[1] Yan X L, Xue Z K, Xiang Y Y et al. Fine-scale structures and material flows of quiescent filaments observed by the New Vacuum Solar Telescope[J]. Research in Astronomy and Astrophysics, 15, 1725(2015).

[2] Berger T E, Shine R A, Slater G L et al. Hinode SOT observations of solar quiescent prominence dynamics[J]. The Astrophysical Journal, 676, L89-L92(2008).

[3] Berger T E, Slater G, Hurlburt N et al. Quiescent prominence dynamics observed with the Hinode solar optical telescope. I. Turbulent upflow plumes[J]. The Astrophysical Journal, 716, 1288-1307(2010).

[4] Shen Y D, Liu Y, Liu Y D et al. Fine magnetic structure and origin of counter-streaming mass flows in a quiescent solar prominence[J]. The Astrophysical Journal, 814, L17(2015).

[5] Li D, Shen Y D, Ning Z J et al. Two kinds of dynamic behavior in a quiescent prominence observed by the NVST[J]. The Astrophysical Journal, 863, 192(2018).

[6] Ning Z, Cao W, Goode P R. Behavior of the spines in a quiescent prominence observed BYHINODE/sot[J]. The Astrophysical Journal, 707, 1124-1130(2009).

[7] Zhang Q M, Li D, Ning Z J. Simultaneous transverse and longitudinal oscillations in a quiescent prominence triggered by a coronal jet[J]. The Astrophysical Journal, 851, 47(2017).

[8] Zhang Q M, Li T, Zheng R S et al. Large-amplitude longitudinal oscillations in a solar filament[J]. The Astrophysical Journal, 842, 27(2017).

[9] Wang J C, Yan X L, Xue Z K et al. A formation mechanism for the large plumes in the prominence[J]. Astronomy & Astrophysics, 659, A76(2022).

[10] Yan X L, Xue Z K, Pan G M et al. The formation and magnetic structures of active-region filaments observed by NVST, SDO, and HINODE[J]. The Astrophysical Journal Supplement Series, 219, 17(2015).

[11] Deng K R, Huang J, Cao K. Progress of sodium beacon technology[J]. Laser & Optoelectronics Progress, 61, 1500005(2024).

[12] Jiang W H. Overview of adaptive optics development[J]. Opto-Electronic Engineering, 45, 170489(2018).

[13] Rao C H, Zhong L B, Guo Y M et al. Astronomical adaptive optics: a review[J]. PhotoniX, 5, 16(2024).

[14] Rao C H, Zhu L, Zhang L Q et al. Development of solar adaptive optics[J]. Opto-Electronic Engineering, 45, 170733(2018).

[15] Zhang L Q, Bao H, Rao X J et al. Ground-layer adaptive optics for the new vacuum solar telescope: instrument description and first results[J]. Science China Physics, 66, 269611(2023).

[16] Taylor G E, Rimmele T R, Marino J et al. An off-limb solar adaptive optics system: design and testing[J]. Proceedings of SPIE, 8862, 88620C(2013).

[17] Taylor G E, Schmidt D, Marino J et al. Performance testing of an off-limb solar adaptive optics system[J]. Solar Physics, 290, 1871-1887(2015).

[18] Schmidt D, Rimmele T R, Gorceix N. Wavefront sensing and adaptive optics for solar prominences[J]. Proceedings of SPIE, 10703, 107035W(2018).

[19] Schmidt D, Schad T A, Yurchyshyn V et al. Observations of fine coronal structures with high-order solar adaptive optics[J]. Nature Astronomy, 9, 1148-1157(2025).

[20] Xu Y, Liu C, Lan B et al. Research progress of adaptive optics in satellite-to-ground laser communication[J]. Laser & Optoelectronics Progress, 60, 0500004(2023).

[21] Ballesteros E, Collados M V, Bonet J A et al. Two-dimensional, high spatial resolution, solar spectroscopy using a correlation tracker. I. Correlation tracker description[J]. Astronomy & Astrophysics Supplement Series, 115, 353-365(1996).

[22] von der Luehe O, Widener A L, Rimmele T et al. Solar feature correlation tracker for ground-based telescopes[J]. Astronomy and Astrophysics, 224, 351-360(1989).

[23] Zhang C B, Zhong L B, Rao C H. Detection of static aberrations in imaging optical path considering residual constraints of wavefront sensor[J]. Laser & Optoelectronics Progress, 61, 1412002(2024).