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We discuss the appearance of EUV brightpoints (BPs) in the analysis oflong-duration observations in the He II 304 Angstrom passband of the Solar andHeliospheric Observatory (SOHO) Extreme-ultraviolet Imaging Telescope (EIT).The signature of the observed 304 Angstrom passband intensity fluctuationsaround the BPs suggest that the primary source of the mass and energy suppliedto the magnetic structure is facilitated by relentless magnetoconvection-drivenreconnection, forced by the magnetic evolution of the surroundingsupergranules. Further, we observe that if the magnetic conditions in thesupergranules surrounding the footpoints of the cool 304 Angstrom BPs aresufficient (large net imbalance with a magnetic field that closes beyond theboundaries of the cell it originates in) the magnetic topology comprising theBP will begin to reconnect with the overlying corona, increasing its visibilityto hotter EUV passbands and possibly Soft X-Rays.

On The Mass and Energy Loading of EUV Brightpoints