Fine structures of a quiescent prominence are studied by analyzing high resolution H alpha filtergrams and H alpha line spectra observed at the Hida Observatory of Kyoto University. We have found two kinds of downward motions in the prominence. One of them is a movement with a constant acceleration below the solar gravity( ≃ 1 / 4 g s ) and the other with an uniform velocity( ≃ 16 K m / s ). The average life time and the size of prominence knots are estimated to be about 7 minutes and 4000Km, respectively. Spatial and brightness distribution of knots are also presented in this paper. With the analytical solutions derived from magnetostatic equilibrium in the prominence, we have examined the filamentary structure based on the Kippenhahn-Schluter model. Sag angles of the magnetic fields supporting the prominence matter are predicted from the observed density profile.

ABSTRACT
Ⅰ. INTRODUCTION
Ⅱ. OBSERVATIONS
Ⅲ. FILAMENTARY STRUCTURE
Ⅳ. DISCUSSIONS
Ⅴ. CONCLUSIONS
ACKNOWLEDGMENT
REFERENCES

• KIM KAP-SUNG(Department of Astronomy and Space Science, Kyung Hee University)