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Analysis of Optical Turbulence over the South China Sea Using Balloon-Borne Microthermal Data and ERA5 Data
Using Improved XGBoost Algorithm to Obtain Modified Atmospheric Refractive Index
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Seeing Measurements with the Merak H$\upalpha$ Telescope
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P. G. Kovadlo, A. Yu. Shikhovtsev, E. A. Kopylov, A. V. Kiselev and I. V. Russkikh Russian Physics Journal 63(11) 1952 (2021) https://doi.org/10.1007/s11182-021-02256-y
Near ground horizontal high resolution Cn2 profiling from Shack–Hartmann slopeand scintillation data
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Daytime optical turbulence profiling with a profiler of the differential solar limb
Characterizing daytime wind profiles with the wide-field Shack–Hartmann wavefront sensor
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Measurement of Astronomical Seeing Using Long Exposure Solar Images
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MISOLFA: a generalized monitor for daytime spatio-temporal turbulence characterization
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Daylight operation of a sodium laser guide star for adaptive optics wavefront sensing
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CRISPRED: A data pipeline for the CRISP imaging spectropolarimeter
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Profiles of the daytime atmospheric turbulence above Big Bear solar observatory
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