  We demostrate that the measurement of fluctuations of polarization due to the
galactic interstellar scintillations may be used to study the structure of the
radiation field at compact radio sources. We develop a mathematical formalism
and demonstrate it on a simple analytical model in which the scale of the
polarization variation through the source is comparable to the source size. The
predicted amplitude of modulation of the polarized radiation flux is ~20% x
(pi_s) x (m_sc), where (pi_s) is the characteristic degree of polarization of
radiation at the source and (m_sc) is the typical modulation index due to
scattering, i.e., (m_sc)~1 for diffractive scintillations and (m_sc)<1 for
refractive scintillations.
