Interferometric studies of the lower and upper atmosphere and near space environment

VHF Radar techniques for wind profiling the troposphere and lower stratosphere are well established [3], as are meteor detection techniques for measurement of the neutral wind in the mesosphere [1].More recently it has been shown VHF wind profiling radars are also capable of detecting satellites [2] and thus present an opportunity to use existing systems for space domain awareness.Buckland Park (BP) is a field station located approximately 40 km North of the city of Adelaide, South Australia.BP houses a 55 MHz Stratospheric Tropospheric (ST) radar, consisting of 144 Yagi antennas arranged on a 12 x 12 square grid.The BPST uses phase delays to steer its 6-degree beam vertically and 15 degrees off vertical in the cardinal directions, and utilizes the Doppler Beam Steering technique to estimate horizontal and vertical winds in the region between 500-m and 20 km [3].An adjacent meteor transmit antenna, and 5-antenna receive array configured in a Jones cross arrangement [4] share the same hardware and can estimate neutral horizontal winds from meteor detections in the mesosphere and lower thermosphere (~70 to 110 km).The shared hardware operates at 48-kW peak power.

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Publication Details

Published
2025-01-01
DOI
https://doi.org/10.46620/ursiaprasc25/ukgd7318
Primary Topic
Calibration and Measurement Techniques
Type
article
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article

Interferometric studies of the lower and upper atmosphere and near space environment

B. K. Dolman, Iain Murray Reid
Calibration and Measurement Techniques
article

Interferometric studies of the lower and upper atmosphere and near space environment

B. K. Dolman, Iain Murray Reid
article en

Abstract

VHF Radar techniques for wind profiling the troposphere and lower stratosphere are well established [3], as are meteor detection techniques for measurement of the neutral wind in the mesosphere [1].More recently it has been shown VHF wind profiling radars are also capable of detecting satellites [2] and thus present an opportunity to use existing systems for space domain awareness.Buckland Park (BP) is a field station located approximately 40 km North of the city of Adelaide, South Australia.BP houses a 55 MHz Stratospheric Tropospheric (ST) radar, consisting of 144 Yagi antennas arranged on a 12 x 12 square grid.The BPST uses phase delays to steer its 6-degree beam vertically and 15 degrees off vertical in the cardinal directions, and utilizes the Doppler Beam Steering technique to estimate horizontal and vertical winds in the region between 500-m and 20 km [3].An adjacent meteor transmit antenna, and 5-antenna receive array configured in a Jones cross arrangement [4] share the same hardware and can estimate neutral horizontal winds from meteor detections in the mesosphere and lower thermosphere (~70 to 110 km).The shared hardware operates at 48-kW peak power.

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Calibration and Measurement Techniques
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Interferometric studies of the lower and upper atmosphere and near space environment — B. K. Dolman, Iain Murray Reid · (2025) | TGRS Research Map | TGRS