姜傑

太陽和恆星物理（主要包括：1、太陽磁周期的產生機理（發電機）和物理預報；2、太陽和日球層磁場的長期變化及其對地球氣候的影響；3、類太陽恆星磁活動及磁周期）

2007年7月中國科學院國家天文台博士

2002年7月安徽大學學士

2017.01 -- 至今 北京航空航天大學空間與環境學院

2016.04 --2017.01 中國科學院國家天文台研究員

2010.10 --2016.04 中國科學院國家天文台副研究員

2008.07 --2010.10 德國馬普太陽系研究所博士后

2007.07 --2008.07 中國科學院國家天文台助理研究員

2011年獲亞太太陽物理科學委員會頒發的“最佳論文獎”

2008年獲國際空間研究委員會(COSPAR)頒發的“COSPAR青年科學家傑出論文獎”

1. 第29屆IAU大會Focus Meeting13（2015年8月）的科學委員會成員；

2. 第41屆COSPAR大會E2.1分會（2016年8月）執行主席；

3. 每年多次為Astronomy &Astrophysics, Solar Physics, Journal of Geophysical Research, Research inAstronomy and Astrophysics, New Astronomy等國際SCI期刊審稿；

1. May 2017, SessionI: Solar photosphere and solar cycle, The First China-Europe Solar PhysicsMeeting, Kunming China.

2. August2016, Global solar dynamo, Conference on Solar and Stellar Magnetic Fields,Goslar Germany.

3. March 2016,Observation-based stochastic effects and nonlinearities in the solarlarge-scale magnetic field evolution, ISSI/VarSITI forum on Futureevolution of solar activity, Bern Switzerland.

4. November2015, Dynamo Models and Solar Cycle Predictions, The third Asia-Pacific solarphysics meeting, Seoul Korea (cancelled due to visa issue)

5. August2015, Primary cause of the weak solar cycle 24, Asia Oceania GeosciencesSociety (AOGS) 12th Annual Meeting, Singapore

6. June 2015, Advancesin dynamo modeling: convective dynamos, NASA LWS Workshop on Solar DynamoFrontiers: Helioseismology, 3D Modeling, and Data Assimilation, HAO USA(cancelled due to visa issue).

7. October2014, Evolution of the solar polar field, SCOSTEP-13th Solar TerrestrialPhysics symposium, Xi'an China.

8. November2013, The roles of the meridional flow in the solar flux transport dynamos,ISSI workshop, The solar activity cycle: physical causes and consequences,Bern Switzerland.

9. October2013, Causes and consequences of the solar polar field around cycle minima, Thesecond Asia-Pacific solar physics meeting, Hangzhou China.

10. April2013, Polar field around cycle minima versus subsequent and preceding solarcycles, AGU Chapman Conference on the Causes and Consequences of theExtended Solar Minimum Between Solar Cycles 23 and 24, Florida USA

11. August2012, Solar-cycle precursors and predictions, IAU Symposium 294--Solarand astrophysical dynamos and magnetic activity, Beijing China.

12. August2012, Solar magnetic field, XXVIII IAU General Assembly Special Session10, Beijing China.

13. August2011, Solar cycle prediction using dynamos and its implication for the solarcycle, International Living with a Star-2011 Workshop (ILWS-2011),Beijing China.

14. April2010, The Current solar minimum, ISSI workshop, Cosmic Rays in theHeliosphere II, Bern Switzerland.

15. October2009, Modeling the Interplanetary Magnetic Field, The 2nd international spaceweather symposium, Nanjing China.

16. July 2006,A Non-axisymmetric Solar Dynamo model, the 36th COSPAR-E2.1.

1. 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)

2. 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")

3. 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

4. Jiang,J., Cameron, R., Schmitt, D., and Işik, E., Modeling solar cycles 15 to 21using a flux transport dynamo, Astron. Astrophys., 2013, 553, 128

5. 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")

6. 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

7. 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

8. Jiang, J.,Işik, 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

9. 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

10. 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

11. JiangJie and Wang Jing-xiu, Mode selection mechanism and magnetic diffusivity ina non-axisymmetric solar dynamo model, Adv. Space Res., 2008, 41,847-880

12. 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

13. 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

14. Jiang,Jie, Chatterjee, Piyali and Choudhuri, Arnab Rai, Solar activity forecastwith a dynamo model, Mon. Not. R. Astron. Soc., 2007, 381, 1527 -1542

15. Jiang,Jie and Wang, Jing-Xiu, A Non-axisymmetric Spherical α2-Dynamo, Chin. J.Astron. Astrophys., 2006, 6, 227-236

16. Cameron,R. Jiang, J., Schüssler, M., Solar Cycle 25: Another Moderate Cycle? Astrophys.J. Lett., 2016, 823, L22

17. Dasi-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

18. 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")

19. Dasi-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

20. Cameron,R. H., Jiang, J., Schüssler, M. and Gizon L., Physical causes of solarcycle amplitude variability, J. Geophys. Res., 2014, 119, 9

21. Cameron,R. H., Dasi-Espuig, M., Jiang, J., Isık,E., Schmitt, D. and Schüssler,M, Limits to solar cycle predictability: Cross-equatorial flux plumes, 2013, Astron.Astrophys., 557, A141

22. Wiengarten, 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

23. Cameron,R., Schmitt, D., Jiang, J., and Işik, E., Surface flux evolutionconstraints for flux transport dynamos, Astron. Astrophys., 2012, 542,127

24. Schrinner,M., Schmitt, D., Jiang, J. and Hoyng, P., An efficient method forcomputing the eigenfunctions of the dynamo equation, Astron. Astrophys., 2010, 519, A80

25. Cameron,R. H., Jiang, J., Schmitt, D. and Schüssler, M., Surface Flux TransportModeling for Solar Cycles 15-21, Astrophys. J., 2010, 719, 264-270

26. 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)