  We present two examples of velocity distributions for light dark matter
particles that reconcile the annual modulation signal observed by DAMA with all
other negative results from dark matter searches. They are: (1) a conventional
Maxwellian distribution for particle masses of 6 to 9 GeV; (2) a dark matter
stream coming from the general direction of Galactic rotation (not the
Sagittarius stream). Our idea is based on having a signal in Na, instead of I,
in DAMA, and can be tested in the immediate future by CDMS-II (using Si) and
CRESST-II (using O).
