1. Qu, Z.Q., Dun, G.T., 2012, “Spectral line intensity irreversibility in circulatory plasma magnetization processes”,APL, 100, 2402-2405;

2. Qu, Z.Q., 2011, “A Fiber Arrayed Solar Optical Telescope (FASOT)”,ASPC, 437, 423-430;

3. 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;

4. 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’,MNRA S, 370, 1790-1796;

5. Qu, Zhong-Quan;  Xu, Zhi,  2002, ‘ Key Properties of Solar Chromospheric Line Formation Process’,CJ A A.  2(1), 71-80；

6. 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;

7. Qu, Z.Q., Zhang, X.Y. and Gu, X.M. 1999, ‘On the line formation process in stellar  atmospheres-I. Unpolarized light’,MNRAS, 305(4), 737-745;

8. 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;