The eruption of miniature Ðlaments on the quiet Sun has been analyzed from time sequences of digital Ha Ðltergrams obtained at Big Bear Solar Observatory during 1997 September 18È24. The 2 days with the best image quality were selected for this initial study. During 13 hr of time-lapse observations on these 2 days, in an e †ective 640@@ ] 480@@ area of quiet Sun close to the disk center, 88 erupting miniature Ðlaments were identiÐed. On average, these small-scale erupting Ðlaments have a

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... ed length of 19,000 km, an observed ejection speed of 13 km s~1, and a mean lifetime of 50 minutes from Ðrst appearance through eruption. The total mass and kinetic energy involved in a miniature Ðlament eruption is estimated to be 1013 g and 1025 ergs, respectively. They are distinguished from macrospicules by the same criteria that large-scale Ðlaments, before and during eruption, are distinguished from surges. Prior to eruption, one end, both ends, or the midsection of a miniature Ðlament is superposed over a polarity reversal boundary on line-of-sight magnetograms. We conclude that miniature Ðlaments are the small-scale analog to large-scale Ðlaments.