  We investigate to what extent correlating the Fourier components at slightly
shifted frequencies of the fluctuations of the electric field measured with a
one-dimensional antenna array on board of a satellite flying over a plane,
allows one to measure the two-dimensional brilliance temperature as function of
position in the plane. We find that the achievable spatial resolution resulting
from just two antennas is of the order of $h\chi$, with $\chi=c/(\Delta r
\omega_0)$, both in the direction of flight of the satellite and in the
direction perpendicular to it, where $\Delta r$ is the distance between the
antennas, $\omega_0$ the central frequency, $h$ the height of the satellite
over the plane, and $c$ the speed of light. Two antennas separated by a
distance of about 100m on a satellite flying with a speed of a few km/s at a
height of the order of 1000km and a central frequency of order GHz allow
therefore the imaging of the brilliance temperature on the surface of Earth
with a resolution of the order of one km. For a single point source, the
relative radiometric resolution is of order $\sqrt{\chi}$, but for a uniform
temperature field in a half plane left or right of the satellite track it is
only of order $1/\chi^{3/2}$, indicating that two antennas do not suffice for a
precise reconstruction of the temperature field. Several ideas are discussed
how the radiometric resolution could be enhanced. In particular, having $N$
antennas all separated by at least a distance of the order of the wave-length,
allows one to increase the signal-to-noise ratio by a factor of order $N$, but
requires to average over $N^2$ temperature profiles obtained from as many pairs
of antennas.
