  The exploration of the parameter space of axion and axion-like particle dark
matter is a major aim of the future program of astroparticle physics
investigations. In this context, we present a possible strategy that focuses on
detecting radio emissions arising from the conversion of dark matter axions in
the Sun's magnetic field, including conversion in sunspots. We demonstrate that
near-future low-frequency radio telescopes, such as the SKA Low, may access
regions of unexplored parameter space for masses $m_a\lesssim 10^{-6}$ eV.
