Exposure to a Cr-51 neutrino source as that used in Gallex win provide
an excellent overall performance test of Borexino, which should colle
ct about 1400 source induced events, with an initial rate of about 35
counts per day. This will be particularly important if MSW-small-angle
turns out to be the solution of the solar neutrino problem. In additi
on, if an independent, accurate calibration is available, one will hav
e an interesting experiment on neutrino properties: as an example, a n
eutrino magnetic moment of the order 5 . 10(-11) mu(B) could be detect
ed/excluded at the 90% C.L.