PIC simulation study of electron kinetic effects on nonlinear plasma waves비선형 플라즈마 파동 현상에서 전자운동 효과에 대한 PIC 전산모사 연구

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We have studied electron kinetic effects on nonlinear plasma waves using 1D PIC simulation. First, electron kinetic effects on electron holes propagating in density homogeneous region is studied. Electron holes (EHs) are known to be generated by streaming instability after magnetotail reconnection and to propagate to Earth’s polar region along the magnetic field line. While propagating, they encounter density inhomogeneity and their structures are changed due to interactions with the density gradient. Passing the density gradient region. We figured out that the oscillation is odd eigenmode trapped in the electron hole (OEM) which is closely related to the electron bouncing motion in EH potential. Potential amplitude of OEM in density inhomogeneity is asymmetric and ions are accelerated backward direction due to this potential difference. As a result, backward propagating ion acoustic waves or ion acoustic solitary waves are formed. We have derived the frequency and shape of OEM using Lewis’s formalism and they show very good agreement with the simulation results. Second, nonlinear evolution of oblique whistler waves is studied. When wave parameters correspond to non-stochastic region (or O’Neil-like damping region), vortex structures in $x-v_x$ phase space distribution, plateau distribution in parallel velocity distribution and saturation of wave energy and electron energy are commonly observed. The waves and electron energy are saturated in time scale of t∼O(100 $omega_{ce}^{-1}$). Therefore, we conclude that electron parallel energy is increased by Landau-resonance and the energy exchange is saturated after particle trapping is fully developed in those case. On the other hand, the wave parameters in stochastic region, the saturation is prevented by the stochastic change of particle motion. They lead fully thermalized phase space distribution and extreme damping of wave energy. These results imply that very large amplitude oblique whistler waves could be hardly observed in satellite data due to their very rapid damping.
Advisors
Min, Kyoung Wookresearcher민경욱researcher
Description
한국과학기술원 :물리학과,
Publisher
한국과학기술원
Issue Date
2017
Identifier
325007
Language
eng
Description

학위논문(박사) - 한국과학기술원 : 물리학과, 2017.8,[vi, 74 p. :]

Keywords

BGK mode▼aelectron hole▼aoblique whistler wave▼aelectron kinetics▼aparticle-in-cell; BGK 모드▼a전자 공동▼a사각 whistler 파동▼a전자운동▼aparticle-in-cell 전산모사

URI
http://hdl.handle.net/10203/241792
Link
http://library.kaist.ac.kr/search/detail/view.do?bibCtrlNo=718819&flag=dissertation
Appears in Collection
PH-Theses_Ph.D.(박사논문)
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