“…It is argued [18] that such a system will be more efficient than standard AMS using sputter sources, especially if 14 C measurements of very small gaseous samples (CO 2 ) is of interest (see Section 2.2 below). Atmosphere Production of radionuclides by cosmic rays 14 c, 10 Be, 26 Al, 32 si, 36 cl, 39 Ar, 81 Kr, 129 10 Be, 26 Al, 41 ca, 53 Mn, 59 ni, 60 Fe Live supernova remnants in terrestrial materials 26 Al, 60 Fe, 244 Pu, ( 146 sm, 182 hf, 247 cm) stable trace isotopes in presolar grains 194,195,196,198 Pt Geochemical solar neutrino detection ( 97,98…”