In the present study, we have investigated morphology and evolution of small-scale Ha dynamic features on the quiet sun by analyzing video magnetograms and high resolution Ha images simultaneously taken for 5 hours at Big Bear Solar Observatory on April 18, 1997. From comparisons between time sequential longitudinal magnetograms and Hα images covering 150" × 150", several small-scale Hα dynamic features have been observed at a site of magnetic flux cancellation. A close relationship between such features and cancelling magnetic fluxes has been revealed temporarily and spatially. Our results support that material injection by chromospheric magnetic reconnect ion may be essential in supporting numerous small-scale Hα dynamical absorption features, being in line with recent observational studies showing that material injection by chromospheric magnetic reconnect ion is essential for the formation of solar filaments.

• SANGWOO LEE(Astronomy Program, SEES, Seoul National University)
• HONG SIK YUN(Astronomy Program, SEES, Seoul National University)
• JONGCHUL CHAE(Department of Astronomy and Space Science, Chungnam National University)
• PHILIP R. GOODE(Big Bear Solar Observatory, NJIT)