基本信息
林隽 男 汉族 博导 云南天文台
电子邮件：jlin@ynao.ac.cn
联系电话：**
手机号码：
通信地址：昆明市东郊凤凰山云南天文台
邮政编码：650011

研究领域太阳物理
招生信息

招生专业070401-天体物理
070420-天文技术与方法
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070401-天体物理
070420-天文技术与方法
-
招生方向太阳活动与日地关系
实测天体物理
太阳物理
天文仪器与方法
教育背景1， 1981--1985年南京大学天文系天体物理专业，获理学学士学位。
2， 1985--1988年获得南京大学天体物理学硕士学位，导师章振大教授。


出国学习工作 1997--2001年在美国新罕布什尔（New Hampshire）大学获物理学博士学位，导师Terry G. Forbes教授。

1994年11月--1994年12月意大利Torino 大学物理研究所访问学者，研究太阳耀斑能量释放机制。

1995年12月--1996年12月获得了香港王宽诚 (K. C. Wong) 奖(贷)学金的资助，在美国新罕布什尔州立大学(University of New Hampshire, Durham, NH, USA) 空间研究中心，在另一位国际太阳物理学界理论权威T. G. Forbes教授的指导下进行太阳爆发理论模型的研究。

1997年7月--2001年6月在Forbes教授的帮助下转入新罕布什尔州立大学物理系博士研究生的学习和研究程序。2001年9月获得物理学博士学位 (PhD in Physics)。

2001年7月—2005年3月，到哈佛-史密松天体物理中心 (Harvard-Smithsonian Center for Astrophysics) 工作，在太阳和恒星部UVCS研究组从事空间资料研究。

工作经历2005年4月—现在，科学院第三期创新工程云南天文台《太阳活动与CME理论研究》团组首席科学家。研究领域及兴趣：理论太阳物理，太阳爆发（太阳耀斑，爆发日珥，日冕物质抛射）过程中的等离子体和磁场特征，不稳定性，磁力线重联，解析模型。

专利与奖励A， 1992年8月获中国天文学会青年优秀科技论文奖二等奖；
B， 1999年1月获教育部科学技术进步奖二等奖；
C， 2000年6月获美国天文学会太阳物理部奖学金奖
D，2006年申请了杰出青年基金，获得“杰青”称号

奖励信息
出版信息

发表论文1. Ma, S., Attrill, G. D. R., Golub, L., & Lin, J.: `Statistical Study of Coronal Mass
Ejections With and Without Distinct Low Coronal Signatures', 2010, ApJ, 722, 289;

2. Lin, J.,Wang, X., & Meng, Y.: `The catastrophe theory and applications to the solar eruption and other research areas of astrophysics', 2010, Progress in Astronomy, 28, 10;

3. Ma, Y., Wang, D., Lin, J., Dai, S., & Zhang, X.: `Associations of decimetric type III bursts with coronal mass ejections and H ares', 2010, RAA, 10, 484;

4. Ma, S., Wills-Davey, M. J., Lin, J., et al.: `A New View of Coronal Waves from
STEREO', 2009, ApJ, 707, 732;

5. Lin, J.: `Studies of Solar Flares and CMEs Related to the Space Missions in the Future', 2009, Sci. China Ser. G, 52 1646.

6. Wang, H., Shen, C. & Lin, J.:`Numerical Experiments of Wave-Like Phenomena Caused by the Disruption of an Unstable Magnetic Con guration', 2009, Astrophys. J., 700, 1716.

7. Lin, J., Li, J., Ko, Y.-K., & Raymond, J. C.: `Investigation of Thickness and
Electrical Resistivity of the Current Sheets in Solar Eruptions', 2009, Astrophys. J., 693, 1666.

8. Lin, J., Cranmer, S. R., & Farrugia, C. J.: `Plasmoids in Reconnecting Current Sheets: Solar and Terrestrial Contexts Compared', 2008, J. Geophys. Res., 113, A11107.

9. Mei, Z., & Lin, J.: `Changes in the Photospheric Magnetic Field Associated with Solar Flares', 2008, New Astron., 13, 526.

10. Lin, J.: `Observational Features of Large-Scale Structures Revealed by the Catas- trophe Model in Solar Eruptions', 2007, Chinese J. Astron. Astrophys., 7, 457.

11. Lin, J.: `Thickness and Electrical Resistivity of the Current Sheet in Solar Erup- tions', 2007, Adv. GeoSci., 14, 83.

12. Lin, J.: `Start Frequencies and Onset Positions of Type II Radio bursts i Solar Eruptions', 2007, Adv. GeoSci., 14, 141.

13. Lin, J., Li, J., Forbes, T. G., Ko, Y.-K., Raymond, J. C., & Vourlidas, A.: `Features and Properties of Coronal Mass Ejection/Flare Current Sheets', 2007, Astrophys. J., 658, L123.

14. Lin, J., Mancuso, S., & Vourlidas, A.:`Theoretical Investigation of the Onsets of Type II Radio Bursts during Solar Eruptions', 2006, Astrophys. J., 649, 1110.

15. Huang, G., & Lin, J.: `Quasi-Periodical Reversal of Radio Polarizations at 17 GHz Observed in 2002 April 21 Event', 2006, Astrophys. J., 639, L99.

16. Lin, J., & van Ballegooijen, A. A.: `Equilibrium and Evolution in the Multipolar Magnetic Con gurations Resulting from Interactions among Active Regions', 2005, Astrophys. J., 629, 582.

17. Lin, J., Ko, Y.-K., Sui, L., Raymond, J. C., Stenborg, G. A., Jiang, Y., Zhao, S., & Mancuso, S.: `Direct Observations of Magnetic Reconnection Site of An Eruption on November 18, 2003', 2005, Astrophys. J., 622, 1251.

18. Lin, J., and Soon, W.: `Evolution of Morphological Features of CMEs Deduced from Catastrophe Model of Solar Eruptions', 2004, New Astronomy, 9(8), 611-628.

19. Lin, J.: `Motions of Flare Ribbons and Loops in Various Magnetic Con gurations', 2004, Solar Phys., 222, 115-136.

20. Lin, J.: `CME-Flare Association Deduced from Catastrophic Model of CMEs', 2004, Solar Phys., 219, 169;

21. Lin, J., Raymond, J. C., and van Ballegooijen, A. A.: `The Role of Magnetic Recon- nection in The Observable Features of Solar Eruptions', 2004, Astrophys. J., 602, 422;

22. Ko, Y.-K., Raymond, J. C., Lin, J., Lawrence, G., Li, J., Fludra, A., `Dynamical and Physical Properties of a Post-CME Current Sheet', 2003, Astrophys. J., 594, 1068;

23. Lin, J., Soon, W., and Baliunas, S. L, `Theories of Solar Eruptions: A Review', 2003, New Astronomy Review , 47(2), 53-84;

24. Lin, J., Soon, W., and Baliunas, S. L, `Eruptive Processes in Solar Atmosphere and Theories', 2002, Chinese Science Bulletin (in Chinese), 47(21), 1601-1612;

25. Lin, J., van Ballegooijen, A. A., and Forbes, T. G.: `Evolution of A Semi-Circular Flux Rope with Two Ends Anchored in The Photosphere', 2002, J. Geophys. Res., 107(A12), 1438;

26. Lin, J.: `Energetics and Propagation of Coronal Mass Ejections in Di erent Plasma Environments', 2002, Chinese J. Astron. Astrophys., 2(No.6), 539-556;
27. Lin, J., and van Ballegooijen, A. A.: `Catastrophic and Noncatastrophic Mecha- nisms for Coronal Mass Ejections', 2002, Astrophys. J., 576, 485;

28. Lin, J., Forbes, T. G., and Isenberg, P. A.: `Prominence Eruptions and Coronal Mass Ejections Triggered by Newly Emerging Flux', 2001, J. Geophys. Res., 106(A11), 25053;

29. Forbes, T. G., and Lin, J.: `What Can We Learn about Reconnection from Coronal Mass Ejections?', 2000, Journal of Atmospheric and Solar-Terrestrial Physics, 62, 1499.

30. Lin, J. and Forbes, T. G.: `E ects of Reconnection on The Coronal Mass Ejection Process', 2000, J. Geophys. Res., 105(A2), 2375;

31. Lin, J., Forbes, T. G., Isenberg, P. A. and Demoulin, P.: `The E ect of Curvature on Flux-Rope Models of Coronal Mass Ejections', 1998, Astrophys. J., 504, 1006;

32. Zhang, Z., Lin, J., Chen, J. and Wu, N.: `Researches on Ideal MHD Models of Coronal Mass Ejections', 1998, Progress in Astronomy (in Chinese), 16, 196;

33. Xuan, J. Y., Gu, X. M., Lin. J., and another three co-authors: `Time Evolution and Morphological Characteristics of White-Light Flare on January 1989', 1998, Astron. Astrophys. Supple. Series, 129, 553;

34. Lin, J., Martin, R. and Wu, N.: `Higher Blueshift Components in Higher-Resolution FeXXV line Pro les as An Evidence of Time-Dependent Petschek-Type Reconnec-tion', 1996, Astron. Astrophys., 311, 1015;

35. Li, K. J., Lin, J., Gu, X. M. and Zhong, S. H.: `Quantitative Analysis of The Surge on March 19, 1989', 1996, Solar Phys., 168, 91;

36. Gu, X. M., Lin, J., Li, K. J. and Dun, J. P.: `Multi-Cloud Model Method and Its
Applications to The Study of Asymmetry Spectral Pro les', 1996, Astrophys. and Space Sci., 240, 263;

37. Lin, J., Forbes, T. G., Priest, E. R., and Bungey, T. N.: `Models for the Motions of Flare loops and Ribbons', 1995, Solar Phys., 159, 275;

38. Lin, J., Rijnbeek, R. P., Semenov, V. S.: `Analysis of Petschek-Type Reconnection in Y-type Magnetic Field Distribution', 1995, Planet. Space Sci., 43, No. 7, 923;

39. Gu, X. M., Li, K. J., and Lin, J.: `The Multi-Cloud Model Method and Its appli-
cations to the Study of Asymmetric Pro les of Spectral Lines Forms by Discrete
Objects on the Sun', 1995, Acta Astrophys. Sinica, 15, No. 4, 365;

40. Gu, X. M., Lin, J., Li, K. J. and other three co-authors: `Kinematic Characteristics of The Surge on March 19, 1989', 1994, Astron. Astrophys., 282, 240;

41. Wang, J. C., Xie, G. Z. and Lin, J.: `The Physics E ect of Relativistic Electron
Beam in Active Galactic Nuclei', 1994, Acta Astrophys. Sinica, 14, 217;

42. Wang, J. C., Xie, G. Z. and Lin, J.: `A Quantitative Model of Coherent, Stimulated Emission in Astrophysical Jets', 1994, Astrophys. and Space Sci., 213, 257; 10

43. Xuan, J, Y. and Lin, J.: `Two-Dimensional Multiband Spectroheliograh', 1993, Solar Phys., 144, 307;

44. Lin, J. and Zhang, Z.: `The E ects of AlfvenWaves on Heating Plasma in Post-Flare Loops', 1992, Astrophys. and Space Sci., 187, 291;

45. Lin, J., Zhang, Z., Wang, Z. and Smartt, R. N.: `The Morphology Characteristics and The Cooling Mechanisms of Post-Flare Loop System on April 28, 1980', 1992, Astron. Astrophys., 253, 557;

46. Gu, X. M., Lin, J., Luan, T. and Schmieder, B.: `Time Evolution of A Two-Ribbon Flare: Characteristics of Post-Flare Loops', 1992, Astron. Astrophys., 259, 649;

47. Xuan, J. Y., Zhong, S. H., Luo, Z., Lin, J. and other two co-workers: `The Spectral Observations of Continuous Emission of A Solar Flare on Jan. 18, 1989', 1992, Chinese Science Bulletin (in English), 37, 391;

48. Gu, X., Lin, J. and Li, Q.: `Quantitative Research on The Velocity Field of a
Post-Flare Loop Prominence System', 1991, Chinese Journal of Space Science (in Chinese), 11, 291;

49. Lin, J., Zhang, Z., Wang, Z. and Smartt, R. N.: `The Evolutional Features in
Morphology and Its Cooling Mechanism of the Post-Flare Loop System on April 28, 1980', 1990, Acta Astron. Sinica (in Chinese), 31, 313;

50. Lin, J., Wang, Z., Zhang, Z. and Smartt, R. N.: `The Plasma Nature of Cool Flare Loops of April 28, 1980', 1989, Acta Astron. Sinica (in Chinese), 30, 52;

51. Zhang, Z., Lin, J. and Wang, Z.: `The Contribution of Plasma Turbulent Fields to The Stark Broadening Functions', 1989, Acta Astrophys. Sinica, 9, 60;

发表著作Theoretical Investigations of Mechanisms for Solar Eruptions
Jun Lin &Terry G. Forbes
978-3-639-06965-5
科研活动A， 2005年12 月 5—9日在加利福尼亚洲旧金山AGU秋季年会上作“太阳爆发的灾变模型和观测结果”的特邀报告；
B， 2005年3 月 8—10日在日本Hyogo县的 Awajishima 岛给出题为“磁重联，等离子合并和磁喷射---天体物理重联和粒子加速”特邀报告；
C， 2004年10 月 18—22日在美国新墨西哥萨克峰天文台第22次学术讨论会上作题为“和太阳表面爆发现象有关的大尺度组织”的特邀报告；
D， 2003年10 月 14—16日在美国科罗拉多的波尔多高山天文台学术研讨会上做邀请报告。


科研项目

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指导学生已指导学生

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