In this study, turbulence activity is measured from 100 to 105 km altitude using a sodium (Na) resonance-fluorescence lidar system. Previous approaches have been limited to altitudes below 100 km due to sparse Na layer density above 97 km. Using the lidar system at the Andes Lidar Observatory in Cerro Pachón, Chile (30.3ºS, 70.7ºW), a novel reconstruction algorithm measuring turbulence fluctuation power at smaller signal-to-noise ratios (SNRs) than existing methods is derived and validated. Results are compared against instability, Na mixing ratio, and total constituent diffusion coefficient measurements. Twenty-seven (27) nights of lidar data spanning 2500 hours in the zenith and 2375 hours in the off-zenith directions at 25 m, 6 s resol...
The Aerospace Corporation\u27s Nightglow Imager (ANI) observes nighttime OH emission (near 1.6 μm) e...
The performance of adaptive optics (AO) systems are highly dependent upon optical turbulence. Thus, ...
The Aerospace Corporation\u27s Nightglow Imager (ANI) observes nighttime OH emission (near 1.6 µm) e...
Turbulence is ubiquitous in the mesopause region, where the atmospheric stability is low and wave br...
Atmospheric turbulence activity in the mesosphere and lower thermosphere (MLT) region is determined ...
Modern astronomical instrumentation employs adaptive optics (AO) systems that correct for atmospheri...
Results of 3-month continuous monitoring of turbulence profile and seeing at Cerro Tololo (Chile) in...
Vertical transport by turbulent mixing plays a fundamental role in establishing the thermal and cons...
Based on explicit, experimentally proven formulae, an ameliorated lidar scheme for turbulence retrie...
The International Society for Atmospheric Research using Remotely-piloted Aircraft (ISARRA) hosted a...
International audienceThe motion field of the upper atmosphere was studied with the aid of sodium tr...
The first statistical results of simulations of optical turbulence over Cerro Paranal by an atmosphe...
The Atmospheric Turbulence and Diffusion Laboratory at Oak Ridge, Tennessee has been conducting rout...
To investigate the low-atmosphere turbulence at the South Pole, we have measured, using a SODAR, th...
To investigate the low-atmosphere turbulence at the South Pole, we have measured, using a SODAR, the...
The Aerospace Corporation\u27s Nightglow Imager (ANI) observes nighttime OH emission (near 1.6 μm) e...
The performance of adaptive optics (AO) systems are highly dependent upon optical turbulence. Thus, ...
The Aerospace Corporation\u27s Nightglow Imager (ANI) observes nighttime OH emission (near 1.6 µm) e...
Turbulence is ubiquitous in the mesopause region, where the atmospheric stability is low and wave br...
Atmospheric turbulence activity in the mesosphere and lower thermosphere (MLT) region is determined ...
Modern astronomical instrumentation employs adaptive optics (AO) systems that correct for atmospheri...
Results of 3-month continuous monitoring of turbulence profile and seeing at Cerro Tololo (Chile) in...
Vertical transport by turbulent mixing plays a fundamental role in establishing the thermal and cons...
Based on explicit, experimentally proven formulae, an ameliorated lidar scheme for turbulence retrie...
The International Society for Atmospheric Research using Remotely-piloted Aircraft (ISARRA) hosted a...
International audienceThe motion field of the upper atmosphere was studied with the aid of sodium tr...
The first statistical results of simulations of optical turbulence over Cerro Paranal by an atmosphe...
The Atmospheric Turbulence and Diffusion Laboratory at Oak Ridge, Tennessee has been conducting rout...
To investigate the low-atmosphere turbulence at the South Pole, we have measured, using a SODAR, th...
To investigate the low-atmosphere turbulence at the South Pole, we have measured, using a SODAR, the...
The Aerospace Corporation\u27s Nightglow Imager (ANI) observes nighttime OH emission (near 1.6 μm) e...
The performance of adaptive optics (AO) systems are highly dependent upon optical turbulence. Thus, ...
The Aerospace Corporation\u27s Nightglow Imager (ANI) observes nighttime OH emission (near 1.6 µm) e...