Published September 15, 2025 | Version 1.0.0
Dataset Open

CLAMPS2 Doppler Lidar Vertical Stares

  • 1. ROR icon NOAA National Severe Storms Laboratory
  • 2. Cooperative Institute for Severe and High Impact Weather Research and Operations (CIWRO)
  • 3. ROR icon University of Oklahoma
  • 4. Cooperative Institute for Severe and High Impact Weather Research and Operations

Description

These files contain 24 hour periods of data collected from the CLAMPS2 Halo Streamline XR+ Doppler lidar. While not conducting other scans, the lidar directs the beam to zenith, allowing for the measurement of vertical velocity. These data were collected during the SCALES project.

The Halo Streamline XR+ is a commercial platform. The Doppler lidar (DL) is an active remote-sensing instrument that provides range- and time-resolved measurements of radial velocity, attenuated backscatter, and signal-to-noise ratio (SNR). The principle of operation is similar to radar in that pulses of electromagnetic energy (infrared in this case) are transmitted into the atmosphere; the energy scattered back to the transceiver is collected and measured as a time-resolved signal. From the time delay between each outgoing transmitted pulse and the backscattered signal, the distance to the scatterer is inferred. The radial or line-of-sight velocity of the scatterers is determined from the Doppler frequency shift of the backscattered radiation. The DL uses a heterodyne detection technique in which the return signal is mixed with a reference laser beam (i.e., local oscillator) of known frequency. An onboard signal-processing computer then determines the Doppler frequency shift from the power spectra of the heterodyne signal. The energy content of the Doppler spectra can also be used to estimate attenuated backscatter. The DL operates in the near-infrared (IR;1.5 microns) and is sensitive to backscatter from micron-sized aerosols. Aerosols are ubiquitous in the lower troposphere and behave as ideal tracers of atmospheric winds. In contrast to radar, the DL is capable of measuring radial velocities under clear-sky conditions with very good precision – typically ~10 cm/sec (Newsom and Krishnamurthy 2020).  It is important to note that DL scans are fully user configurable, so special attention should be paid to the scan strategy applied for this dataset.

Additional information is available within the dataset as a readme file

Files

Files (6.0 GB)

Name Size Download all
md5:e2c9ce002b2126fcb8d032adf6e487a3
34.7 kB Download
md5:1193ac7dbdec3a9f17944efb5db7736a
2.0 GB Download
md5:af10073f5bbba131e7f866368bd4213e
1.7 GB Download
md5:d4c0a36204284ba0b0bbf24ac47cb775
386.5 MB Download
md5:ec6fa40908ee05802ea11309e3e664ae
386.5 MB Download
md5:adc2d2e48e00238346b900a3048e794b
386.4 MB Download
md5:b1afa2f3d1d28418422f74a732e793e9
379.2 MB Download
md5:bfcb1aec4cd703b373e384399f64dc62
366.6 MB Download
md5:88dc001ef2e5728e797cf9fce6920cb9
367.6 MB Download

Additional details

Dates

Valid
2024-09-07
Observation period begins
Valid
2024-09-14
Observation period ends
Submitted
2025-09-15
Data submitted