夏利東

夏利東教授

職稱：教授、博導

學歷：博研

學位：博士

畢業院校：本科和碩士畢業於中國科學技術大學，博士畢業於德國哥廷根大學 ^[1] 

1993年-1999年，中國科學技術大學，助教、講師

1999年-2003年，德國哥廷根大學天文台博士生（馬普太陽系研究所做論文）

2003年-2004年，德國馬普太陽系研究所博士後、英國Armagh天文台博士後

2004年6月-2007年4月，中國科學技術大學地球和空間科學學院，副教授

2007年4月，山東大學（威海）空間科學與應用物理系，教授

研究方向為太陽大氣物理、日地關係物理和空間探測。曾經從事電離層哨聲波傳播、行星際基波傳播和太陽大氣磁場重聯的數值研究，參加完成了多項國家自然科學基金和重點項目子課題。主要從事太陽紫外/極紫外光譜學觀測研究，研究重點在高速太陽風的起源和加速機制、色球和低日冕大氣中的小尺度事件等，是SOHO飛船搭載的紫外輻射光譜儀（SUMER）數據分析階段的研究組成員，承擔國家自然科學基金面上項目和教育部新世紀優秀人才支持計劃各1項。空間探測方面，參加國家自然科學基金重點項目“‘夸父’空間天氣探測計劃”預研究，擔任夸父A星預研負責人；參加國家民用航天“十一五”背景項目—“夸父計劃”的預先研究，擔任綜合論證階段有效載荷論證負責人。 ^[1] 

1、Tu, C.-Y., Schwenn, R., Donovan, E., Marsch, E., Wang, J.-S., Xia, L.-D., Zhang, Y.-W., KuaFu working team, Space weather explorer - the KuaFu mission, Advances in Space Research, doi: 10.1016/j.asr.2007.04.049, 2007

2、Chen, Y., Y.Q. Hu and L.D. Xia, Two energy release processes for CMEs: MHD catastrophe and Magnetic reconnection, Advances in Space Research, doi: 10.1016/j.asr.2007.02.011, 2007

3、Xia L.-D., C.-Y. Tu, R. Schwenn, E. Donovan, E. Marsch, J.-S. Wang, Y.-W. Zhang, Z. Xiao, F.-S. Wei, The KuaFu Mission, Chinese J. of Space Science, Vol. z1, 2006

4、Lu, Q.M., Xia, L.D., Wang, S., Hybrid simulations of parallel and oblique electromagnetic alpha/proton instabilities in the solar wind, JGR, Volume 111, Issue A9, CiteID A09101,2006

5、Xia, L. D., M. D. Popescu, Doyle, J. G. and Giannikakis, J., Time series study of the EUV spicules observed by SUMER/SoHO, Astron. & Astrophys., 438, 1115-1122, 2005

6、Tu, C.-Y., Zhou, C., Marsch, E., Xia, L.-D., Zhao, L., Wang, J.-X. and Wilhelm, K., Solar Wind Origin in Coronal Funnels, SCIENCE, Volume 308, Issue 5721, pp.519-523, 2005

7、Tu, C.-Y., Zhou, C., Marsch, E., Wilhelm, K., Zhao, L., Xia, L.-D. and Wang, J.-X.., Correlation Heights of the Sources of Solar Ultraviolet Emission Lines in a Quiet-Sun Region, The Astrophysical Journal, 624, L133-L136, 2005

8、Popescu, M. D., Banerjee, D., O'Shea, E., Doyle, J. G., Xia, L. D.,Very long period activity at the base of solar wind streams, Astron. & Astrophys., 442, 1087-1090, 2005

9、Doyle, J. G., Giannikakis, J., Xia, L. D. and Madjarska, M. S., Line broadening of EUV lines across the Solar limb: A spicule contribution? Astron. & Astrophys., 431, L17-L20, 2005

10、Wiegelmann, T., Xia, L. D. and Marsch, E., Links between magnetic fields and plasma flows in a coronal hole, Astron. & Astrophys., 432, L1-L4, 2005

11、Popescu, M. D., Doyle, J. G. and Xia, L. D., Network boundary origins of fast solar wind seen in the low transition region? Astron. & Astrophys., 421, 339-348, 2004

12、Xia, L. D., Marsch, E. and Wilhelm, K., On the network structures in solar equatorial coronal holes. Observations of SUMER and MDI on SOHO, Astron. & Astrophys., 424, 1025-1037, 2004

13、Marsch, E., Wiegelmann, T. and Xia, L. D., Coronal plasma flows and magnetic fields in solar active regions. Combined observations from SOHO and NSO/Kitt Peak, Astron. & Astrophys., 428, 629-645, 2004

14、Xia, L.D., Marsch, E. and Curdt, W., On the outflow in an equatorial coronal hole, Astron. & Astrophys., 399, L5-L9, 2003

15、Wilhelm, K., Dammasch, I. E. and Xia, L.D., Observations of ultraviolet emission lines in solar coronal holes on the disk with SUMER on SOHO, Advances in Space Research, 30, 517-522, 2002

16、Xia, L.D. and Marsch, E., Equatorial Coronal Holes and Their Relation to High-Speed Solar Wind Streams, SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference. AIP Conference Proceedings, 679, 319-322, 2003

17、Xia, L. D. and Marsch, E. and Wilhelm, K., Topological Changes of the Magnetic Network as Seen in Different UV/EUV Emission Lines, ESA SP-547, p.169, 2004

18、Xia, L.D. and Marsch E., Observational Constraints on Ion Acceleration by Waves in Coronal Holes, ESA SP-547, p.387, 2004

19、Xia, L. D., Popescu, M. D. and Doyle, J. G., Dynamic Properties of Solar Spicules Observed by SUMER/SOHO, ESA SP-575, p.362, 2004

20、Popescu, M. D., Xia, L. D. and Doyle, J. G., Temporal Evolution of the Magnetic Network in Polar Coronal Holes, ESA SP-575, p.513, 2004

21、Xia, L. D., M. D. Popescu, Chen, Y. and Doyle, J. G., On the connection between the disk and limb events observed by SOHO, ESA SP-592, p.575, 2005

22、Liu W., Hu, Y. Q., Xia L. D. and Yang Y. L., “Disturbance of prominence caused by magnetic cancellation”, Chinese Astronomy and Astrophysics, V. 24, Issue 3, 2000.

23、Hu Y. Q., Xia L. D., Li X., Wang J. X. and Ai G. X., "Evolution of Magnetic Helicity in Magnetic Reconnection", Solar Physics, V.170, 283, 1997.

24、Xia L. D. and Hu Y. Q., "Numerical Study of the Propagation of Interplanetary Pressure Disturbance", J. of China University of Science and Technology, V.27, No.3, 1997 (in Chinese).

25、Hu Y. Q., Xia L. D., Li X., Wang J. X. and Ai G. X., "Helicity Conservation in Magnetic Reconnection", Chinese Science Bulletin, V.42, No.5, 1997.

26、Hu Y. Q. and Xia L. D., "Numerical Simulation of Flare‑induced Shock Waves", Chinese J. of Space Science, V.17, No.1, 1997 (in Chinese).

27、Xia L. D. and Hu Y. Q., "Interaction between Flare‑induced Shocks", Chinese J. of Space Science, V.17, No.1, 1997 (in Chinese).

28、Hu Y. Q. and Xia L. D., "Origin of Solar Wind Stream Interfaces", ACTA Geophysica Sinica, V.39, No.1, 1996.

29、Liu S. L., Xia L. D. and Hu X. L., "Radial Distribution of the Interplanetary Fast Shock between 0.3 and 1.0AU", Proc. of the Third SOLTIP Symposium, p.425, 1996.

30、Xia L.D. and Wang Y.S., "A Statistical Analysis of the observations of Whistler atSanya Area", J. of China University of Science and Technology, V.24, No.3, 1994 (in Chinese). ^[1]