  We discuss the appearance of EUV brightpoints (BPs) in the analysis of
long-duration observations in the He II 304 Angstrom passband of the Solar and
Heliospheric Observatory (SOHO) Extreme-ultraviolet Imaging Telescope (EIT).
The signature of the observed 304 Angstrom passband intensity fluctuations
around the BPs suggest that the primary source of the mass and energy supplied
to the magnetic structure is facilitated by relentless magnetoconvection-driven
reconnection, forced by the magnetic evolution of the surrounding
supergranules. Further, we observe that if the magnetic conditions in the
supergranules surrounding the footpoints of the cool 304 Angstrom BPs are
sufficient (large net imbalance with a magnetic field that closes beyond the
boundaries of the cell it originates in) the magnetic topology comprising the
BP will begin to reconnect with the overlying corona, increasing its visibility
to hotter EUV passbands and possibly Soft X-Rays.
