The chaos of motion of the charged particles in the earth's magnetotail.
碩士 === 國立中央大學 === 太空科學研究所 === 84 === The nightside magnetotail is an important region of the Earth's magnetosphere, which contains a current sheet sepa- rating regions of nearly oppositely directed magnetic field. In this region the mo...
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ndltd-TW-084NCU000690092016-02-05T04:16:39Z http://ndltd.ncl.edu.tw/handle/61258830340563351618 The chaos of motion of the charged particles in the earth's magnetotail. 帶電荷粒子在地球磁尾中的混沌運動 Hsin-Lun Liu 劉興倫 碩士 國立中央大學 太空科學研究所 84 The nightside magnetotail is an important region of the Earth's magnetosphere, which contains a current sheet sepa- rating regions of nearly oppositely directed magnetic field. In this region the motion of charged particles cannot be described by the standard Guiding-Center Drift Formulation, we thus consider the nonlinear dynamics of collisionless plasma. By using numerical simulation, we study the motion of charged particles in one-dimensional and two-dimensional equilibrium magnetic field models; the results are shown in real space abd phase space. Depending on the initail condi- tion and magnetic field configuration, the orbit of charged particles may be classified as: bounded integrable, unbounded stochastic and unbounded transient orbits with different trapped time in the current sheet. We will also study the particle dynamics in the presece of an electric field due to the penetration of the solar wind into Eath's magnetotail. Lin-Ni Hau 郝玲妮 1996 學位論文 ; thesis 101 zh-TW |
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碩士 === 國立中央大學 === 太空科學研究所 === 84 === The nightside magnetotail is an important region of the Earth's
magnetosphere, which contains a current sheet sepa- rating
regions of nearly oppositely directed magnetic field. In this
region the motion of charged particles cannot be described by
the standard Guiding-Center Drift Formulation, we thus consider
the nonlinear dynamics of collisionless plasma. By using
numerical simulation, we study the motion of charged particles
in one-dimensional and two-dimensional equilibrium magnetic
field models; the results are shown in real space abd phase
space. Depending on the initail condi- tion and magnetic field
configuration, the orbit of charged particles may be classified
as: bounded integrable, unbounded stochastic and unbounded
transient orbits with different trapped time in the current
sheet. We will also study the particle dynamics in the presece
of an electric field due to the penetration of the solar wind
into Eath's magnetotail.
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author2 |
Lin-Ni Hau |
author_facet |
Lin-Ni Hau Hsin-Lun Liu 劉興倫 |
author |
Hsin-Lun Liu 劉興倫 |
spellingShingle |
Hsin-Lun Liu 劉興倫 The chaos of motion of the charged particles in the earth's magnetotail. |
author_sort |
Hsin-Lun Liu |
title |
The chaos of motion of the charged particles in the earth's magnetotail. |
title_short |
The chaos of motion of the charged particles in the earth's magnetotail. |
title_full |
The chaos of motion of the charged particles in the earth's magnetotail. |
title_fullStr |
The chaos of motion of the charged particles in the earth's magnetotail. |
title_full_unstemmed |
The chaos of motion of the charged particles in the earth's magnetotail. |
title_sort |
chaos of motion of the charged particles in the earth's magnetotail. |
publishDate |
1996 |
url |
http://ndltd.ncl.edu.tw/handle/61258830340563351618 |
work_keys_str_mv |
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