中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究

碩士 === 國立中央大學 === 太空科學研究所 === 89 === Abstract Gathered during the year 2000 from the ion trop sensor on the ROCSAT-1, a satellite in a circular orbit at the height of 600km, the high resolution ion density data in the equatorial spread F (ESF) events are analyzed in the thesis. The occurr...

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Main Author: 何旭慧
Other Authors: 蘇信一
Format: Others
Language:zh-TW
Published: 2001
Online Access:http://ndltd.ncl.edu.tw/handle/15825545687825441319
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spelling ndltd-TW-089NCU000690082016-01-29T04:28:17Z http://ndltd.ncl.edu.tw/handle/15825545687825441319 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究 何旭慧 碩士 國立中央大學 太空科學研究所 89 Abstract Gathered during the year 2000 from the ion trop sensor on the ROCSAT-1, a satellite in a circular orbit at the height of 600km, the high resolution ion density data in the equatorial spread F (ESF) events are analyzed in the thesis. The occurrence distributions of the plasma bubbles with seasons, locations, and magnetic activities have been obtained. During quite times, the ESF events are most likely to occur around 2000 LT. With the increase in magnetic activity, the plasma bubbles appear frequently from midnight to sunrise. The probability of the plasma bubbles occurrence is always high near 0 longitude all year long. The seasonal occurrence is such that it is high in the pacific regions (between 120 and 150 longitude) during northern summer and in the south of America (between -60 - -30 longitude) during northern winter. The result of the spectra analysis for the ESF events, indicate that the spectral index in three scales ranges changes as function as local time during 1800-2000 LT under the condition Kp 3+, and during 0300-0600 LT in the strong geomagnetic activities (Kp 4-). 蘇信一 2001 學位論文 ; thesis 83 zh-TW
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description 碩士 === 國立中央大學 === 太空科學研究所 === 89 === Abstract Gathered during the year 2000 from the ion trop sensor on the ROCSAT-1, a satellite in a circular orbit at the height of 600km, the high resolution ion density data in the equatorial spread F (ESF) events are analyzed in the thesis. The occurrence distributions of the plasma bubbles with seasons, locations, and magnetic activities have been obtained. During quite times, the ESF events are most likely to occur around 2000 LT. With the increase in magnetic activity, the plasma bubbles appear frequently from midnight to sunrise. The probability of the plasma bubbles occurrence is always high near 0 longitude all year long. The seasonal occurrence is such that it is high in the pacific regions (between 120 and 150 longitude) during northern summer and in the south of America (between -60 - -30 longitude) during northern winter. The result of the spectra analysis for the ESF events, indicate that the spectral index in three scales ranges changes as function as local time during 1800-2000 LT under the condition Kp 3+, and during 0300-0600 LT in the strong geomagnetic activities (Kp 4-).
author2 蘇信一
author_facet 蘇信一
何旭慧
author 何旭慧
spellingShingle 何旭慧
中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
author_sort 何旭慧
title 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
title_short 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
title_full 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
title_fullStr 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
title_full_unstemmed 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
title_sort 中華衛星一號觀測電離層電漿氣泡密度變化之統計及研究
publishDate 2001
url http://ndltd.ncl.edu.tw/handle/15825545687825441319
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