  We report the discovery of a rare new form of long-term radio variability in
the light-curves of active galaxies (AG) --- Symmetric Achromatic Variability
(SAV) --- a pair of opposed and strongly skewed peaks in the radio flux density
observed over a broad frequency range. We propose that SAV arises through
gravitational milli-lensing when relativistically moving features in AG jets
move through gravitational lensing caustics created by $10^3-10^6 \;{\rm
M}_{\odot}$ subhalo condensates or black holes located within intervening
galaxies. The lower end of this mass range has been inaccessible with previous
gravitational lensing techniques. This new interpretation of some AG
variability can easily be tested and if it passes these tests, will enable a
new and powerful probe of cosmological matter distribution on these
intermediate mass scales, as well as provide, for the first time,
micro-arcsecond resolution of the nuclei of AG --- a factor of 30--100 greater
resolution than is possible with ground-based millimeter VLBI.
