EMIC waves converted from equatorial noise due to M/Q = 2 ions in the plasmasphere: Observations from Van Allen Probes and Arase

dc.contributor.authorMiyoshi, Y.
dc.contributor.authorMatsuda, S.
dc.contributor.authorKurita, S.
dc.contributor.authorNomura, K.
dc.contributor.authorKeika, K.
dc.contributor.authorShoji, M.
dc.contributor.authorKitamura, N.
dc.contributor.authorKasahara, Y.
dc.contributor.authorMatsuoka, A.
dc.contributor.authorShinohara, I.
dc.contributor.authorShiokawa, K.
dc.contributor.authorMachida, S.
dc.contributor.authorSantolik, O.
dc.contributor.authorBoardsen, S. A.
dc.contributor.authorHorne, R. B.
dc.contributor.authorWygant, J. F.
dc.date.accessioned2019-10-31T17:44:54Z
dc.date.available2019-10-31T17:44:54Z
dc.date.issued2019-06-07
dc.description.abstractAbstract Equatorial noise (EN) emissions are observed inside and outside the plasmapause. EN emissions are referred to as magnetosonic mode waves. Using data from Van Allen Probes and Arase, we found conversion from EN emissions to electromagnetic ion cyclotron (EMIC) waves in the plasmasphere and in the topside ionosphere. A low‐frequency part of EN emissions becomes EMIC waves through branch splitting of EN emissions, and the mode conversion from EN to EMIC waves occurs around the frequency of M/Q = 2 (deuteron and/or alpha particles) cyclotron frequency. These processes result in plasmaspheric EMIC waves. We investigated the ion composition ratio by characteristic frequencies of EN emissions and EMIC waves and obtained ion composition ratios. We found that the maximum composition ratio of M/Q = 2 ions is ~10% below 3,000 km. The quantitative estimation of the ion composition will contribute to improving the plasma model of the deep plasmasphere and the topside ionosphere. Plain Language Summary Equatorial noise (EN) emissions are whistler mode waves. Using Van Allen Probe and Arase (ERG) plasma wave data, we found that EN emissions propagate toward the Earth and are converted to electromagnetic ion cyclotron (EMIC) waves in the deep plasmasphere and the topside ionosphere. We suggest that minor ions with a mass per charge (M/Q) = 2, that is, deuteron or alpha particles, play an important role in this process. The processes reported here are a new generation process of plasmaspheric EMIC waves. Moreover, we determined the ion composition ratio using characteristics of wave dispersion. We derived the altitude profile of the ion composition ratio and identified the maximum ratio of M/Q = 2 ions of about 10% in the deep plasmasphere.en_US
dc.description.sponsorshipThe Van Allen Probes data used in thisstudy have been opened to the publicfrom the University of Minnesota(http://www.space.umn.edu/missions/rbspefw‐home‐university‐of‐minnesota/). We acknowledge usefuldiscussions with C. Klezing, Y. Kato,and D.‐H. Lee. Science data of the ERG(Arase) satellite were obtained from theERG Science Center operated byISAS/JAXA and ISEE/NagoyaUniversity (https://ergsc.isee.nagoya‐u.ac.jp/index.shtml.en). In the presentdata, we use level 1‐prime WFC version7 data and level‐2 MGF 64 Hz v01.01.The Arase satellite data will be publiclyavailable via ERG Science Center on aproject‐agreed schedule. This study issupported by Grants‐in‐Aid forScientific Research (14J02108,15H05815, 16H06286, 16J02163,17K05668, 17K14400, 17K14402 and26800257) of Japan Society for thePromotion of Science (JSPS). Thisresearch was supported by the NaturalEnvironment Research Council(NERC) Highlight Topic grantsNE/P01738X/1 (Rad‐Sat) andNE/R016038/1. This study was sup-ported by JSPS Bilateral OpenPartnership Joint Research Projects. Wealso acknowledge support from theMEYS LTAUSA17070 project and fromthe Czech Academy of Sciences throughthe JSPS‐17‐14 project and through thePraemium Academiae award.en_US
dc.description.urihttps://agupubs.onlinelibrary.wiley.com/doi/epdf/10.1029/2019GL083024en_US
dc.format.extent8 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m202qd-dwd9
dc.identifier.citationMiyoshi, Y.; Matsuda, S.; Kurita, S.; Nomura, K.; Keika, K.; Shoji, M.; Kitamura, N.; Kasahara, Y.; Matsuoka, A.; Shinohara, I.; Shiokawa, K.; Machida, S.; Santolik, O.; Boardsen, S. A.; Horne, R. B.; Wygant, J. F.; EMIC waves converted from equatorial noise due to M/Q = 2 ions in the plasmasphere: Observations from Van Allen Probes and Arase; Geophysical Research Letters, 46, 5662–5669; https://doi.org/10.1029/ 2019GL083024en_US
dc.identifier.urihttps://doi.org/10.1029/2019GL083024
dc.identifier.urihttp://hdl.handle.net/11603/16017
dc.language.isoen_USen_US
dc.publisherAmerican Geophysical Unionen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectEMICen_US
dc.subjectmagnetsonic wavesen_US
dc.subjectAraseen_US
dc.subjectVan Allen Probesen_US
dc.subjectplasmasphereen_US
dc.subjectM/Q = 2 ionsen_US
dc.titleEMIC waves converted from equatorial noise due to M/Q = 2 ions in the plasmasphere: Observations from Van Allen Probes and Araseen_US
dc.typeTexten_US

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