[1] Osborn J, Wilson R, Butterley T, et al. Profiling the surface layer of optical turbulence with SLODAR[J]. Monthly Notices of the Royal Astronomical Society, 2010, 406(2): 1405–1408.
Osborn J, Wilson R, Butterley T, et al. Profiling the surface layer of optical turbulence with SLODAR[J]. Monthly Notices of the Royal Astronomical Society, 2010, 406(2): 1405–1408.
[2] Rigaut F. Ground-conjugate wide field adaptive optics for the ELTs[C]//European Southern Observatory Conference & Work-shop, 2002.
Rigaut F. Ground-conjugate wide field adaptive optics for the ELTs[C]//European Southern Observatory Conference & Work-shop, 2002.
[3] Hart M, Milton N M, Baranec C, et al. A ground-layer adaptive optics system with multiple laser guide stars[J]. Nature, 2010, 466(7307): 727–729.
Hart M, Milton N M, Baranec C, et al. A ground-layer adaptive optics system with multiple laser guide stars[J]. Nature, 2010, 466(7307): 727–729.
[4] Rabien S, Angel R, Barl L, et al. ARGOS at the LBT. Binocular laser guided ground-layer adaptive optics[J]. Astronomy and Astrophysics, 2019, 621: 21.
Rabien S, Angel R, Barl L, et al. ARGOS at the LBT. Binocular laser guided ground-layer adaptive optics[J]. Astronomy and Astrophysics, 2019, 621: 21.
[9] Jia P, Osborn J, Kong L T, et al. Modelling synthetic atmospheric turbulence profiles with temporal variation using Gaussian mix-ture model[J]. Monthly Notices of the Royal Astronomical So-ciety, 2018, 480(2): 2466–2474.
Jia P, Osborn J, Kong L T, et al. Modelling synthetic atmospheric turbulence profiles with temporal variation using Gaussian mix-ture model[J]. Monthly Notices of the Royal Astronomical So-ciety, 2018, 480(2): 2466–2474.
[13] Jia P, Basden A, Osborn J. Ground-layer adaptive-optics system modelling for the Chinese large optical/infrared telescope[J]. Monthly Notices of the Royal Astronomical Society, 2018, 479(1): 829–843.
Jia P, Basden A, Osborn J. Ground-layer adaptive-optics system modelling for the Chinese large optical/infrared telescope[J]. Monthly Notices of the Royal Astronomical Society, 2018, 479(1): 829–843.
[15] Jia P, Cai D M, Wang D, et al. Simulation of atmospheric turbu-lence phase screen for large telescope and optical interferome-ter[J]. Monthly Notices of the Royal Astronomical Society, 2015, 447(4): 3467–3474.
Jia P, Cai D M, Wang D, et al. Simulation of atmospheric turbu-lence phase screen for large telescope and optical interferome-ter[J]. Monthly Notices of the Royal Astronomical Society, 2015, 447(4): 3467–3474.
[16] Osborn J, Wilson R W, Sarazin M, et al. Optical turbulence profiling with stereo-SCIDAR for VLT and ELT[J]. Monthly No-tices of the Royal Astronomical Society, 2018, 478(1): 825–834.
Osborn J, Wilson R W, Sarazin M, et al. Optical turbulence profiling with stereo-SCIDAR for VLT and ELT[J]. Monthly No-tices of the Royal Astronomical Society, 2018, 478(1): 825–834.
[17] Els S G, Schoeck M, Seguel J, et al. The Multi Aperture Scintil-lation Sensor (MASS) used in the site selection of the Thirty Meter Telescope (TMT)[J]. Proceedings of SPIE, 2008, 7012: 701222.
Els S G, Schoeck M, Seguel J, et al. The Multi Aperture Scintil-lation Sensor (MASS) used in the site selection of the Thirty Meter Telescope (TMT)[J]. Proceedings of SPIE, 2008, 7012: 701222.
[19] Hussain E A, Alrajhi Y M. Accelerated genetic algorithm solu-tions of some parametric families of stochastic differential equa-tions[J]. International Journal of Scientific & Technology Re-search, 2015, 4(1): 237–243.
Hussain E A, Alrajhi Y M. Accelerated genetic algorithm solu-tions of some parametric families of stochastic differential equa-tions[J]. International Journal of Scientific & Technology Re-search, 2015, 4(1): 237–243.