博碩士論文 966203006 完整後設資料紀錄

DC 欄位 語言
DC.contributor太空科學研究所zh_TW
DC.creator陳怡璇zh_TW
DC.creatorYi-shyuan Chenen_US
dc.date.accessioned2009-7-17T07:39:07Z
dc.date.available2009-7-17T07:39:07Z
dc.date.issued2009
dc.identifier.urihttp://ir.lib.ncu.edu.tw:88/thesis/view_etd.asp?URN=966203006
dc.contributor.department太空科學研究所zh_TW
DC.description國立中央大學zh_TW
DC.descriptionNational Central Universityen_US
dc.description.abstract磁層頂的位置和形狀主要取決於太陽風的動壓和地球磁層內的磁壓平衡。本篇文章為了討論磁層頂內側磁場與地球磁偶極場的比值,我們使用了THEMIS任務中的五顆衛星的資料。利用五顆衛星擁有相同酬載的優點當作我們觀測資料的來源。經過資料處理之後我們發現日側磁層頂內側磁場與地球磁偶極場的比值與靜止平衡距離在南向行星際磁場(Southward IMF)的時候會呈現正比的關係。此外在北向行星際磁場的時候,磁層頂內側磁場會隨著靜止平衡距離的-2.6次方而變化;在南向行星際磁場的時候,磁層頂內側磁場會隨著靜止平衡距離的-1.9次方而變化。這有別於地球磁偶極場隨著靜止平衡距離的-3.0次方而改變,藉由磁層頂內側磁場與靜止平衡距離之間的關係可以得到一個最佳的方程式。 zh_TW
dc.description.abstractThe pressure is balanced at the magnetopause where separates the shocked solar wind and the compressed geomagnetic field. In this research, we use the magnetic fields from five THEMIS probes and the theoretical dipole magnetic field model to calculate the ratio of the compressed geomagnetic field just inside the magnetopause to the dipole magnetic field. Here we find that the ratio is linearly proportional to the subsolar standoff distance. Additionally, we also research the relation between the compressed geomagnetic field and the subsolar distance. Here we also find that the compressed geomagnetic field varies with the subsolar distance in a power law of -2.6 (-1.9) on the Northward (Southward) IMF, which is different from that estimated from the dipole magnetic field (-3.0). Furthermore, this relation can be turned into a function of the compressed geomagnetic field in terms of the subsolar distance. en_US
DC.subject地球磁層頂內側磁場zh_TW
DC.subjectgeomagnetic fielden_US
DC.title太陽風對地球磁層頂內側磁場之影響zh_TW
dc.language.isozh-TWzh-TW
DC.titleSolarWind Control of the Geomagnetic Field insidethe Magnetopauseen_US
DC.type博碩士論文zh_TW
DC.typethesisen_US
DC.publisherNational Central Universityen_US

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