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A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

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IPSN PhD Forum April 7, 2013. A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring. Clinton J. Smith. Dept. of Electrical Engineering, Princeton University, Princeton, NJ 08544 pulse.princeton.edu. Motivation. - PowerPoint PPT Presentation
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A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring Clinton J. Smith IPSN PhD Forum April 7, 2013 Dept. of Electrical Engineering, Princeton University, Princeton, NJ 08544 pulse.princeton.edu
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Page 1: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Clinton J. Smith

IPSN PhD ForumApril 7, 2013

Dept. of Electrical Engineering, Princeton University, Princeton, NJ 08544

pulse.princeton.edu

Page 2: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• Carbon dioxide (CO2) is a major atmospheric greenhouse gas (GHG) Need to better understand the carbon cycle Quantify the exchange of CO2 between the surface of the earth and the

atmosphere

• Natural and manmade CO2 sources and sinks are both temporally and spatially varied

Natural variations in CO2 concentration range from 370 ppmv to 10,000 ppmv Global ambient CO2 concentration is ~390 ppmv

• Regulations to limit GHG emissions will lead to technology such as carbon capture and sequestration (CCS)

Requires monitoring for leak signals which are significantly smaller than the natural background CO2 variations

• Characterization of diverse CO2 sources and sinks requires many measurement sensors running continuously to accurately monitor

Motivation

2

Page 3: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Project Goal & Outline

http://www.coas.oregonstate.edu/research/po/satellite.gif

The project goal:• Develop a CO2 measurement technique consisting of a low-power

autonomous wireless sensor network with each node capable of measuring local CO2 concentration changes in a footprint area of 1 m to 100 m radius.

Outline• Existing technology cannot accurately monitor diverse CO2 sources and

sinks• Requirements for trace gas sensor networks• Overview of sensor node and network design• Field deployment and measurements• Conclusions and future directions

3

Page 4: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• Chamber measurements are used for measuring concentration at the smallest spatial scales of areas < 1 m3.

• Due to the size of the chamber measurement area, they result in geographically sparse CO2 data points.

Flow-through chamber designs can have errors of as much as ±15% In accumulation chamber designs, concentration gradients are degraded over

time as CO2 accumulates in the chamber

Chamber measurement of CO2 exchange

Accumulation chamber & TDLAS nodeLI-COR Flux Chamber

4

Page 5: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• Eddy Covariance can measure the CO2 exchange of entire ecosystem Commonly used for spatial scales on the order of 100 m to several kilometers Uses micrometeorological theory to interpret the covariance between vertical

wind velocity and a scalar CO2 concentration measurement Sample at as much as 20 Hz, which enables great temporal resolution in

monitoring for low time-duration events• Limitations with the Eddy Covariance method

Most accurate during steady environmental conditions Measurement areas with uneven terrain, diverse vegetation, or buildings cause

errors to be introduced into the measurement

Eddy Covariance measurement of CO2 exchange

5

Page 6: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Requirements for Trace Gas Sensor Networks

A trace gas sensor for networks must provide:

•Small size/portability•Low unit/capital cost

• Low maintenance and operating costs

•Robust construction•Low power consumption•High sensitivity (ppb)

• High selectivity to trace gas species

•Wireless networking capability

•Ease of mass production

6

Sensors

Base Station

Radio Range

Sensors work autonomously in the field

Page 7: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

CO2 Sensor Node Design & Specifications

7

• Tunable diode laser absorption spectroscopy (TDLAS)

• Housed within a NEMA enclosure for environmental protection “Quasi-Open Path”

• 3.5 m path Herriott multi-pass cell• 2 μm VCSEL & InGaAs photodetector• Custom electronics board

Drives instrument and communications• Powered by either Li-Ion or 12-V battery for

solar applications• Total power consumption < 1W

2x to 10x less than commercial sensors

CO2Laser Detector

Controlling Electronics

nLeII 0

Page 8: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

2 μm VCSEL & CO2 Absorption Spectrum

Source: HITRAN 2000 database 8

• Low power vertical cavity surface emitting laser (VCSEL) Consumes ~5 mW

power• VCSEL temperature tuning

range of ~5 cm-1

• Absorption coefficients in this range correspond to ~1% absorption over 3.5 m path

• Water absorption lines have limited impact on CO2 absorption lines

P=1 atm

AtmosphericConcentration,HITRAN/GEISA

nLeII 0

Page 9: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Wavelength Modulation Spectroscopy

9

• Wavelength Modulation Spectroscopy (WMS) used for greater noise filtering better sensitivity 0.1 – 0.3 ppmv CO2 concentration sensitivity achieved in 1 second

measurement (~400 ppmv ambient)• VCSEL is wavelength modulated at 10 kHz

Via current modulation 2nd harmonic peak value will be used for CO2 concentration measurement

• A lock-in amplifier is used to select and demodulate each harmonic WMS signal correlates linearly with gas concentration

Page 10: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Custom Control and Acquisition Board

10

TEC driverDirect Digital Synthesizer

MCU8MHz

Lock-In Amplifier + Front End

Modulated Current Driver

So, S., Sani, A. A., Zhong, L., Tittel, F., and Wysocki, G. 2009. Demo abstract: Laser-based trace-gas chemical sensors for distributed wireless sensor networks. In /Proceedings of the 2009 international Conference on information Processing in Sensor Networks/ (April 13 - 16, 2009). Information Processing In Sensor Networks. IEEE Computer Society, Washington, DC, 427-428

Page 11: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Wireless Communications Interface

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• Commercial Xbow TelosB wireless interface card IEEE 802.15.4/ZigBee compliant communications Running TinyOS

• Communicates with acquisition & control board via UART• Communicates with the base station PC via USB

Labview used for control and data logging

http://moodle.utc.fr/file.php/498/SupportWeb/co/Module_RCSF_35.html

Page 12: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Wireless network specifications

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• TinyOS ActiveMessage used for transmission of data Single-hop only Transmission rates as fast as 250 kbps 6 Hz transmission of sensor data packets (30 bytes each, ~1 kbps)

• MultiHopRouter, Tymo (Dynamic MANET On-demand implementation) available for multihop

Built on ActiveMessage protocol Node bandwidth is reduced due to aggregate bandwidth limit and increased

overhead

Base Station

Node 1Node 2Node 3

TDMA with data update every 15 seconds

Page 13: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Field Campaign Layout & Locations

Princeton University Engineering-Quad (E-Quad) buildingLICOR

Node 2

Node 1 Node 3

• Node 1 was deployed in the E-Quad courtyard ~0.5 m above the ground

• Node 2 was deployed to B-wing rooftop ~23.5 m above the ground.

• Node 3 was deployed at the northwest outside corner of E-Quad near the intersection of Olden St. and a service road leading to a parking lot

~1 m above the ground and ~1.5 m from the service road

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Page 14: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Solar Irradiance Calculations

• Calculations based on historical Princeton, NJ solar irradiance data

Found a 100 Ah battery with 35 W panels is needed for areas of shade (1/3 direct sunlight per day)

Corresponds to 3 sq. ft. of solar panels• Solar panel power is rated based on 1

kW/m2 irradiance• Enabled Nodes 1 and 3 to be solar

powered indefinitely• For comparison, Eddy Covariance

stations typically consume a minimum of 12 W power

Would require a minimum of 350 W solar panels

Corresponds to > 30 sq. ft. of solar panels

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Page 15: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• 30 minute averages shown• 5 minute rolling average σ is 1.6 – 3.7 ppmv (depending on the node)• TDLAS measurements compared against commercial LI-COR Non-Dispersive

Infrared (NDIR) CO2 sensor Node 2 on rooftop

• Large changes such as diurnal cycles are common to all three nodes• Node 3 is largely decoupled from Nodes 1 & 2

Street corners have increased turbulence

Field Campaign Measurements Over a Week

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Page 16: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• All sensor nodes calibrated a priori with known CO2 concentration.• Scatter plot of the LI-COR and TDLAS sensor Node 2, computed for Jan. 11• The measurements are in good agreement• A robust regression (with downweighting of outliers) between the two

measurements produces a slope of 0.9966 and an offset of 8.1 ppmv Approximately the calibration accuracy of the two instruments.

LI-COR and Node 2 Correlation

Perfect correlation

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Page 17: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• The network is able to capture some of the localized effects induced by the geometry of the landscape

• The low wind speed (< 1m/s) and ustar (<.2 m/s) indicate low turbulence and hence less mixing during this period.

• These conditions lead to a gradual build up of CO2 (from approximately 11.4 to 11.6)

• At the courtyard, aided by low ventilation, the buildup of CO2 is higher/more gradual

compared to other nodes.• Sources and sinks vary from within the E-

Quad courtyard to out on the street The sharp dip a little past 11.5 UTC is only

visible at the Courtyard and Rooftop node. The Street Corner node does not pick up this

dip.

Vignette of Jan. 11 Network Measurements

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12 AM 2:15 PM7 AM

Page 18: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• We built a solar-powered distributed wireless network for atmospheric trace gas monitoring.

Captured events on different time and spatial scales.• The sensor nodes in the network were completely autonomous .

Placed in areas such as street corners and courtyards where CO2 exchange is difficult to quantify with conventional techniques .

• The sensor nodes were shown to have similar sensitivity on the 5 minute time scale as the NDIR based eddy covariance CO2 sensors .

Enabling reasonable comparison between the two technologies. • Distributed wireless networks with many nodes could help fill in the gaps in

understanding carbon cycle sources and sinks in areas with heterogeneous landscapes.

Can complement the use of eddy covariance and measurement chambers in quantifying environmental carbon exchange.

• Implement multi-hop and explore 3G transceivers for greater geographic coverage.

Conclusion and Future Directions

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Page 19: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Acknowledgements

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AdvisorProf. Gerard Wysocki

CollaboratorsDr. Prathap Ramamurthy

Prof. Mohammed Amir KhanWen Wang

Dr. Stephen SoProf. Mark A. ZondloProf. Ellie Bou-Zeid

Page 20: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Acknowledgements

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This work was sponsored in part by:

The National Science Foundation’s MIRTHE Engineering Research Center

An NSF MRI award #0723190 for the openPHOTONS systems

An innovation award from The Keller Center for Innovation in Engineering Education

National Science Foundation Grant No. 0903661 “Nanotechnology for Clean Energy IGERT”

Page 21: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

Questions?

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Page 22: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

TDLAS CO2 Sensor 3rd Harmonic Line Locking

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• Overcome laser frequency drift from temperature and electronics instability

• Control laser temperature so that 3rd harmonic signal is near zero This corresponds to the maximum of the

2nd harmonic signal

Measure the CO2 concentration by continuously monitoring the 2nd harmonic signal value at the peak

Page 23: A Solar-powered, TDMA Distributed Wireless Network for Trace-gas Monitoring

• When the Node 3 data (near the street-corner) is examined with only 15 seconds of averaging, the influence of passing cars can be detected

• Direction of the tail-pipe and the size and model of the car correlate with the degree of the increase in CO2 concentration

Traditional internal combustion engine based cars with a tail-pipe facing the direction of the sensor cause much higher concentration spikes than hybrid vehicles (for which there is no measurable concentration change).

• Larger vehicles have a much greater impact on the local CO2 concentration.

Vignette of Street Corner

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