snodar (surface layer non-doppler acoustic radar) a new instrument to measure the height of the...
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Snodar(Surface layer NOn-Doppler Acoustic Radar)
A new instrument to measure the height of the Atmospheric boundary layer on the Antarctic plateau.
Colin S. [email protected]
Michael C.B. Ashley, Jon S. Lawrence, Daniel Luong-Van, John W.V. Storey
What is a SODAR?
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
S. Bradley, et al “Sodar calibration for wind energy applications,” March 2005.
Why build a new SODAR?
• We needed it…
• The single purpose of Snodar is to measure the height of the boundary layer in Antarctica to ±1m.
– Obtaining a calibrated CT2 profile is a bonus.
• Snodar was not intended to measure CV2 or wind
profiles.
– Snodar is truly monostatic and cannot measure CV2,
however it is possible to construct wind profiles.
South Pole 2001…
… Dome C 2003
…and Dome A 2008 ???Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
System overview
USB PC sound card, 96kHz 24bits.
Custom 12-bit programmable gain preamplifier.
Hardware loop back.
16bits
Class-D power amplifier.
Hardware triggered low noise solid state switch.
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Hardware
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Acoustics
Operating frequency is a function of atmospheric absorption, scattering due to turbulence and background noise.
- Background noise 1/f, but unknown at Dome A.
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
An Antisocial instrument?
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Snodar
D.M. Howard, J. Angus, “Acoustics and psychoacoustics”. 2006
Acoustics
We initially looked at a phased array with inertia-driven Piezoelectric speakers.
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Acoustics
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Acoustics
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Acoustics
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Acoustics
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Acoustics
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
SoftwareThe software is simple and runs in user space – not kernel space and does not require a real-time operating system.
- Uses POSIX threads and ALSA API.
- Hardware loop back allows software synchronization of signals and hardware relay triggering reduces timing constraints.
- On site data reduction and compression (500x reduction, 2x comp.).
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Performance - Noise
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Performance - Example data
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Calibration
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Calibrate Snodar using another instrument, but what?
Calibration
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Calibration
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Calibrate Snodar using another instrument, but what?
Direct in situ measurement of CT2 with differential
thermocouples:
CT2 = <[T(x) – T(x+r)]2> / r2/3
K <...>x2
Calibration
Differential thermocouple
•Measurement BW 0.5 Hz to 300 Hz.
•Type E thermocouples with 13ms time constant (FW05).
• r = 0.75m
• H = 5.75m
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Calibration
0 20 40 60 80 100 1200
0.2
0.4
0.6
0.8
1
1.2
Time [Seconds]
CT2 [
k2 m-2
/3]
SNODAR
Microthermal
0 0.2 0.4 0.6 0.8 1 1.20
0.2
0.4
0.6
0.8
1
1.2
SNODAR CT2 [k2 m-2/3]
Mic
roth
erm
al C
T2 [k2 m
-2/3
]
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Noise equivalent CT2
10 20 30 40 50 60 70 80 90 10010
-10
10-9
10-8
10-7
10-6
10-5
10-4
CT2
Height [m]
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
Plans for the future
Optical Turbulence Astronomy meets Meteorology, 15-18 September 2008, Sardegna (Italy)
- More calibration.- Dome A - again.- Dome C.- Possible collaboration with the British Antarctic Survey.
AcknowledgmentsWe would like to thank Elena Masciadri, Stuart Bradley, the entire Chinese PANDA traverse team.