代表论著: |
[1] Xu,Z.,Lagg, A., Solanki, S., 2010,Magnetic structure of an emerging flux region in the solar photosphere and chromosphere.,A&A, 520, 77.
[2] Xu, Z. Lagg, A, Solanki ,S., 2012, Magnetic Fields of an Active Region Filament from Full Stokes Analysis of Si I 1082.7 and He I 1083.0 nm., ApJ, 749 138.
[3] Wang, R., Xu, Z., Jin, Z., Li, Z., Fu, Y., Liu,Z.., 2013, The first observation and data reduction of the Multi-wavelength Spectrometer on the New Vacuum Solar Telescope.,, RAA, 13, 1240.
[4] Feng, S., Xu, Z., Wang, F., Deng, H., Yang, Y. Ji, K., 2014,Automated Detection of Low-Contrast Solar Features Using the Phase-Congruency Algorithm. , SoPh, 77.
[5] Xu, F., Xu, Z., Xu,S., Fu, Y., Guo, T., Wang, R., 2014, Installation of an Near-infrared Spectrograph on the New Vacuum Solar Telescope and the First observation around Fe I 1.56 Micron., Astronomical Research & Technology-Publications of National Astronomical Observatories of China., 11(2).
[6] Xu, Z., Yang,L, Xiang,Y.,Mao,W., Jin, Z., 2014, Investigation of a scanned profile of the narrow-band Halpha Lyot Filter of the New Vacuum Solar Telescope., Astronomical Research & Technology-Publications of National Astronomical Observatories of China.
[7] Xu, Z., Hénoux, J.-C., Chambe, G., Karlicky, M., Fang, C.? 2005, Multiwavelength Analysis of the Impact Polarization of 2001 June 15 Solar Flare, ApJ, 631, 618-627.
[8] Xu, Z., Hénoux, J.-C., Chambe, G., Karlicky, M., Fang, C, 2005, Information on particle acceleration and transport derived from solar flare spectropolarimetry, Adv. Space Res., 35, 1841-1845.
[9] Xu, Z., Fang, C., Gan, W.-Q. , 2005, Multi-wavelength Diagnostics of Bombardment by Non-thermal Particles in Solar Flares, ChJAA, 5, 519-530.
[10] Xu, Z., Hénoux, J. C., Chambe, G., Petrashen, A. G., Fang, C., 2006, First Results of Mg I (3p 1P1-4d 1D2) Line Linear Impact Polarization during the Solar Flare on 2001 June 15, ApJ, 650, 1193-1198.
[11] Xu, Z., Zhang, S., 2006, Polarization observation of white light corona during the total solar eclipse?on?2006?march 29, Astronomical Research and Technology, 2006, 3, 408 – 413. |