Electrostatic Streaming Instability
碩士 === 國立中央大學 === 太空科學研究所 === 93 === Streaming instability may occur in many space plasma environments. In this study, we examine the electrostatic streaming instability based on the one-dimensional electrostatic full particle numerical code. The applications include the plasma sheet boundary layer...
Main Authors: | , |
---|---|
Other Authors: | |
Format: | Others |
Language: | zh-TW |
Published: |
2005
|
Online Access: | http://ndltd.ncl.edu.tw/handle/07887390878874877032 |
id |
ndltd-TW-093NCU05069023 |
---|---|
record_format |
oai_dc |
spelling |
ndltd-TW-093NCU050690232015-10-13T16:31:54Z http://ndltd.ncl.edu.tw/handle/07887390878874877032 Electrostatic Streaming Instability 靜電場中帶電粒子束不穩定性 Chun-Shun Jao 饒駿頌 碩士 國立中央大學 太空科學研究所 93 Streaming instability may occur in many space plasma environments. In this study, we examine the electrostatic streaming instability based on the one-dimensional electrostatic full particle numerical code. The applications include the plasma sheet boundary layer of the Earth’s magnetosphere, where the electron beams may encounter the background plasma, and the Gamma-ray burst, where high speed plasma may encounter the interstellar plasma. We vary the ratio of the beam drift velocity to the speed of light, the ratio of the beam thermal velocity to the drift velocity, and the mass ratio of the ion to electron to examine the relations between these parameters and the formation as well as the characteristics of the electrostatic solitary waves. none 郝玲妮 2005 學位論文 ; thesis 78 zh-TW |
collection |
NDLTD |
language |
zh-TW |
format |
Others
|
sources |
NDLTD |
description |
碩士 === 國立中央大學 === 太空科學研究所 === 93 === Streaming instability may occur in many space plasma environments. In this study, we examine the electrostatic streaming instability based on the one-dimensional electrostatic full particle numerical code. The applications include the plasma sheet boundary layer of the Earth’s magnetosphere, where the electron beams may encounter the background plasma, and the Gamma-ray burst, where high speed plasma may encounter the interstellar plasma. We vary the ratio of the beam drift velocity to the speed of light, the ratio of the beam thermal velocity to the drift velocity, and the mass ratio of the ion to electron to examine the relations between these parameters and the formation as well as the characteristics of the electrostatic solitary waves.
|
author2 |
none |
author_facet |
none Chun-Shun Jao 饒駿頌 |
author |
Chun-Shun Jao 饒駿頌 |
spellingShingle |
Chun-Shun Jao 饒駿頌 Electrostatic Streaming Instability |
author_sort |
Chun-Shun Jao |
title |
Electrostatic Streaming Instability |
title_short |
Electrostatic Streaming Instability |
title_full |
Electrostatic Streaming Instability |
title_fullStr |
Electrostatic Streaming Instability |
title_full_unstemmed |
Electrostatic Streaming Instability |
title_sort |
electrostatic streaming instability |
publishDate |
2005 |
url |
http://ndltd.ncl.edu.tw/handle/07887390878874877032 |
work_keys_str_mv |
AT chunshunjao electrostaticstreaminginstability AT ráojùnsòng electrostaticstreaminginstability AT chunshunjao jìngdiànchǎngzhōngdàidiànlìzishùbùwěndìngxìng AT ráojùnsòng jìngdiànchǎngzhōngdàidiànlìzishùbùwěndìngxìng |
_version_ |
1717771278203486208 |