Data Quality Reports for Session: 123016 User: jean1charl Completed: 09/23/2009


TABLE OF CONTENTS

DQR IDSubjectData Streams Affected
D060621.4TWP/MPL/C2 - Missing datatwpmplC2.00, twpmplC2.a1
D080529.1TWP/MPL/C2 - Intermittent Double Pulse from lasertwpmplC2.a1


DQRID : D060621.4
Start DateStart TimeEnd DateEnd Time
12/14/2004233002/01/20052130
Subject:
TWP/MPL/C2 - Missing data
DataStreams:twpmplC2.00, twpmplC2.a1
Description:
The MPL was turned off due to a dead detector.
Measurements:twpmplC2.00:
  • null(Raw data stream - documentation not supported)

twpmplC2.a1:
  • time(time)
  • Laser Temperature(laser_temp)
  • Repetition rate, or Trigger Frequency of the laser(trigger_freq)
  • Maximum altitude retrieved from multichannel scalar card.(max_altitude)
  • Sum of raw backscatter counts per bin prior to ANY corrections.(total_counts)
  • Time in nanoseconds for each range bin of multichannel scalar card.(range_bin_time)
  • Angle of inclination with respect to horizontal(transceiver_altitude_angle)
  • Background Signal(background_signal)
  • Laser output energy per pulse(energy_monitor)
  • Number of laser shots recorded(shots_summed)
  • Angle of orientation with respect to true geographic north(transceiver_azimuth_angle)
  • Voltage level which operates the A/D card and the detector(voltage_05)
  • Amount of time laser pulse lags behind the scalar trigger(laser_scalar_sync_offset)
  • Time offset of tweaks from base_time(time_offset)
  • Voltage level which operates the thermistor(voltage_10)
  • lon(lon)
  • base time(base_time)
  • lat(lat)
  • Width of range-bins calculated from range_bin_time(range_bin_width)
  • Dummy altitude for Zeb(alt)
  • required to correct raw counts for detector deadtime prior to all other
    corrections.(deadtime_correction)
  • Amount of time the scalar lags behind the sync trigger(scalar_sync_offset)
  • Distance from leading edge of first range bin to the center of each bin .(range_bins)
  • Aerosol backscatter coefficient at 355 nm(backscatter)
  • Preliminary cloud base height(preliminary_cbh)
  • Number of laser pulses summed during measurement interval(shots_sum)
  • Array of heights for the range gates(height)
  • Detector Temperature(detector_temp)
  • Instrument Temperature(instrument_temp)
  • range(range)
  • Assumed zero-range bin number\(assumed_zero_range_bin)
  • Attenuated backscatter(detector_counts)
  • Repetition Rate, or Trigger Frequency of the laser(pulse_rep)
  • Voltage level which operates the energy monitor(voltage_15)
  • Filter Temperature(filter_temp)
  • effective range offset due to poor sync between laser firing and A/D trigger.(range_offset)
  • value represents date of last configuration change as yyyymmdd(property)
  • Amount of time the actual laser pulse lags behind the sync trigger(laser_sync_offset)


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DQRID : D080529.1
Start DateStart TimeEnd DateEnd Time
02/01/2005000011/27/20060500
Subject:
TWP/MPL/C2 - Intermittent Double Pulse from laser
DataStreams:twpmplC2.a1
Description:
When Spectra Physics discontinued support for their laser diode power supply, an 
alternative was need to extend the usefulness of the Spectra Physics laser head inside the MPLs.  
The solution was to use a Coherent laser diode. Unfortunately, the Coherent diode lasers 
do not have the exact same characteristics as the Spectra Physics diode lasers. As a 
result, the output of the Spectra Physics laser head sometimes produces a second pulse close 
in time but lower in intensity from the first main pulse. This is known as ?double pulsing?.

Not all of the Spectra Physics/Coherent combination systems produce a double pulse and the 
systems that do produce a double pulse do not always exhibit this behavior. It can be 
identified by a second peak at ~.2km. At first glance the signal in the data will resemble 
a low aerosol or cloud layer. When the double pulse is weak, the atmospheric signal will 
obscure the double pulse signal. At the ARM sites with a sunshade such as TWP and AMF, 
the double pulse can be seen when the sunshade closes during solar noon. When the sunshade 
closes, the MPL does not see atmospheric signal so the second pulse is evident. At SGP, a 
daily window cleaning is part of the routine. During this time the double pulse can be 
seen. Without a sunshade or window cleaning it is impossible to say definitively if double 
pulse is present. 

The first system to produce a double pulse was MPL s/n 008 located at TWP ? C2 Nauru in 
February 2005. The second system was MPL s/n 004 located at SGP in August 2005. The 
potential for the other systems to produce a double pulse is high. However, as of March 2006, 
the MPLs at NSA, TWP ? C1, TWP ? C3 and AMF have not recorded data with the double pulse 
artifact.  

The ARM program is in the process of replacing all the MPLs with a newer model. After the 
new MPLs are deployed the double pulse problem should not be an issue. The old systems 
will be relegated as spares. The double pulse problem will return if an old system is 
needed to replace a failed new system.
Measurements:twpmplC2.a1:
  • Attenuated backscatter(detector_counts)


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