Ion Temperatures as Observed in A Solar Coronal Hole

摘要

From the widths of the extreme ultraviolet (EUV) lines measured by the SUMER instrument on SOHO, it was found previously (Tu et al. 1998) that average temperature of Ne~(+7), at heights (relative to h_0) above the southern solar limb from 17" to 64", ranges between 1.3 and 5 X 10~6 K and of Ne~(+6) between 1 and 4 X 10~6 K. For mass-per-charge numbers greater than 4 the temperatures of the ions increase slightly with increasing mass-per-charge, while the thermal speed reveals no clear trend. We present a new data set with exposure times much longer than the ones in the previous study. The results obtained from line width analysis of Fe XII (1242 A), Mg X (1249 A), Mg VIII (772 A) Ne VIII (770 A), and Hi VIII (1445 A) support our previous study. In this case, the trend of increasing temperature begins at a mass-per-charge number of 3. A qualitative explanation based on ion-cyclotron-resonance heating within linear kinetic theory is suggested.