  We report the detection of a potential cosmic radio transient source using
the two stations of the Long Wavelength Array. The transient was detected on 18
October 2017 08:47 UTC near the celestial equator while reducing 10,240 hours
of archival all-sky images from the LWA1 and LWA-SV stations. The detected
transient at 34 MHz has a duration of 15 - 20 seconds and a flux density of 842
+/- 116 Jy at LWA1 and 830 +/- 92 Jy at LWA-SV. The transient source has not
repeated, and its nature is not well understood. The Pan-STARRS optical
telescope has detected a supernova that occurred on the edge of the position
error circle of the transient on the same day.
