日冕物質拋射運動性質分析

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李先明(Hsien-ming Li) 查詢紙本館藏

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太空科學研究所

論文名稱

日冕物質拋射運動性質分析
(The Analysis of Coronal Mass Ejections Kinematic Properties)

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摘要(中)

本論文用STEREO(Solar Terrestrial Relations Observatory)太空船上的SECCHI(Sun Earth Connection Coronal and Heliospheric Investigation)儀器研究2008年3月25日及12月12日兩個日冕物質拋射事件，第一個事件伴隨強度M1.7級的閃焰，最高加速度距太陽表面0.55太陽半徑處，強度達1020.8 m/s2；第二個事件則是在日珥爆發後發生，距太陽表面1.98太陽半徑處，最高加速度達28.9 m/s2。兩事件在傳播過程中在速度上有明顯不同的性質，第一個事件起始速度快速增加但隨著距離的增加，速度逐漸下降，第二個事件起始速度低但隨著距離的增加，速度逐漸上升，造成如此不同的運動型態有可能是在傳播時受到太陽風的影響。伴隨閃焰事件加速度增加行為與軟X光射線通量微分值在時間的尺度上具有一致的關係。分別用等加速度及變加速度的冪次多項式擬合日冕物質拋射高度，結果顯示以變加速度的冪次多項式優於等加速度的冪次多項式，表示這兩個事件的加速度具有時變性質。

摘要(英)

The objective of this work is to study the kinematic properties of two coronal mass ejections (CMEs) detected on 2008 March 25 and December 12 respectively by the SECCHI (Sun Earth Connection Coronal and Heliospheric Investigation) on-board STEREO (Solar Terrestrial Relations Observatory) spacecraft. The first CME was associated with an M1.7 class solar flare. Its highest acceleration occurred at about 0.55 R☉ from the solar surface with a magnitude of 1020.8 m/s2. The second event broke out after a prominence eruption. Its maximum acceleration occurred at about 1.98 R☉ from the solar surface with a magnitude of 28.9 m/s2. The kinematics profiles of the two CMEs are different. The velocity of the first event rises rapidly during the initial phase and then decreases afterward, while the velocity of the second one increases monotonically. The cause of the difference may be due to the effect of solar wind. The peak acceleration of the first event coincided with the peak of the derivative of the soft X-ray flux. The CME heights were fitted by the polynomials derived from constant and variable acceleration, respectively. The fitting results show that the “variable acceleration” polynomial fits both events better than the “constant acceleration” polynomial does. This means that the accelerations of both CMEs are time-varying.

關鍵字(中)

★ 日冕物質拋射
★ 運動性質

關鍵字(英)

★ coronal mass ejections
★ kinematic property

論文目次

中文摘要 ………………………………………………i
英文摘要 ………………………………………………ii
誌謝 ………………………………………………iii
目錄 ………………………………………………iv
圖目錄 ………………………………………………vi
表目錄 ………………………………………………xii
符號說明 ………………………………………………xiii
一、研究動機與目的………………………………………1
1-1研究動機…………………………………………………1
1-2研究目的…………………………………………………1
二、太陽與太陽活動事件簡述………………………………3
2-1太陽………………………………………………………3
2-2太陽活動事件……………………………………………5
三、日冕物質拋射……………………………………………9
3-1概述………………………………………………………9
3-2觸發機制…………………………………………………10
3-2-1需要磁重聯作為觸發機制的模式－爆發模式………11
3-2-2無需磁重聯作為觸發機制的模式－質量負載模式…12
3-3運動傳播性質……………………………………………12
四、儀器與資料處理…………………………………………15
4-1儀器…………………………………………………………15
4-2資料處理……………………………………………………19
五、研究方法……………………………………………………21
5-1概述…………………………………………………………21
5-2三維三角法…………………………………………………22
5-3正運算法……………………………………………………25
5-4誤差計算……………………………………………………29
六、事件分析與討論……………………………………………31
6-12008年3月25日事件………………………………………31
6-22008年12月12日事件……………………………………50
6-3兩事件運動性質綜合比較…………………………………64
6-4討論…………………………………………………………70
6-4-1運動性質…………………………………………………70
6-4-2日冕物質拋射加速現象與閃焰關係……………………71
6-4-3日冕物質拋射傳播………………………………………72
七、總結與未來研究方向………………………………………75
7-1總結…………………………………………………………75
7-1-12008年3月25日事件……………………………………75
7-1-22008年12月12日事件…………………………………76
7-2未來研究方向………………………………………………77
參考文獻 ………………………………………………………78

參考文獻

〔1〕K. D. Abhyankar, “A survey of the solar atmospheric models”, Bull. Astr. Soc. India, Vol 5, pp. 40-44, June 1977.
〔2〕D. Alexander, T. R. Metcalf, and N. V. Nitta, “Fast acceleration of a CME-related X-ray structure in the low solar corona”, Geophys. Res. Lett., Vol 29, pp. 44-1 - 44-4, October 2002.
〔3〕S. K. Antiochos, C. R. DeVore, J. A. Klimchuk, “A Model for Solar Coronal Mass Ejections”, ApJ, Vol 510, pp. 485-493, January 1999.
〔4〕R. Aster, B. Borchers, and C. Thurber, Parameter Estimation and Inverse Problems, Second Edition, Elsevier, 2012.
〔5〕Aschwanden, M. J., Physics of the solar corona: An Introduction, Praxis Publishing Ltd., Chichester, UK, 2004.
〔6〕M. J. Aschwanden, N. V. Nitta, J. Wuelser, and J. R. Leman et al., “First measurements of the mass of coronal mass ejections from the EUV dimming observed with STEREO EUVI A+B spacecraft”, ApJ, Vol 706, pp. 376-392, October 2009.
〔7〕Bevington, P. R., Data reduction and error analysis for the physical science, McGraw-Hill Co., New York, USA,1969.
〔8〕J. D. Bohlin and N. R. Sheeley, “Exteme ultraviolet observations of coronal holes”, Sol. Phys., Vol 56, pp. 125-151, January 1978.
〔9〕B. M. Bein, S. Berkebile-Stoiser, A. M. Veronig, and M. Temmer et al., “Impulsive Acceleration of Coronal Mass Ejections. II. Relation to Soft X-Ray Flares and Filament Eruptions”, ApJ, Vol 755, pp. 44-1-44-2, August 2012.
〔10〕L. Burlaga, E. Sittler, F. Mariani, and R. Schwenn, “Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations”, J. Geophys. Res., Vol 86, pp. 6673-6684, August 1981.
〔11〕P. J. Cargill, “On the aerodynamic drag force acting on interplanetary coronal mass ejections”, Sol. Phys., Vol 221, pp. 135-149, May 2004.
〔12〕J. Chen, “Effects of toroidal forces in current loops embedded in a background plasma”, ApJ, Vol 338, pp. 453-470, March 1989.
〔13〕J. Chen, “Theory of prominence eruption and propagation: interplanetary consequences”, J. Geophys. Res., Vol 101, pp. 27499-27519, December 1996.
〔14〕H. Cremades, O. C. St. Cry, “Coronal mass ejections: solar cycle aspects”, Adv. Space Res., Vol 40, pp. 1024-1048, October 2007.
〔15〕K. P. Dere, G. E. Brueckner, R. A. Howard, and D. J. Michels et al., “LASCO and EIT Observations of Helical Structure in Coronal Mass Ejections”, ApJ, Vol 516, pp465-474, May 1999.
〔16〕C.J. Eyles, R. A. Harrison, C. J. Davis, and N. R. Waltham et al., “The Heliospheric Imagers Onboard the STEREO Mission”, Sol. Phys., Vol 254, pp. 387-445, January 2009.
〔17〕R. A. Frazin and P. Janzen, “Tomography of the solar corona. II. robust, regularized, positive estimation of the three-dimensional electron density distribution from LASCO-C2 polarized white-light images”, ApJ, Vol 570, pp408-422, May 2002.
〔18〕H. R. Gilbert, T. E. Holzer, J. T. Burkepile, and A. J. Hundhausen, “Active and eruptive prominences and their relationship to coronal mass ejections”, ApJ, Vol 537, pp503-515, July 2000.
〔19〕N. Gopalswamy, A. Lara, R. P. Lepping, and M. L. Kaiser et al., “Interplanetary acceleration of coronal mass ejections”, Geophys. Res. Lett., Vol 27, pp. 145-148, January 2000.
〔20〕N. Gopalswamy, A. Lara, S. Yashiro, M. L. Kaiser, and R.A. Howard, “Predicting the 1-AU arrival times of coronal mass ejections”, J. Geophys. Res., Vol 106, pp. 29207-29218, December 2001.
〔21〕N. Gopalswamy, A. Lara, S. Yashiro, and R.A. Howard, “Coronal mass ejections and solar polarity reversal”, ApJ, Vol 598, pp. L63-L66, November 2003.
〔22〕N. Gopalswamy, “Properties of interplanetary coronal ejections”, Space Sci. Rev., Vol 124, pp. 145-168, June 2006.
〔23〕J. T. Gosling, E. Hildner, R. M. MacQueen, and R. M., Munro et al., “The speeds of coronal mass ejection events”, Sol. Phys., Vol 48, pp. 389-397, June 1976.
〔24〕J. T. Gosling, “The solar flare myth”, J. Geophys. Res., Vol 98, pp. 18937-18949, November 1993.
〔25〕L. L. House, W. J. Wagner, E. Hildner, and C. Sawyer et al., “Studies of the corona with the Solar Maximum Mission coronagraph/polarimeter”, ApJ, Vol 244, pp. L117-L121, March 1981.
〔26〕R. A. Howard, N. R. Sheeley, D. J. Michels, and M. J. Koomen, “Coronal mass ejections 1979~1981”, J. Geophys. Res., Vol 90, pp. 8173-8191, September 1985.
〔27〕R. A. Howard, G. E. Brueckner, and O. C. St. Cry et al., “ Observations of CMEs from SOHO/LASCO”, In N. Crooker, J. A. Joselyn, and J. Feynman, Coronal mass ejections, Geophysical Monograph Vol 99, American Geophysical Union, 1997.
〔28〕A. J. Hundhausen, “Sizes and locations of coronal mass ejections: SMM observations from 1980 and 1984-1989”, J. Geophys. Res., Vol 98, pp. 13177-13200, August 1993.
〔29〕R. M. E. Illing and A. J. Hundhausen, “Observation of a coronal transient from 1.2 to 6 solar radii”, J. Geophys. Res., Vol 90, pp. 275-282, January 1985.
〔30〕B. Inhester, “Stereoscopy basics for the STEREO mission”, arXiv: astro-ph/ 0612649, December 2006.
〔31〕M. L. Kaiser, T. A. Kucera, J. M. Davila, and O. C. St. Cyr et al., “The STEREO Mission: An Introduction”, Space Sci. Rev., Vol 136, pp. 5-16, April 2008.
〔32〕I. W. Kienreich, M. Temmer, A. M. Veronig, “STEREO quadrature observations of the three-dimensional structure and driver of a global coronal wave”, ApJ, Vol 703, pp. L118-L122, October 2009.
〔33〕S. Koutchmy, F. Baudin, K. Bocchialini,and J.-Y. Daniel et al., “The August 11th, 1999 CME”, Astron. Astrophys., Vol 420, pp. 709-718, June 2004.
〔34〕R. P. Lepping, L. F. Burlaga, J. A. Jones, “Magnetic field structure of interplanetary magnetic clouds at 1 AU”, J. Geophys. Res., Vol 95, pp. 11957-11965, August 1990.
〔35〕P. C. Liewer, E. M. De Jong, J. R. Hall, R. A. Howard, and W. T. Thompson et al., “Stereoscopic analysis of the 19 May 2007 erupting filament”, Sol. Phys., Vol 256, pp. 57-72, May 2009.
〔36〕B. C. Low, J. R. Hundhausen, “Magnetostatic structures of the solar corona. 2: The magnetic topology of quiescent prominences”, ApJ, Vol 443, pp. 818-836, April 1995.
〔37〕B. J. Lynch, S. K. Antiochos, and C. R. DeVore et al., “Topological evolution of a fast magnetic breakout CME in three dimensions”, ApJ, Vol 683, pp. 1192-1206, August 2008.
〔38〕P. MacNeice, S. K. Antiochos, and A. Phillips et al., “A numerical study of the breakout model for coronal mass ejection initiation”, ApJ, Vol 614, pp. 1028-1041, October 2004.
〔39〕R. M. MacQueen and R. R. Fisher, “The kinematics of solar inner coronal transients”, Sol. Phys., Vol 89, pp. 89-102, November 1983.
〔40〕S. A. Maloney, P. T. Gallagher, “Solar wind drag and the kinematics of interplanetary coronal mass ejections”, ApJ L, Vol 724, pp. L127-L132, December 2010.
〔41〕J. T. Mariska, “The quiet solar transition region”, Ann. Rev. Astron. Astrophys., Vol 24, pp. 23-48, 1986.
〔42〕M. Mierla, J. Davila, W. Thompson, and B. Inhester et al., “A quick method for estimating the propagation direction of coronal mass ejections using STEREO-COR1 images”, Sol. Phys., Vol 252, pp. 385-396, November 2008.
〔43〕M. Minnaert, “On the continuous spectrum of the corona and its polarisation. With 3 figures”, Z. Astrophys., Vol 1, pp. 209-236, 1930.
〔44〕R. Mitalas, K. R. Sills, “On the photon diffusion time scale for the sun”, ApJ, Vol 401, pp. 759-760, December 1992.
〔45〕Y.-J. Moon, G. S. Choe, H. Wang, and Y. D. Park et al., “A Statistical Study of Two Classes of Coronal Mass Ejections” , ApJ, Vol 581, pp. 694-702, December 2002.
〔46〕D. J. Mullan, “Solar Physics: from the deep interior to the hot corona”, In D. Page, J. G. Hirsch, From the Sun to the great attractor, Springer, 2000.
〔47〕R. H. Munro, J. T. Gosling, E. Hildner, and R. M. MacQueen et al., “The association of coronal mass ejections transients with other forms of solar activity”, Sol. Phys., Vol 61, pp. 201-215, February 1979.
〔48〕W. M. Neupert, “Comparison of solar X-ray line emission with microwave emission during flares”, ApJ, Vol 153, pp. L59-L64, July 1968.
〔49〕L. Ofman, “Source regions of the slow solar wind in coronal streamers”, Geophys. Res. Lett., Vol 27, pp. 2885-2888, September 2000.
〔50〕V. N. Obridko, B. D. Shelting, “Relationship between the parameters of coronal holes and high-speed solar wind streams over an activity cycle, Sol. Phys., Vol 270, pp. 297-310, May 2011.
〔51〕A. Shanmugaraju, Y.-J. Moon, B. Vršnak and D. Vrbanec, “Radial evolution of well-observed slow CMEs in the distance range 2-30 Rsun”, Sol. Phys., Vol 257, pp. 351-361, July 2009.
〔52〕N. R. Sheeley, J. W. Harvey and W. C. Feldman, “Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976”, Sol. Phys., Vol 49, pp. 271-278, August 1976.
〔53〕N. R. Sheeley, Y.-M. Wang, S. H. Hawley and G. E. Brueckner et al., “Measurements of flow speeds in the corona between 2 and 30 Rsun”, ApJ, Vol 484, pp. 472-478, July 1997.
〔54〕N. R. Sheeley, J. H. Walters, Y.-M. Wang, R. A. Howard, “Continuous tracking of coronal outflows: Two kinds of coronal mass ejections”, J. Geophys. Res., Vol 104, pp. 24739-24768, November 1999.
〔55〕N. Srivastava, R. Schwenn, B. Inhester, and G. Stenborg et al., “Acceleration profile of the slow solar wind as inferred from gradual mass ejections observed by LASCO”, Space Sci. Rev., Vol 87, pp. 303-306, January 1999.
〔56〕O. C. St. Cyr, A. J. Hudhausen, and J. T. Burkepile, “Speeds and accelerations of coronal mass ejections”, Proceedings of the first SOHO workshop: coronal streamers, coronal loops, and coronal and solar wind composition, pp.125., November 1992.
〔57〕D. L. Stephens Jr., L. W. Townsend, and J. L. Hoff, “Interplanetary crew dose estimates for worst case solar particle events base on historical data for the Carrington flare of 1859”, Acta Astronautica, Vol 56, pp. 969-974, June 2005.
〔58〕M. Sugiura, “A note on harmonic analysis of geophysical data with special reference to the analysis of geomagnetic storms”, J. Geophys. Res., Vol 65, pp. 2721-2725, September 1960.
〔59〕M. Temmer, A. M. Veronig, E. P. Kontar, and S. Krucker et al., “Combined STEREO/RHESSI study of coronal mass ejection acceleration and particle acceleration in solar flares”, ApJ, Vol 712, pp.1410-1420, April 2010.
〔60〕A. F. R. Thernisien, R. A. Howard, A. Vourlidas, “Modeling of Flux Rope Coronal Mass Ejections”, ApJ, Vol 652, pp. 763-773, November 2006.
〔61〕A. Thernisien, A. Vourlidas, R. A. Howard, “Forward Modeling of Coronal Mass Ejections Using STEREO/SECCHI Data”, Sol. Phys., Vol 256, pp. 111-130, May 2009.
〔62〕W.T. Thompson, “3D triangulation of a Sun-grazing comet”, Icarus, Vol 200, pp. 351-357, April 2009.
〔63〕R. Tousey, “The solar corona”, Space Res., Vol 13, pp. 713-730, 1973.
〔64〕L. W. Townsend, D. L. Stephens Jr., J. L. Hoff, and E. N. Zapp et al., “The Carrington event: possible does to crews in space from a comparable event”, Adv. Space Res., Vol 38, pp. 226-231, July 2006.
〔65〕N. B. Trivedi, I. Vitorello, W. Kabata, and S. L. G. Dutra et al., “Geomagnetically induced currents in an electric power transmission system at low latitudes in Brazil: A case study”, Space Weather, Vol5, S04004, doi:10.1029/2006SW000282, April 2007.
〔66〕A. M. Veronig, M. Temmer, and B. Vršnak, “High-cadence observations of a global coronal wave by STEREO EUVI”, ApJ, Vol 681, pp. L113-L116, July 2008.
〔67〕E. Verwichte, M. J. Aschwanden, T. Van Doosselaere, and C. Foullon etal., “Seismology of a large solar coronal loop from EUVI/STEREO observation of its transverse oscillation”, ApJ, Vol 698, pp.397-404, May 2009.
〔68〕B. Vršnak, “Deceleration of coronal mass ejections”, Sol. Phys., Vol 202, pp. 173-189, August 2001.
〔69〕B. Vršnak, “Forces governing coronal mass ejections”, Adv. Space Res., Vol 38, pp. 431-440, January 2006.
〔70〕B. Vršnak and T. Zic, “Transit times of interplanetary coronal mass ejections and the solar wind speed”, Astron. Astrophys., Vol 472, pp. 937-943, September 2007.
〔71〕J. P. Wuelser, J. R. Lemena, T. D. Tarbella, and C. J. Wolfsona et al., “EUVI: the STEREO-SECCHI extreme ultraviolet imager”, Proc. SPIE, Vol 5171, pp. 111-122, February 2004.
〔72〕J. Zhang, K. P. Dere, R. A. Howard, and M. R. Kundu et al., “On the temporal relationship between coronal mass ejections and flares”, ApJ, Vol 559, pp. 452-462, September 2001.
〔73〕J. Zhang, K. P. Dere, R. A. Howard, and A. Vourlidas, “A study of the kinematic evolution of coronal mass ejections”, ApJ, Vol 604, pp. 420-432, March 2004.
〔74〕J. Zhang and K. P. Dere, “A statistical study of main and residual accelerations of coronal mass ejections”, ApJ, Vol 649, pp. 1100-1109, October 2006.
〔75〕J. Zhang, G. Richardson, D. F. Webb, and N. Gopalswamy et al. , “Solar and interplanetary sources of major geomagnetic storms (Dst ≤ −100 nT) during 1996–2005”, J. Geophys. Res., Vol 112, A10102, doi:10.1029/2007JA012321, December 2007.
〔76〕 Solar-Geophysical data prompt reports, Number 764 Part 1,National Oceanic and Atmospheric Administration, Colorado, April 2008.

指導教授

林佳賢(Chia-hsien Lin)

審核日期

2013-6-18

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