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个人简介

学习经历 2007年7月中国科学院国家天文台博士 2002年7月安徽大学学士 工作经历 2017.01 -- 至今 北京航空航天大学空间与环境学院 2016.04 --2017.01 中国科学院国家天文台研究员 2010.10 --2016.04 中国科学院国家天文台副研究员 2008.07 --2010.10 德国马普太阳系研究所博士后 2007.07 --2008.07 中国科学院国家天文台助理研究员 主要获奖情况 2011年获亚太太阳物理科学委员会颁发的“最佳论文奖” 2008年获国际空间研究委员会(COSPAR)颁发的“COSPAR青年科学家杰出论文奖” 主要公共服务 第29届IAU大会Focus Meeting13(2015年8月)的科学委员会成员 第41届COSPAR大会E2.1分会(2016年8月)执行主席 每年多次为Astronomy &Astrophysics, Solar Physics, Journal of Geophysical Research, Research inAstronomy and Astrophysics, New Astronomy等国际SCI期刊审稿

研究领域

太阳和恒星物理(主要包括:1、太阳磁周期的产生机理(发电机)和物理预报;2、太阳和日球层磁场的长期变化及其对地球气候的影响;3、类太阳恒星磁活动及磁周期)

近期论文

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Jiang,J.,Cameron,R.H., Schüssler,M., The Cause of the Weak Solar Cycle 24, Astrophys.J. Lett., 2015, 808, L28 (HMI Science Nugget,http://hmi.stanford.edu/hminuggets/?p=1234) Jiang,J., Hathaway, D. H., Cameron, R. H., Solanki, S. K., Gizon, L., Upton, L.,Magnetic Flux Transport at the Solar Surface, Space Sci. Rev.,,2014,186, 491–523 (Chapter of ISSI book on "The Solar ActivityCycle") Jiang,J., Cameron, R., and Schüssler, M., Effects of the Scatter in Sunspot GroupTilt Angles on the Large-scale Magnetic Field at the Solar Surface, Astrophys.J., 2014, 791, 5 Jiang,J., Cameron, R., Schmitt, D., and I?ik, E., Modeling solar cycles 15 to 21using a flux transport dynamo, Astron. Astrophys., 2013, 553, 128 Jiang,J., Cameron, R., Schmitt, D. and Schüssler, M., Can Surface Flux TransportAccount for the Weak Polar Field in Cycle 23? Space Sci. Rev., 2013,176, 289-298 (Chapter of ISSI book on "Cosmic Rays in theHeliosphere") Jiang,J., Cameron, R., Schmitt, D. and Schüssler, M., The solar magnetic fieldsince 1700. II. Physical reconstruction of total, polar and open flux, Astron.Astrophys. , 2011, 528, A83 Jiang,J., Cameron, R., Schmitt, D. and Schüssler, M., The solar magnetic fieldsince 1700. I. Characteristics of sunspot group emergence and reconstruction ofthe butterfly diagram, Astron. Astrophys., 2011, 528, A82 Jiang, J.,I?ik, E., Cameron, R. H., Schmitt, D. and Schüssler, M., The Effect ofActivity-related Meridional Flow Modulation on the Strength of the Solar PolarMagnetic Field, Astrophys. J., 2010, 717, 597-602 Jiang,J., Cameron, R., Schmitt, D. and Schüssler, M., Modeling the Sun's OpenMagnetic Flux and the Heliospheric Current Sheet, Astrophys. J., 2010,709, 301-307 Jiang,J., Cameron, R., Schmitt, D. and Schüssler, M., Countercell Meridional Flowand Latitudinal Distribution of the Solar Polar Magnetic Field, Astrophys.J., 2009, 693, L96-L99 JiangJie and Wang Jing-xiu, Mode selection mechanism and magnetic diffusivity ina non-axisymmetric solar dynamo model, Adv. Space Res., 2008, 41,847-880 Jiang,Jie, Choudhuri, Arnab Rai and Wang, Jingxiu, A New Explanation for theOrigin of Trans-equatorial Loops based on a Dynamo Model , Sol. Phys.,2007, 245, 19-25 Jiang,J. and Wang, J. X., A dynamo model for axisymmetric and non-axisymmetricsolar magnetic fields, Mon. Not. R. Astron. Soc., 2007, 377, 711-718 Jiang,Jie, Chatterjee, Piyali and Choudhuri, Arnab Rai, Solar activity forecastwith a dynamo model, Mon. Not. R. Astron. Soc., 2007, 381, 1527 -1542 Jiang,Jie and Wang, Jing-Xiu, A Non-axisymmetric Spherical α2-Dynamo, Chin. J.Astron. Astrophys., 2006, 6, 227-236 Cameron,R. Jiang, J., Schüssler, M., Solar Cycle 25: Another Moderate Cycle? Astrophys.J. Lett., 2016, 823, L22 asi-Espuig, M., Jiang, J., Krivova, N. A., Solanki, S. K.,Unruh, Y. C.,Yeo, K. L., Reconstruction of spectral solar irradiance since 1700 fromsimulated magnetograms, Astron. Astrophys., 2016, 590, A63 Karak, B. Jiang,J., Miesch, M. S., Charbonneau, P., Choudhuri, A. R., Flux TransportDynamos: From Kinematics to Dynamics, Space Sci. Rev. , 2014, 186, 561–602 (Chapterof ISSI book on "The Solar Activity Cycle") asi-Espuig, M., Jiang, J., Krivova1, N. A. and Solanki, S. K.,Modelling total solar irradiance since 1878 from simulated magnetograms, Astron.Astrophys., 2014, 570, A23 Cameron,R. H., Jiang, J., Schüssler, M. and Gizon L., Physical causes of solarcycle amplitude variability, J. Geophys. Res., 2014, 119, 9 Cameron,R. H., Dasi-Espuig, M., Jiang, J., Is?k,E., Schmitt, D. and Schüssler,M, Limits to solar cycle predictability: Cross-equatorial flux plumes, 2013, Astron.Astrophys., 557, A141 iengarten, T., Kleimann, J. Fichtner, H., Cameron, R. Jiang, J.,Kissmann, R., and Scherer, K., MHD simulation of the inner-heliosphericmagnetic field, J.,Geophys. Res., 2013, 118, 29 Cameron,R., Schmitt, D., Jiang, J., and I?ik, E., Surface flux evolutionconstraints for flux transport dynamos, Astron. Astrophys., 2012, 542,127 Schrinner,M., Schmitt, D., Jiang, J. and Hoyng, P., An efficient method forcomputing the eigenfunctions of the dynamo equation, Astron. Astrophys., 2010, 519, A80 Cameron,R. H., Jiang, J., Schmitt, D. and Schüssler, M., Surface Flux TransportModeling for Solar Cycles 15-21, Astrophys. J., 2010, 719, 264-270 Choudhuri,Arnab Rai, Chatterjee, Piyali and Jiang, Jie, Predicting Solar Cycle 24With a Solar Dynamo Model, Phys. Rev. Lett., 2007, 98, 131103 (selectedas "Editors' suggestion" in PRL)

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