Velocity Difference of Ions and Neutrals in Solar Prominences

Abstract

Marked velocity excesses of ions relative to neutrals are obtained from two time series of the neighboring emission lines He i 5015 angstrom and Fe ii 5018 angstrom in a quiescent prominence. Their Doppler shifts show time variations of quasi-periodic character where the ions are faster than the neutrals, 1.0 <= V (macro)(Fe ii)/V (macro)(He i) <= 1.35 in series A and <= 1.25 in series B. This "ratio excess" confirms our earlier findings of a 1.22 ion velocity excess, but the present study shows a restriction in space and time of typically 5 Mm and 5 minutes. The ratio excess is superposed by a time- and velocity-independent "difference excess" of -0.3 <= V (macro)(Fe ii)-V (macro)(He i) <= +0.7 km s(-1) in series A (also indicated in series B). The high repetition rate of 3.9 s enables the detection of high-frequency oscillations with several damped 22 s periods in series A. These show a ratio excess with a maximum of 1.7. We confirm the absence of a significant phase delay of He neutrals with respect to the Fe ions.