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dc.contributor.author정영대-
dc.date.accessioned2018-02-05T01:18:13Z-
dc.date.available2018-02-05T01:18:13Z-
dc.date.issued2016-03-
dc.identifier.citationPHYSICS LETTERS A, v. 380, NO 11-12, Page. 1193-1196en_US
dc.identifier.issn0375-9601-
dc.identifier.issn1873-2429-
dc.identifier.urihttp://www.sciencedirect.com/science/article/pii/S0375960116000815?via%3Dihub-
dc.identifier.urihttp://hdl.handle.net/20.500.11754/35369-
dc.description.abstractThe influence of magnetic field and dust rotation on the resonant instability of surface electrostatic ion-cyclotron wave is kinetically investigated in a semi-bounded warm magnetized dusty plasma. The dispersion relation and the temporal growth rate of the surface electrostatic-ion-cyclotron wave are derived by the specular-reflection boundary condition including the magnetic field and dust rotation effects. It is found that the instability domain decreases with an increase of the rotation frequency of elongated dust grain. It is also found that the dependence of the propagation wave number on the temporal growth rate is more significant for small ion cyclotron frequencies. In addition, it is shown that the scaled growth rate increases with an increase of the strength of magnetic field. The variation of the domain and magnitude of temporal growth rate due to the change of plasma parameters is also discussed. (C) 2016 Elsevier B.V. All rights reserved.en_US
dc.description.sponsorshipThis paper is dedicated to the late Prof. P.K. Shukla in memory of exciting and stimulating collaboration on physical processes in dusty plasmas. The authors gratefully acknowledge Prof. H.J. Lee for providing highly useful references and valuable discussions. One of the authors (Y.-D.J.) gratefully acknowledges Prof. W. Roberge for useful discussions and warm hospitality while visiting the Department of Physics, Applied Physics, and Astronomy at Rensselaer Polytechnic Institute (RPI). This research was initiated while one of the authors (Y.-D.J.) was affiliated with Rensselaer as a visiting professor. This research was supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science and Technology (Grant No. 2012-001493).en_US
dc.language.isoenen_US
dc.publisherELSEVIER SCIENCE BVen_US
dc.subjectResonant instabilityen_US
dc.subjectSurface electrostatic-ion-cyclotron waveen_US
dc.subjectSemi-bounded magnetized dusty plasmasen_US
dc.titleCharacteristics of the resonant instability of surface electrostatic-ion-cyclotron waves in a semi-bounded warm magnetized dusty plasmaen_US
dc.typeArticleen_US
dc.relation.no11-12-
dc.relation.volume380-
dc.identifier.doi10.1016/j.physleta.2016.01.038-
dc.relation.page1193-1196-
dc.relation.journalPHYSICS LETTERS A-
dc.contributor.googleauthorHong, Woo-Pyo-
dc.contributor.googleauthorJung, Young-Dae-
dc.relation.code2016003673-
dc.sector.campusS-
dc.sector.daehakGRADUATE SCHOOL[S]-
dc.sector.departmentDEPARTMENT OF BIONANOTECHNOLOGY-
dc.identifier.pidydjung-
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GRADUATE SCHOOL[S](대학원) > BIONANOTECHNOLOGY(바이오나노학과) > Articles
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