  We present images at 6 and 14 GHz of Source I in Orion-KL. At higher
frequencies, from 43 to 340 GHz, images of this source are dominated by thermal
emission from dust in a 100 AU diameter circumstellar disk, but at 6 and 14 GHz
the emission is elongated along the minor axis of the disk, aligned with the
SiO bipolar outflow from the central object. Gaussian fits to the 6, 14, 43,
and 99 GHz images find a component along the disk minor axis whose flux and
length vary with frequency consistent with free-free emission from an ionized
outflow. The data favor a broad outflow from a disk wind, rather than a narrow
ionized jet. Source I was undetected in higher resolution 5 GHz e-MERLIN
observations obtained in 2021. The 5-6 GHz structure of SrcI may be resolved
out by the high sidelobe structure of the e-MERLIN synthesized beam, or be time
variable.
