The sputtering of carbon materials by energetic particles leads mainly
to the emission of monoatomic carbon, but also to C-2 and C-2 cluster
s. Time-of-flight measurements were performed to determine the energy
distributions of C-1, C-2 and C-3 sputtered from graphite during 5 keV
Ne+ impact. All energy distributions are characterized by the Thompso
n distribution with a surface binding energy of 7.5 eV for C, 3.5 eV f
or C-2 and 0.8 eV for C-3. Using these distribution data the flux rati
os of sputtered C-2 and C-3 to sputtered C can be determined to be 0.0
6 for C-2/C and 0.03 for C-3/C by 5 keV Ar+ impact, 0.05 for C-2/C and
0.02 for C-3/C by 5 keV Ne+ impact and 0.06 for C-2/C and 0.01 for C-
3/C by 5 keV He+ impact, respectively. Thus, 11% of all sputtered carb
on is emitted as C-2 and in the case of 5 keV Ar+ impact 9% as C-3.