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  • Presentation | SM11D: Heavy Ions as Tracers and Regulators of Plasma Processes in the Solar System Poster
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  • SM11D-1974: Bi-ion Hybrid Resonant Frequency Observation and Ion Concentration Evaluation
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  • Board 1974‚ Hall EFG (Poster Hall)
    NOLA CC
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Author(s):
Xu Liu, University of Texas at Dallas (First Author, Presenting Author)
Shujie Gu, University of Texas at Dallas
Lunjin Chen, University of Texas at Dallas
Maria Usanova, Laboratory for Atmospheric and Space Physics


Bi-ion hybrid resonant frequency fbi-ion is a characteristic frequency between two ion species. For the quasi-perpendicular wave propagation, the polarization change occurs near fbi-ion, but the wave frequency is almost unchanged. fbi-ion is not commonly observed in the spectrum since such polarization change occurs in a narrow frequency range. This study reports a bi-ion hybrid resonant frequency observation with a clear magnetic field polarization change from the compressional component dominance to the transverse component dominance. The determination of such a frequency is valuable for estimating ion concentrations, which is a critical parameter in space plasma. The ion concentration usually cannot be measured directly due to spacecraft charging, which often prevents cold ions from reaching detectors. The bi-ion hybrid resonant frequency is directly related to the ion concentration and, thus, can be used to infer the ion concentration. Using the bi-ion hybrid resonant frequency, we can determine the ranges of ion concentrations for each species in proton-helium-oxygen plasma and their one-to-one relation. Combining the observed proton, helium ion, and oxygen ion distributions, we further narrow down the range of ion concentrations.



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