  In the direct detection of the galactic dark matter, experiments using
cryogenic solid-state detectors or noble liquids play for years a very relevant
role, with increasing target mass and more and more complex detection systems.
But smaller projects, based on very sensitive, advanced detectors following new
technologies, could help in the exploration of the different proposed dark
matter scenarios too. There are experiments focused on the observation of
distinctive signatures of dark matter, like an annual modulation of the
interaction rates or the directionality of the signal; other ones are intended
to specifically investigate low mass dark matter candidates or particular
interactions. For this kind of dark matter experiments at small scale, the
physics case will be discussed and selected projects will be described,
summarizing the basics of their detection methods and presenting their present
status, recent results and prospects.
