Optically changing-look active galactic nuclei (AGNs) are a class of objects that exhibit appearance or disappearance of broad lines. Recent studies have shown that these changing-look activities very likely result from the accretion activities of the central supermassive black holes. Large variation of the accretion rate might cause jet ejection and fading events, thus lead to a certain variability of observational radio properties. From the published literature, 74 changing-look AGNs and 90 changing-look AGN candidates identified in optical observations were collected. Based on this largest, complex and incomplete sample to date, the radio properties of changing-look AGNs were investigated. The radio counterparts of 51 changing-look AGNs (including 21 candidates) were discovered from the all-sky surveys conducted by the Australian Square Kilometre Array Pathfinder (ASKAP) and Very Large Array (VLA) covering the frequency range of 0.9--3GHz. This corresponds to a detection rate of about 41 percent, which is similar to general AGNs. The radio spectral indices between 0.9 and 1.4GHz, and between 1.4 and 3GHz were calculated, which suggest that these changing-look AGNs tend to have flatter radio spectra than normal AGNs. This statistical result indicates that changing-look AGNs might host some young, compact, and faint radio jets.