Houssiau, L.
Bertrand, Patrick
[UCL]
The influence of primary ion nature and energy on ISS polar plots is studied experimentally and by simulation for scattering on a Cu(110) surface. The scattering of He and Ne ions in the energy range 1-3 keV is determined by the sampling depth of these ions. Simulations performed with the MARLOWE code show that helium ions analyse a large depth into the crystal while neon ions analyse the very first few atomic layers only.
Bibliographic reference |
Houssiau, L. ; Bertrand, Patrick. Surface-structure Analysis By Time-of-flight Iss - Influence of Primary Ion Nature and Energy for Scattering On Cu(110). In: Vacuum : surface engineering, surface instrumentation & vacuum technology, Vol. 45, no. 4, p. 409-412 (1994) |
Permanent URL |
http://hdl.handle.net/2078.1/63284 |