第23太陽週期之前半期大尺度日珥暗紋之研究

以作者查詢圖書館館藏

、以作者查詢臺灣博碩士

、以作者查詢全國書目

、勘誤回報

、線上人數：21

、訪客IP：18.188.152.162

姓名

鄭麗香(Li-Hsiang Cheng) 查詢紙本館藏

畢業系所

太空科學研究所

論文名稱

第23太陽週期之前半期大尺度日珥暗紋之研究
(A study of solar prominenes/filament during the raising period of solar cycle 23)

相關論文

★ 非週期不均勻電漿系統中靜電電漿動力數值模擬碼之設計與應用	★ 利用台灣日震觀測網的太陽影像資料研究太陽差動自轉的變化情形
★ Simulation and Theoretical Study of the Kelvin-Helmholtz Instabilityin the MHD Plasmas	★ 太陽風中旋轉不連續面及非線性艾爾文波之數值模擬研究
★ 無碰撞電漿中靜電雙流不穩定之數值模擬研究	★ 靜電激震波之電漿動力數值模擬與理論研究
★ 透過高頻電磁波加速電子來間接加速質子的數值模擬研究	★ 磁流體力學中電漿團加速與磁場重聯率變化成因之數值模擬研究
★ 利用強場電磁波產生高能質子束的數值模擬研究	★ 太空電漿中跨尺度快波中速波與慢波的頻散關係之研究
★ 極端AU指數事件之研究	★ 擾動層厚度對 Kelvin-Helmholtz 不穩定之成長率隨波長分佈的影響
★ 磁層與電離層耦合模式中磁層與電離層邊界條件對磁副暴發生時夜側極光弧分布之影響	★ 太空電漿中之中低頻波的研究
★ 理論與數值模擬研究次磁音速的寬頻Kelvin-Helmholtz不穩定波動成長率與非線性發展過程

檔案

[Endnote RIS 格式]

[Bibtex 格式]

[相關文章]

[文章引用]

[完整記錄]

[館藏目錄]

[檢視]

[下載]

本電子論文使用權限為同意立即開放。
已達開放權限電子全文僅授權使用者為學術研究之目的，進行個人非營利性質之檢索、閱讀、列印。
請遵守中華民國著作權法之相關規定，切勿任意重製、散佈、改作、轉貼、播送，以免觸法。

摘要(中)

日珥在太陽表面是一個特殊的現象。直到目前為止，日珥的形成原因一直都還沒有定論。在本論文研究中，我們由全球資訊網（WWW）取得了1998年與1999年的地面觀測之Hα影像資料以及衛星觀測之MDI（Michelson Doppler Imager）、EIT（Extreme Ultraviolet Imaging Telescope）、SXT（Soft X-ray Telescope）等影像資料。我們根據Hα影像資料決定日珥在太陽全球的分佈情形與形貌特徵。並根據日珥的緯度分佈與形貌特徵加以分類。我們再配合MDI、EIT、SXT等影像資料，分析各類型日珥的上方日冕結構與背景磁場強度。我們由資料分析的結果推論：除了Radiative cooling instability可形成日珥外，Kelvin-Helmholtz instability、magnetic buoyancy instability和Rayleigh-Taylor instability等三種機制在日珥的形成過程中，應該也扮演著重要的角色。

摘要(英)

Prominences are distinct phenomena on solar disk. However, the physical processes that can lead to formation of solar prominences are not fully understood yet.
In this study, we obtain observational data from websites. These data include Hα image data from ground-based observatories as well as MDI (Michelson Doppler Imager), EIT (Extreme Ultraviolet Imaging Telescope) and SXT (Soft X-ray Telescope) image data from SoHO and Yohkoh satellites’ observations. We analyze Hα data obtained during 1998 and 1999 to determine the distribution and shape of prominences on solar disk. We classify the observed prominences into several types according to their latitudinal distribution and their shape. For each type of prominences, we analyze the coronal structure above them and the line-of-sight magnetic field intensity around them based on MDI, EIT and SXT images.
Based on our analysis, we infer that besides radiative cooling instability, the Kelvin-Helmholtz instability, magnetic buoyancy instability and Rayleigh-Taylor instability should also play important roles on the formation of solar prominences.

關鍵字(中)

★ 日珥
★ 暗紋

關鍵字(英)

★ filaments
★ prominences

論文目次

中文摘要 i
英文摘要 ii
誌謝 iii
目錄 iv
圖目錄 v
表目錄 vi
第一章緒論 1
1.1 文獻回顧 1
1.2 研究目的 5
第二章背景介紹 6
2.1 關於日珥（暗紋） 6
2.2 觀測儀器介紹 7
第三章不同時期日珥結構和分佈之變化 12
3.1 1998年與1999年日珥的緯度分佈情形 12
3.2 不同區域的日珥結構 19
3.2.1 高緯區的日珥 19
3.2.2 中低緯區的日珥 30
3.2.3 連接性日珥 46
3.3 1999年高緯區日珥的POLEWARD移動現象 49
3.4 結果與討論 54
第四章日珥形成之理論 56
4.1 太陽的差動自轉 56
4.2 日珥的形成 60
第五章總結與討論 68
附錄A ： KELVIN-HELMHOLTZ INSTABILITY 71
參考文獻 78

參考文獻

Adams, W. and F. Tang, Differential rotation of short-lived solar filaments,
Sol. Phys., 55, 499, 1977
Amari, T., J. F. Luciani, Z. Mikic, and J. Linker, Three-dimensional solutions
of magnetohydrodynamic equations for prominence magnetic support: Twisted
magnetic flux rope, Astrophys. J., 518, 57, 1999.
Ballester, J., and E. R. Priest, A two-D model for a solar prominences, Sol.
Phys., 109, 335, 1987.
Carolus, J. S., and M. T. Alan, Today’s science of the sun, Sky & Telescope,
101, number 2, 34, 2001.
Chiueh, T., and L. C. C. Lin, Quiescent Prominence Equilibria, Astrophys. J.,
517, 1002, 1999.
Fan, Y., The emergence of a twisted Ω-tube into the solar atmosphere,
Astrophys. J. Letters, 554, L111, 2001.
Fleck, B., V. Domingo, and A. I. Poland, The SoHO Mission, ed., Kluwer Acad.,
Norwell, Mass., 1995.
Harold, Z., Solar rotation, Astrophysics of the sun, ed., the Press Syndicate
of the University of Cambridge, 1988.
Harvey, J. W., F. Hill, and R. P. Hubbard, The Global Oscillation Network Group
Project, Science, 272, 1284, 1996.
Kippenhahn, R., and A. Schlüter, Eine Theorie der solaren Filamente, Z.
Astrophys., 43, 36, 1957.
Kuperus, M., and M. A. Raadu, The support of prominences formed in neutral
sheets, Astron. Astrophys., 31, 189, 1974.
Kuperus, M., and E. Tandberg-Hansser, The Nature of Quiescent Solar
Prominences, Sol. Phys., 2, 39, 1967.
Leroy, J. L., Observation of prominences magnetic fields, In Dynamics and
Structure of Quiescent Solar Prominences, ed. E. R. Priest, Kluwer Acad.,
Dordrecht, 77, 1989.
Martin, S. F., and A. H. Mcallister, Predicting the Sign of Magnetic Helicity
in Erupting Filaments and Coronal Mass Ejections, in Coronal Mass Ejections,
edited by N. Crooker, J. A. Joselyn, and J. Feynman, p.127, 1997.
Milne, A., E. R. Priest, and B. Robert, A model for quiescent prominences,
Astrophys. J., 232, 304, 1979.
Priest, E. R., Solar magneto-hydrodynamics, ed., D.Reidel Publishing Company,
1943.
Priest, E. R., A. Hood, and U. Anzer, A twisted flux tube model for solar
prominences, Astrophys. J., 344, 1010, 1989.
Rosner, R., W. H. Tucker, and G. S. Vaiana, Dynamics of the quiescent solar
corona, Astrophys. J., 220, 643, 1978.
Schou, J., H. M. Antia, S. Basu, R. S. Bogart, R. I. Bush, S. M. Chitre, J.
Christensen-Dalsgaard, M. P. di Mauro,
W. A. Dziembowski, A. Eff-Darwich, D. O. Gough, D. A. Haber, J. T. Hoeksema,
R. Howe, S. G. Korzennik, A. G. Kosovichev, R. M. Larsen, F. P. Pijpers, P.
H. Scherrer, T. Sekii, T. D Tarbell, A. M.Title, M. J. Thompson, J. Toomre,
Helioseismic studies of Differential Rotation in the solar envelope by the
solar oscillations investigation using the Michelson Doppler Imager,
Astrophys. J., 505, 390, 1998.
Snodgrass, H. B., Magnetic rotation of the solar photosphere, Astrophys. J.,
270, 288, 1983.
Tang, F., Rotation rate of high-latitude sunspots, Sol. Phys., 69, 399,1981.
Timothy, A. F., A. S. Krieger, and G. S. Vaiana, The structure and evolution of
coronal holes, Sol. Phys., 42, 135, 1975.
van Ballegooijen, A. A., E. R. Priest, D. H. Mackay, Mean field model for the
formation of filament channels on the sun, Astrophys. J., 539, 983, 2000.
林敏德，日側磁層頂之Kelvin-Helmholtz不穩定性之研究，
碩士論文，國立中央大學，1996

指導教授

呂凌霄(Ling-Hsiao Lyu)

審核日期

2002-7-9

推文