研究目的
To demonstrate the capabilities of using modern wide-band phased-array radio telescope technology for incoherent scatter radar measurements and to apply this technology to geoscience applications.
研究成果
KAIRA has been successfully built and is operational, demonstrating its suitability for EISCAT_3-D and other geoscience experiments. The use of radio astronomical technology has direct and effective applications to geoscience experiments, with many other possible types of new innovative experiments anticipated.
研究不足
The presence of pronounced grating sidelobes from the HBA array for imaging applications and the need for manual recovery of large data sets due to limited network bandwidth.
1:Experimental Design and Method Selection:
KAIRA uses the standard LOFAR signal processing system, including RCU boards for processing incoming signals, with switches and filters to select the required antenna input and observing frequency band.
2:Sample Selection and Data Sources:
The facility uses a dual array of omnidirectional VHF radio antennas for active and passive measurements.
3:List of Experimental Equipment and Materials:
Includes LOFAR antenna and digital signal-processing hardware, RCU boards, and HBA and LBA arrays.
4:Experimental Procedures and Operational Workflow:
The signal is split into subbands via a polyphase filter bank, with up to 244 subbands selected for beamforming.
5:Data Analysis Methods:
Data products include 1-s power averages of the spectrum from each RCU, 1-s power averages for each beamlet, and a correlation matrix.
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