Micro-Pulse Lidar Network (MPLNET): 10 Years of Trying to Imitate AERONET
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Micro-Pulse Lidar Network (MPLNET): 10 Years of Trying to Imitate AERONET. Principal Investigator: Judd Welton, NASA GSFC Code 613.1 Instrumentation & Network Management: Sebastian Stewart, SSAI GSFC Code 613.1 Data Processing & Analysis: Larry Belcher, UMBC GSFC Code 613.1

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Micro-Pulse Lidar Network (MPLNET): 10 Years of Trying to Imitate AERONET

Principal Investigator:

Judd Welton, NASA GSFC Code 613.1

Instrumentation & Network Management:

Sebastian Stewart, SSAI GSFC Code 613.1

Data Processing & Analysis:

Larry Belcher, UMBC GSFC Code 613.1

Tim Berkoff, UMBC GSFC Code 613.1

James Campbell, UCAR/Naval Research Lab

Administrative Support:

Sonia Cyrus, SSAI GSFC Code 613.1

GLAS Validation Activities:

Jim Spinhirne, formerly NASA GSFC Code 613.1

Judd Welton, Tim Berkoff

CALIPSO Validation Activities:

Judd Welton, Tim Berkoff, James Campbell

AERONET & Synergy Tool Partnership:

Brent Holben, NASA GSFC Code 614.4

Dave Giles, NASA GSFC Code 614.4

NASA SMART-COMMIT Field Deployments:

Si-Chee Tsay, NASA GSFC Code 613.2

Jack Ji, UMCP GSFC Code 613.2

Site Operations & Science Investigations

…. many network partners around the world

MPLNET is funded by the NASA Radiation Sciences

Program and the Earth Observing System

MPLNET information and results shown here are the

result of efforts by all of our network partners!


Nighttime Imitate AERONET

Morning Afternoon

Level 1 MPLNET Signals from NASA Goddard

Nighttime

Morning Afternoon

MPLNET Data Products

Micro-Pulse Lidar Network (MPLNET)

00:00

12:00

00:00

12:00

00:00

May 2, 2001

May 3, 2001

Time UTC

Asian aerosol entrained

within boundary layer

Tropospheric Aerosol from Asia

Altitude (km)

PBL Growth

PBL Decay

Stratified PBL

Well Mixed PBL

Stratified PBL

Well Mixed PBL

MPLNET Data Products:

Level 1 NRB Signals, Diagnostics

(near real time, no quality screening)

Level 1.5 Level 1.5b: Aerosol, Cloud, PBL Heights and Vertical Feature Mask

Level 1.5a: Aerosol Backscatter, Extinction, Optical Depth Profiles and Lidar Ratio

(near real time, no quality screening)

Level 2 Operational Products Under Development (beta data available upon request)

(not real time, quality assured)

All data are publicly available in netcdf format. Errors included for all data products.

Data policy same as AERONET. We are a federated network, individual site providers deserve credit.

near real time: 1 hour or 1 day


MPLNET Data Products: Cirrus Detection for AERONET AOD Evaluation

Susceptibility of Aerosol Optical Thickness Retrievals to Cirrus Contamination during the BASE-ASIA Campaign

J. Huang, N.C. Hsu, S.C. Tsay, M.-J. Jeong, B. Holben, E.J. Welton


MPLNET Processing Evaluation

Micro-Pulse Lidar Network (MPLNET)

Level 0, Raw Lidar Signal (counts/time):

Calibration “Constant”

(range only, varies w/ time)

Afterpulse

Laser – Detector Crosstalk

(unique to transceiver design)

Laser

Pulse

Energy

Overlap (up to 4 – 6 km,

Long due to transceiver design)

Dark Counts

Detector Deadtime

Level 1 Signal:

Level 1.5 and 2.0 Products:


MPLNET Level 0 Calibrations Evaluation

Deadtime provided by detector manufacturer. Considered fixed for lifetime of detector.

Laser energy and standard deviation measured in real time and stored in raw data file.

Solar background counts obtained from data between 45 – 55 km effective range, stored in raw data file.

The optical alignment of the MPL is checked (and fixed) in lab prior to deployment using our collimator (far field transmit/receive path). Ideal temperature of instrument recorded.

The following calibrations must be performed periodically and are rigorously evaluated:

Dark count (initial calibration, then monthly)

Afterpulse (initial calibration, then monthly)

Overlap (initial calibration, evaluated several times per year)

Calibration constant (generated daily from AERONET, evaluated throughout year)

Dark Count:

Lid on telescope, Laser energy off, record data for ~10 min

Afterpulse:

Lid on telescope, Laser energy at nominal setting, record data for ~10 min


MPLNET Level 0 Calibrations: Dark Count & Afterpulse Evaluation

Total Signal

Afterpulse

Darkcount


MPLNET Level 0 Calibrations: Overlap & Calibration Constant Evaluation

AERONET AOD

used to calculate

calibration constant

in molecular zone

The telescope temperature recorded during the calibration becomes the “set-point” temperature for operations.

Deviations from this value change the overlap shape.

We are testing athermal telescopes as a

solution to the temperature-overlap problem


MPLNET Level 1 Data: Operations Evaluation

MPL Maintained by on-site personnel

Must follow MPLNET specifications/protocol

Climate controlled environment, goal to achieve +- 2° C centered on set point temp

Some sites have special window wash and shutter mechanisms (maintain window quality, shade from sun in tropics at noon)

Afterpulse and darkcount calibrations performed monthly

Data transferred to NASA GSFC daily/hourly via FTP. Push or Pull.

Higher level products are retrieved daily and monitored weekly.

Q/C performed at Level 2








MPLNET Level 2 Data: Manual Assessment of Data Screens Evaluation

Data that are qualified are stored as L2, sunphotometer constrained results

The calibration values from these data are interpolated and used to generate a continuous calibration function for the assessment period. These are used to generate L2 the continuous, gridded aerosol products.






Example Comparisons from study (25 Days total). Evaluation

Also surveyed past 7 field campaigns of such work.

Summary of Study Results: MPLNET among best performers

MPLNET

MPL ARM

Neph/PSAP

AATS

The Micro Pulse Lidar Network (MPLNET): Validation

Altitude (km)

Altitude (km)

Conclusion: state-of-the-art techniques remain 15 - 20% uncertain

MPLNET meets or exceeds that target range

Extinction 1/km

AOT

Validation of MPLNET Aerosol Products: numerous MPL comparisons with AATS since 1997

How well do state-of-the-art techniques measuring the vertical profile of tropospheric aerosol extinction compare?

B. Schmid, R. Ferrare, C. Flynn, R. Elleman, D. Covert, A. Strawa, E. Welton, D. Turner, H. Jonsson, J. Redemann, J. Eilers, K. Ricci, A. G. Hallar, M. Clayton, J. Michalsky, A. Smirnov, B. Holben, and J. Barnard, J. Geophys. Res., 111, D05S07, doi:10.1029/2005JD005837, 2006.

  • Aerosol Extinction & Optical Depth profiles compared in comprehensive study:

  • MPLNET (column AOT anchored to AERONET)

  • MPL from ARM

  • Airborne Ames Sunphotometer (AATS)

  • Airborne in-situ (nephelometer & absorption photometer)

  • Airborne cavity ring-down system (Cadenza)

  • Ground-based Raman lidar (CARL)

  • AATS used as truth

  • AATS is most direct measure of AOT profile

  • AATS Column AOT within 2% of AERONET

Tim Berkoff is working on Lunar AOD capability with Cimel sunphotometer

(examine our nighttime retrievals)

Would like to initiate lidar comparisons in the

Washington DC – Baltimore region

AATS-14 shown above


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