New knowledge about sunspot transition region lines that deviate significan
tly from a Gaussian shape are presented. Attention is given to "multiple fl
ows," a line profile phenomenon in which two or more distinct velocities ar
e observed within the same spatial resolution element. We observe line prof
iles that are well represented by two Gaussian line components in the N v l
ambda 1242 and O v lambda 629 lines and introduce the notation "dual flow."
We have detected transition region oscillations in one of the line compone
nts in the dual-flow events.