  The influence of intergalactic magnetic fields on the strong gravitational
lensing of blazar secondary gamma radiation is discussed. Currently, two cases
of strong gravitational lensing of blazar gamma-radiation are known, where
radiation is deflected by galaxies on the line of sight between the blazars and
the Earth. The magnetic field can affect the movements of electron-positron
pairs generated by primary radiation, and thereby change the directions of
secondary gamma radiation. It modifies the equation of the gravitational lens
and leads to the dependence of the observed signal in the secondary gamma
radiation on the energy of photons and on the magnetic field. Accordingly, it
is possible in principle to estimate the intergalactic magnetic fields from the
time delay of signals, from the angular position of images (for future
high-resolution gamma-ray telescopes) or from the shape of the observed energy
spectrum. This method is demonstrated by the example of the blazar B0218+357.
In this case however it is not possible to obtain useful constraints due to the
large distances to the blazar and the lens galaxy. The result is only a lower
limit on the magnetic field $B>2\times10^{-17}$G, which is weaker than other
existing constraints. But the future discoveries of lensed blazars may provide
more favourable opportunities for measuring the magnetic fields, especially
with the help of new generation of gamma-ray telescopes such as e-ASTROGAM,
GECAM, and SVOM as well as future gamma-ray telescopes with high angular
resolution, ~0.1''.
