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These data include raw scanning Doppler lidar measurements from the deployment of the NREL Halo XR+ (s/n 235) at WFIP3's NOAA ship. The raw measurements include uncalibrated beam azimuth angles, radial velocity, backscatter, signal to noise ratio per each line of sight, and range-gate. The location of the ship is provided separately.
This dataset contains processed data from NREL's Halo XR+ #235 scanning lidar at WFIP3's NOAA ship site. The location of the ship is provided separately. The data have NOT been corrected for the motion of the ship.
These data are from a short deployment of the UC Davis Halo Streamline scanning lidar. The scanning lidar was deployed 880 m south of the NEON tower and in the same location as the field profiling lidar that was deployed later in spring 2024.
These data include raw scanning Doppler lidar measurements from the deployment of the NREL HALO XR+ (s/n 235) at the A1 site. The raw measurements include uncalibrated beam azimuth angles, radial velocity, backscatter, signal to noise ratio per each line of sight, and range-gate.
These data include raw scanning Doppler lidar measurements from the deployment of the NREL HALO XR+ (s/n 235) at the A1 site. The processed measurements include uncalibrated beam azimuth angles, radial velocity, backscatter, signal to noise ratio per each line of sight, and range-gate.
This dataset contains high-frequency vertical velocity recorded by fixed-point vertical scans done by the University of Virginia Halo Streamline scanning lidar at the MLBS station. The quality control is performed according to the algorithm of Goring & Nikora (2002).
This dataset contains high-frequency vertical velocity recorded by fixed-point vertical scans done by the Lawrence Livermore National Laboratory Halo Streamline scanning lidar at Tree Tops. The quality control is performed according to the algorithm of Goring & Nikora (2002).
This dataset contains high-frequency vertical velocity recorded by fixed-point vertical scans done by the UC Davis Halo Streamline scanning lidar. The quality control is performed according to the algorithm of Goring & Nikora (2002).
This dataset contains high-frequency wind profiles from ground-based NLR Halo XR+ 235 performing six-beam scans.
This dataset contains 10-minute wind statistics from ground-based NLR Halo XR+235 performing six-beam scans.
This dataset contains formatted lidar data from ground-based NLR Halo XR+235.
This dataset contains raw lidar data from ground-based NLR Halo XR+235.
This dataset contains raw lidar data from the ground-based NLR Halo XR+ 200.
This dataset contains raw lidar data from the ground-based NLR Halo XR+ 200.
This dataset contains raw lidar data from ground-based NLR Halo XR+ 199.
This dataset contains formatted lidar data from ground-based NLR Halo XR+ 199.
This dataset contains formatted lidar data from ground-based NLR Halo XR+ 200.
I report the discovery that the ninth-mag Galactic-halo star BD+14°3061 is a member of the rare class of luminous metal-poor “yellow post-AGB” stars. Its Gaia DR2 parallax implies an absolute magnitude of M V = -3.44 ± 0.27, and it is a very high-velocity star moving in a retrograde Galactic orbit. BD+14°3061 is a field analog of the half-dozen yellow PAGB stars known in Galactic globular clusters, which have closely similar absolute magnitudes. These objects are the visually brightest members of old stellar populations; their apparently narrow luminosity function makes them potentially useful as Population II standard candles. The spectral-energy distribution of BD+14°3061 out to 22 μm shows no evidence for circumstellar dust. The star is a low-amplitude semiregular pulsating variable, with typical periods of 30–32 days. A radial-velocity study suggests that it is a spectroscopic binary with a period of 429.6 days, making it similar to known binary yellow PAGB stars such as HD 46703 and BD+39°4926.