夏利東

夏利東,博士,教授。1985年至1993年,中國科學技術大學本科、碩士;1999年開始在德國哥廷根大學和馬普太陽系研究所攻讀博士學位,2003年獲得哥廷根大學天文和天體物理學博士學位。1993年參加工作,中國科學技術大學助教、講師。2003和2004年曾先後在馬普太陽系研究所和英國Armagh 天文台從事博士後研究。2004 年,中國科學技術大學副教授。2007,山東大學(威海)教授, 博士生導師。

基本介紹

個人簡介,工作經歷:,研究經歷:,主要論文,

個人簡介

夏利東教授
職稱:教授、博導
學歷:博研
學位:博士
畢業院校重潤鍵: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

工作經歷:

1993年-1999年,中芝歡邀喇國科學技術大學,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,副晚幾龍嚷教授
2007年4月,山東大學(威海)空間科學與套用物理系,教授

研究經歷:

研究方向為太陽大氣物理、日地關係物理和空間牛市仔探測。曾經從事電離層哨聲波傳播、行嚷享星際基波傳播和太陽大氣磁場重聯的欠炒燥數值研究,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慨尋燥秀人才支持計畫各1項。空間探測方面,參加國家自然科學基金重點項目“‘夸父’空間天氣探測計畫”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—“夸父計畫”的預先研究,擔任綜合論證階段有效載荷論證負責人。

主要論文

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).
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).

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