  We report on the measurement of parasitic surface force noise on a hollow
replica of a LISA (Laser Interferometer Space Antenna for the observation of
gravitational waves) proof mass surrounded by a faithful representation of its
in flight surroundings, namely the capacitive sensor used to detect proof-mass
motion. Parasitic forces are detected through the corresponding torque exerted
on the proof mass and measured with a torsion pendulum in the frequency range
0.1 30 mHz. The sensor electrodes, electrode housing and associated readout
electronics have the same nominal design as for the flight hardware, including
4 mm gaps around the proof mass along the sensitive laser interferometry axis.
We show that the measured upper limit for surface forces would allow detection
of a number of galactic binaries signals with signal to noise ratio up to
approximately 40 for 1 year integration. We also discuss how the flight test
under development, LISA Pathfinder, will substantially improve this limit,
approaching the performance required for LISA.
