SPADE demonstrates a small, fully digital phased array spectrograph for decameter solar radio observations, with first 2024 data showing temporal and frequency resolution suitable for coronal turbulence and propagation studies.
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A neural network detector applied to 2011 solar radio spectra identified 50 QFP wave train candidates, with 13 associated with global coronal EUV waves.
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The Small Phased Array DEmonstrator (SPADE) -- Description and first results
SPADE demonstrates a small, fully digital phased array spectrograph for decameter solar radio observations, with first 2024 data showing temporal and frequency resolution suitable for coronal turbulence and propagation studies.
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Detector for fast wave trains in the solar radio emission
A neural network detector applied to 2011 solar radio spectra identified 50 QFP wave train candidates, with 13 associated with global coronal EUV waves.