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Solar bright points in 3840 Å and Hα
Authors:Joan Vorpahl  Thomas Pope
Affiliation:(1) Big Bear Solar Observatory, Hale Observatories, Carnegie Institute of Washington, California Institute of Technology, U.S.A.
Abstract:Analysis of bright features in 3840 Å and Hagr shows that forevery Ellerman bomb (Hagr-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.
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