  The paper contains the result description of the photometric observations of
the Moon surface during the total lunar eclipse of June, 15, 2011 conducted in
southern Russia and Ukraine in three narrow spectral bands with effective
wavelengths equal to 503, 677, and 867 nm. The photometric maps of umbra are
built, the radial dependencies of relative brightness are compared with the
theoretical ones for gaseous atmosphere. Dark anomalies of umbra are shown and
related with the aerosol air pollution of the definite regions above the
surface of Earth.
