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- W2095350813 endingPage "114" @default.
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- W2095350813 abstract "Kinetic Alfvén waves (KAWs) are small-scale dispersive AWs that can play an important role in particle heating and acceleration of space and solar plasmas. An excitation mechanism for KAWs created by the coupling between large-scale oblique AWs and small-scale KAWs is presented in this paper. Taking into account both the collisional and Landau damping dissipations, the results show that the net growth rate of the excited KAWs increases with their perpendicular wavenumber k⊥ and reaches maximum at λek⊥ ∼ 0.3, where λe is the electron inertial length. However, for KAWs with shorter perpendicular wavelengths, the net growth rate decreases rapidly due to dissipative effects. The evaluation of the threshold amplitude of the AW implies that for KAWs with λek⊥ < 0.3, the relative threshold amplitude is well below 10%, which is easy to satisfy. In particular, when applying this mechanism to the case of a solar coronal hole containing a dense plume structure, our results show that KAWs with λek⊥ < 0.3 can be not only efficiently excited in the interplume region but also strongly dissipated in the dense plume due to the Landau damping." @default.
- W2095350813 created "2016-06-24" @default.
- W2095350813 creator A5022899104 @default.
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- W2095350813 date "2011-06-23" @default.
- W2095350813 modified "2023-09-24" @default.
- W2095350813 title "KINETIC ALFVÉN WAVES EXCITED BY OBLIQUE MAGNETOHYDRODYNAMIC ALFVÉN WAVES IN CORONAL HOLES" @default.
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- W2095350813 doi "https://doi.org/10.1088/0004-637x/735/2/114" @default.
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