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2.Qu, Z.Q.,Dun, G.T., Chang, L., Murray, G., Cheng, X.M., Zhang, X.Y., and Deng, L.H., 2017, “Spectro-imaging Polarimetry of the Local Corona during Solar Eclipse”, Solar Physics, 292, 37;
3. Qu,Z.Q., Deng,L.H., Dun,G.T., Chang,L., Zhang,X.Y., Cheng,X.M., Allington-Smith, J., Murray,G., Qu,Z.N., Xue,Z.K. and Ma,L., 2013,“On the Combination of Imaging-polarimetry with Spectropolarimetry of Solar Upper Atmospheres during Solar Eclipses”,ApJ,774,71;
4.Qu,Z.Q., Sun,J., Song,W., Yan,X.L.,2013,“Polarimetric properties of Mercury-like and Venus-like exoplanets”,P&SS, 78, 33;
5.Qu,Z.Q., Dun,G.T., 2012, “Spectral line intensity irreversibility in circulatory plasma magnetization processes”, APL, 100,2402-2405;
6.Qu,Z.Q.,2011,“A Fiber Arrayed Solar Optical Telescope (FASOT)”, ASPC, 437, 423-430;(SPW6会议文集);
7.Qu ,Z.Q., Zhang, X.Y., Xue, Z.K., Dun, G.T., Zhong, S.H., Liang, H.F., Yan, X.L. and Xu, C.L., 2009, ‘Linear Polarization of Flash Spectrum Observed from a Total Solar Eclipse in 2008’, ApJ, 695, L194-L197;
8.Qu, Z.Q., Xu, C .L. Zhang, X.Y.; Yan, X.L.; Jin, C.L., 2006, “On the influence of magnetic fields on level population’, MNRAS, 370, 1790-1796;
9.Qu,Zhong-Quan; Xu,Zhi, 2002, ‘Key Properties of Solar Chromospheric Line Formation Process’,ChJAA. 2(1), 71-80;
10.Qu,Z.Q.;Zhang,X.Y.;Chen,X.K.;Feng,Y.M.;Gu,X.M.;Zhong,S.H.,2001,‘A Solar Stokes Spectrum Telescope’, Sol.Phys.,201(2),241-251;
11.Qu,Z.Q., Zhang,X.Y .and Gu,X.M., 1999,‘On the line formation process in stellar atmospheres-I.Unpolarizedlight’, MNRAS, 305(4), 737-745;
12.Qu,Z.Q.and Ding,Y.J., 1997, ‘On the derivation of the stratification of solar vector magnetic fields by Stokes profile analysis’, MNRAS, 288(1), 53-62;