft Wave propagation Wave spectra |
title | Analytical study of electromagnetic ion cyclotron wave for ring distribution with AC electric field in Saturn magnetosphere |
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