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Wyoming Cloud Lidar (WCL)

 

The Wyoming Cloud Lidar (WCL) is an airborne observational system that provides high-resolution cloud and aerosol structures. There are two WCL systems available, an up-pointing lidar (zenith, WCL-I) at a wavelength of 355 nm and a down-pointing lidar (nadir, WCL-II) at 351 nm, which can be deployed separately or together. WCL is primarily used on the King Air, but has also been used on the NSF/NCAR C-130 and NPS Twin Otter.

WCL overview

WCL is used in operations where it is desired to describe weather events such as clouds, precipitation, and aerosol, and to provide specific information of these targets.

Data Products

Quicklooks and preliminary processed L0 data is made available within 24 hours during deployment. Standard processed data made available after quality control includes:

  • Level 0 product
    • Parallel and perpendicular channels return power
    • Depolarization ratio
  • Level 1 product
    • Calibrated attenuated backscattering coefficient for parallel channel
    • Lab calibrated depolarization ratio
 WCL example data

Specifications

An Ultra Pulsed Nd:YAG Laser from the Big Sky Laser Technologies Inc. providing a 20 Hz 16 mJ output at 355 nm is used for the WCL-I. Operating at 355 nm not only makes it easy to achieve eye-safe operation, it also provides a stronger molecular backscattering signal than a lidar operating at 532 or 1064 nm with the same laser energy. This is important for calibrating backscattering coefficients. The laser beam is expanded 5 times to a diameter of 15 mm before emittance into the atmosphere, making the system eye-safe beyond a distance of ~65 m. To improve lidar linear depolarization measurements, a 1/2 λ wave plate is placed after the beam expander and coupled with a cubic polarization beam splitter in the receiver path.

The receiver in the WCL-I is based on a 75mm refractive lens with a 12.5mm collimated beam that enters into the cubic polarization beam splitter. The field of view is controlled by a pinhole located at the focal plane of the receiving lens. The PMT packages include narrow band filters (0.3 nm), a focus lens, and a compact PMT. To provide the ruggedness and stability needed for the WCL to operate in a turbulent environment, the receiver is designed to share the same optical bench with the transmitter. The PMT's gain can easily be adjusted with bias control voltage. Signals from the PMTs are sent to the LICEL data acquisition system. The data system has a combined A/D and photon counting capability. To provide high-resolution spatial measurements, only strong signals digitized by A/D at 40 MHz are saved at single shot or averaging of number of shots. Thus, the WCL can provide measurements at ~4.5 m horizontal and 3.75 m vertical resolution from the UWKA, for an average cruise speed of ~90 m/s.

  Zenith (up-pointing) WCL-I Nadir (down-pointing) WCL-II
Transmit Laser Wavelength 355 nm 351 nm
Pulse Energy 16 mj 200 μj
Pulse Length 6 ns 30 ns
Pulse Repetition Frequency (PRF) 20 Hz 1 KHz
Laser Beam Divergence 1 mrad 0.3 mrad
Polarization (pol) Radiated Linear Linear
Receiver Diameter 75 mm 108 mm
Receiver Field of View 2 mrad 1 mrad
Receiving Channels 2 4
Polarization Received H&V H&V
Detector PMT PMT
Range Resolution 3.75 m and up 1.5 m and up
Temporal Resolution 0.05 s and up 0.01 s and up
Data Acquisition System LICEL GAGE

 

The area around the flight level where the laser beam enters into the field of view (FOV) of the receiving telescope progressively is the "overlap zone", which is about 100 m in length, depending on the transmitted laser beam divergence, the FOV of the receiving telescope and the angle between the axes of the laser beam and telescope. The processed data are already corrected for this by using calculated overlap factors. However the correction may not be completely accurate for all of the profiles due to the drift in the laser beam's direction.

Also, the near-range signals can saturate when the aircraft is flying through dense clouds. In this situation, the clouds cannot be fully penetrated by the lidar, and the signals can be dramatically attenuated with increasing distance.

Contact

Owen Cruikshank | ocruiksh@uwyo.edu | (307) 766-3245

Citation

University of Wyoming - Flight Center, 2007: The University of Wyoming Cloud Lidar (WCL). University of Wyoming, College of Engineering, Department of Atmospheric Science, doi:10.15786/M25W9D.

Development History

WCL-I and WCL-II were developed within the University of Wyoming's Department of Atmospheric Science. Major funding for the acquisition, development and research use of the WCL has been derived from the NSF, ONR, NASA and UW.

The zenith-pointing WCL-I was developed in 2007 and has been successfully deployed and tested on the UWKA during the Wyoming Airborne Integrated Cloud Observations Experiment (WAICO) in 2008 and 2009, and on the NSF/NCAR C-130 during the Ice Clouds Experiment-Layer Clouds (ICE-L) in 2007. Since then, it has been regularly deployed in in many projects aboard both aircraft.

The nadir-pointing WCL-II was developed in 2008 and  successfully tested during  the WAICO09 experiments.

In 2011, the WCL-II was upgraded by adding two new receiving channels which can enlarge the dynamic range of the receiving signals.