Solar bright points in 3840 Å and Hα

Analysis of bright features in 3840 Å and H shows that forevery Ellerman bomb (H-0.9 Å) there is a cospatial brightening in the 3840 Å network. We give properties of these bright points in both wavelengths as well as describe: (1) the appearance, and subsequent separation, of new elements in the 3840 Å network and (2) the direct transition from a 3840 Å bright point to a new sunspot.