Growth and nonlinear saturation of electromagnetic ion cyclotron waves in multi-ion species magnetospheric plasma

Journal Article · Tue May 30 00:00:00 EDT 2017 · Journal of Geophysical Research. Space Physics

DOI:https://doi.org/10.1002/2017JA024172· OSTI ID:1474282

Ofman, L.  ^[1]; Denton, R. E.  ^[2]; Bortnik, J.  ^[3]; An, X.  ^[3]; Glocer, A.  ^[4]; Komar, C.  ^[1]

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1. Catholic Univ. of America, Washington, D.C. (United States); NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
2. Dartmouth College, Hanover, NH (United States)
3. Univ. of California, Los Angeles, CA (United States)
4. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)

Here, the growth and saturation of electromagnetic ion cyclotron (EMIC) waves is essential to the magnetospheric dynamics. Determining and isolating the effects of multiple ion parameters such as temperatures, anisotropies, and relative abundances is important for quantifying these processes in the magnetospheric plasma. In order to study these process, we utilize a 2.5–D hybrid model (where ions are modeled with the particle–in–cell (PIC) method, and electrons are modeled as background neutralizing fluid) to study the nonlinear electromagnetic wave–particle interactions of hot H⁺, cold H⁺, cold He⁺, and cold or hot O⁺ ions for a broad range of typical magnetospheric parameters. The excitation of EMIC waves is driven by the temperature anisotropy of hot H⁺ in our model. As a result, we quantify the parametric dependence of the linear growth, the nonlinear saturation level of perpendicular magnetic fluctuations, and the temporal evolution of the ion temperature anisotropies. We establish the relation between key plasma parameters and the saturated EMIC wave power, using either power law fits or a nonlinear regression method. We construct the dispersion relation of the waves using the results of the model and investigate the energy content in the various branches of the dispersion (k_∥–ω space), showing that the different modes can generate wave power in different regions of k space. We find that large O⁺ concentration reduces the growth and saturated amplitude of the waves; but the waves are less sensitive to the temperature of the O⁺ in the temperature range relevant to the magnetosphere.

• Research Organization: Univ. of California, Los Angeles, CA (United States)
• Sponsoring Organization: USDOE Office of Science (SC)
• Grant/Contract Number: SC0010578
• OSTI ID: 1474282
• Journal Information: Journal of Geophysical Research. Space Physics, Vol. 122, Issue 6; ISSN 2169-9380
• Publisher: American Geophysical Union
• Country of Publication: United States
• Language: English

Related Subjects

79 ASTRONOMY AND ASTROPHYSICS
EMIC waves
magnetospheric plasma
hybrid modeling
parametric study