Articles | Volume 39, issue 1
https://doi.org/10.5194/angeo-39-165-2021
https://doi.org/10.5194/angeo-39-165-2021
ANGEO Communicates
 | 
22 Feb 2021
ANGEO Communicates |  | 22 Feb 2021

Wavevector spectral signature of decay instability in space plasmas

Horia Comişel, Yasuhito Narita, and Uwe Motschmann

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Cited articles

Comişel, H., Narita, Y., and Motschmann, U.: Wavevector anisotropy of plasma turbulence at ion kinetic scales: solar wind observations and hybrid simulations, Nonlin. Processes Geophys., 21, 1075–1083, https://doi.org/10.5194/npg-21-1075-2014, 2014. a
Comişel, H., Narita, Y., and Motschmann, U.: Multi-channel coupling of decay instability in three-dimensional low-beta plasma, Ann. Geophys., 37, 835–842, https://doi.org/10.5194/angeo-37-835-2019, 2019. a, b, c, d
Comişel, H., Narita, Y., and Motschmann, U.: Alfvén wave evolution into magnetic filaments in 3-D space plasma, Earth Planet. Space, 72, 32, https://doi.org/10.1186/s40623-020-01156-8, 2020. a
Gao, X., Lu, Q., Li, X., Shan, L., and Wang., S.: Parametric instability of a monochromatic Alfven wave: Perpendicular decay in low beta plasma, Phys. Plasmas, 20, 072902, https://doi.org/10.1063/1.4816703, 2013. a, b
Ghosh, S. and Goldstein, M. L.: Nonlinear evolution of a large-amplitude circularly polarized Alfvén wave: Low beta, J. Geophys. Res., 99, 13352–13362, 1994. a
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Short summary
Identification of a large-amplitude Alfvén wave decaying into a pair of ion-acoustic and daughter Alfvén waves is one of the major goals in the observational studies of space plasma nonlinearity. Growth-rate maps may serve as a useful tool for predictions of the wavevector spectrum of density or magnetic field fluctuations in various scenarios for the wave–wave coupling processes developing at different stages in space plasma turbulence.
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