Space-borne analysis of the composition of the solar wind offers the unique
possibility of direct measurement of material originating from the sun. Fo
r development, testing, and calibration of solar wind particle instrumentat
ion, particle beams of highly charged ions for all elements from hydrogen u
p to iron are needed. Although sources for these ions have been available f
or some time, the special demands of space instrumentation made it necessar
y to build a dedicated facility. We built an electron-cyclotron-resonance i
on source operating at 2.45 GHz. The ion source is installed on a high volt
age platform allowing for postacceleration potentials of up to 100 kV. Ions
are produced from elements in gaseous and solid phase; the latter from vap
or emitted from a high temperature furnace closely attached to the ion sour
ce. (C) 2001 American Institute of Physics.