Helioseismic QBO periods show weak latitude dependence with shorter signals at low latitudes and amplitudes that increase with mode frequency, exhibiting a linear but cycle-specific relation to the main solar cycle amplitude.
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Spatio-temporal analysis of helioseismic quasi-biennial oscillations
Helioseismic QBO periods show weak latitude dependence with shorter signals at low latitudes and amplitudes that increase with mode frequency, exhibiting a linear but cycle-specific relation to the main solar cycle amplitude.