  We study the possibility of using correlations between spatial modulations in
the observed luminosity distribution of galaxies and the underlying density
field as a cosmological probe. Considering redshift ranges, where magnification
effects due to gravitational lensing may be neglected, we argue that the dipole
part of such luminosity-density correlations traces the corresponding
velocity-density signal which may thus be measured from a given galaxy redshift
catalogue. Assuming an SDSS-like survey with mean density $\overline{n}$ = 0.01
($h^{-1}$ Mpc)$^{-3}$ and effective volume $V_{\rm eff}$ = 0.2 ($h^{-1}$
Gpc)$^{3}$ at a fiducial redshift z = 0.1, we estimate that the
velocity-density correlation function can be constrained with high
signal-to-noise ratio $\gtrsim$ 10 on scales 10-100 Mpc. Similar conclusions
apply to the monopole which is sensitive to the environmental dependence of
galaxy luminosities and relevant to models of galaxy formation.
