Multi-scale energy release events in the quiet Sun: a possible source for coronal heating

The coronal heating problem remains one of the most challenging questions in solar physics. The energy driving coronal heating is widely understood to be associated with convective motions below the photosphere. Recent high-resolution observations reveal that photospheric magnetic fields in the quiet Sun undergo complex and rapid evolution. These photospheric dynamics are expected to be reflected in the coronal magnetic field. Motivated by these insights, our research aims to explore the relationship between magnetic energy and coronal heating. By combining observations from Solar Orbiter and SDO with a magnetic field extrapolation technique, we estimate the magnetic free energy of multi-scale energy release events in the quiet Sun. Interestingly, our results reveal a strong correlation between the evolution of free energy and the integrated intensity of extreme ultraviolet emission at 171 Å in these events. We quantitatively assess the potential energy flux budget of these events to evaluate their contribution to coronal heating. Our study implies a link between photospheric magnetic field evolution and coronal temperature variations, paving the way for further research into similar phenomena.