Low-cost water vapour radiometry

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Transcription:

Low-cost water vapour radiometry Prospects and progress Tinus Stander, Pr.Eng, PhD, SMIEEE Hilo, 13 June 2017

Agenda Introduction to CEFIM mm-wave group Project Context An engineer s view of WVR Current systems Development Opportunities Project Details Funding Participants Goals Progress Conclusion 2

Introduction to CEFIM

The Carl and Emily Fuchs Institute for Microelectronics Founded 1981 4 academic staff Focus Areas Si / CMOS devices & detectors MEMS devices Microwave and mm-wave devices 4

Microwave and mm-wave microelectronics Principal Investigator: T. Stander Students (full-time): 3 PhD, 6 M.Eng, 2 B.Eng IV Research Interests mm-wave communications front-ends System-on-chip front-end components (filters, oscillators, LNAs, PAs) Low-cost hybrid integration On-chip electromagnetic modelling mm-waves for CubeSat Wideband receivers for solar radiation monitoring Radiation degradation modelling and monitoring Radio Astronomy Fast Digitizers in hybrid GaAs / CMOS Analogue signal pre-processing Water vapour radiometry 5

Facilities VNA (110 GHz) 300mm probe station mm-wave anechoic chamber 50 GHz + Designed in-house 50 GHz signal analyzer Extensions 50 110 GHz Spectrum analysis, phase noise, NF, comms analysis 6

Recent Work On-chip antenna, 85 89 GHz CMOS DC radiation reference circuit SiGe LNA, 65-100 GHz CMOS Current Conveyor, L-band SiGe active enhanced filter, 83 83.5 GHz Dual notch filter, W-band 7

Project Context

One engineer s perspective of WVR Point a mm-wave antenna at the sky, measure noise power, give data to clever people. Some bands give info on water vapour, some on liquid water. Concentration vs. height extraction possible Not the client need Used for data correction in VLBI More important > 10 GHz. Used for site surveys in mm-wave radio astronomy Astronomers Me 9

How an RF engineer sees the problem Low noise receiver (Tsys < 300 K) High resolution (< 0.1K) Stable gain Excellent calibration Thermal stabilization Multiple channels (noise spectrum) 22 GHz for WV, 31 GHz for LW 183 GHz for WV in dry environments Perhaps consider later Scanning antenna Elevation, azimuth Low dwell time (< 1s) Narrow beamwidth antenna (< 5 ) Very low sidelobes 10

Commercial Systems (1) Radiometer Physics LWP basic Liquid water path + Integrated water vapour Total, not vertical profile Scanning parabola Coax, waveguide integration Discrete filters for each channel No variable downconversion Source: Radiometer Physics (www.radiometer-physics.de) 11

Commercial Systems (2) Radiometrics PR-Series Radiometers MP-Series Profilers Anticipated similar internals Source: Radiometrics Corporation (www.radiometrics.com) 12

Research Systems (1) Effelsberg (Max Planck Institute for Radio Astronomy) Modular / waveguide integration Thermal stabilization Scanning dish Sky dip Source: Roy et al, The Water Vapour Radiometer at Effelsberg, Proc. 7th European VLBI Network Symposium, 2004 13

Research Systems (2) MIAWARA University of Bern WV extraction 20 80km Horn feed Waveguide components Uncooled Single channel Source: Deuber et al, A new A New 22-GHz Radiometer for Middle Atmospheric Water Vapor Profile Measurements, IEEE Trans. GeoScience Remote Sensing, 42(5), 2004. 14

Research Systems (3) MIAWARA-C (Compact) University of Bern Horn feed Rotating mirror Waveguide, cables Pattern emerging Source: Straub et al, MIAWARA-C, a new ground based water vapor radiometer for measurement campaigns, Atmos. Meas. Tech., 3, 1 15, 2010 15

Research Systems (4) ATCA Cable and module integration Uncooled 16 26 GHz Horn feed + reflector Source: Indermuehle et al, Water Vapour Radiometers for the Australia Telescope Compact Array, PASA, v. 30, e035, 2013 16

Trends in current systems Modular WG/cable integration Mechanical motor steering Reflector + horn antennas Not cooled Sometimes temp stabilized Typ. two channels Source: Pottiaux et al, First Experiences with a Water Vapor Radiometer at the Royal Observatory of Belgium, Symp. EUREF, 2002 17

Development opportunities (1) RF PCB integration? Ku / Ka band SatCom receivers! Cost! But sensitivity? Custom components? Cooling? Temp. stabilization? How many corners can we cut?? Source: Teledyne Microwave Solutions (www.teledynemicrowave.com) Source: Leica Geosystems (http://metrology.leica-geosystems.com/) 18

Development opportunities (2) Phased array antenna? No more mechanical maintenance Beam shape? Steering? Noise? Source: ESA (www.esa.int) Conformal array? Electronic azimuth & elevation Retrieval Methods Reasonable data from low-cost receiver? Is it worthwhile? Source: CST (www.cst.com) 19

Project Details

Project Funding National Research Foundation of South Africa (NRF) Collaborative Postgraduate Training programme Emphasis on postgraduate student development 2017 2020 ±8 students p.a. 60% bursaries, 40% consumables & small equipment budget 21

Project Participants University of Pretoria mm-wave components Testing Tshwane University of Technology System design Digital & Microwave Engineering North-West University Retrieval Algorithms Site surveys Stellenbosch University Antennas Hartbeeshoek Radio Astronomy Observatory The end user! 22

Project Goals (1) Low-cost planar integrated WVR channel card Possible? Feasible? SIW? (Some) commonality across bands? Solid-state phased array antennas for WVR Conformal array? Synthesis method? Hardware? 23

Project Goals (2) Radiometric site surveying Off-the-shelf downconverters Lab blocks / equipment Until system available Total power radiometer Comparison to other survey methods New retrieval algorithm development Suited to low-cost equipment 24

Project Progress Preliminary system specs defined (SM Walker, TUT) System simulation environment established (SM Walker, TUT) System trade-off study ongoing Student Recruitment 3 B.Sc.Hons (Astronomy), NWU 1 M.Sc (Astronomy), NWU Topic: Retrieval methods 1 M.Sc.Eng (Electronic Engineering), SU Antenna array 1 M.Eng (Electronic Engineering), TUT Digital control, data capture, DSP 25

Conclusion

Conclusion We need WVRs for long-term site surveys Maybe for mm-wave VLBI Cheap, minimal maintenance RF PCB + phased array integration ideal Electronic steering ideal Full system in 3 years unlikely Train students for future development Indication of whether concept is feasible Pathfinder components 27

Tinus Stander Senior Lecturer Carl and Emily Fuchs Institute for Microelectronics Dept. EEC Engineering University of Pretoria Pretoria, 0002 South Africa +27 12 420 6704 tinus.stander@ieee.org http://www.up.ac.za/en/electronics-and-microelectronics-/article/2147601/microwave-and-mm-wave-