Surface structure analysis by time-of-flight ISS: influence of primary ion nature and energy for scattering on Cu(110)

L. Houssiau; Patrick Bertrand

Surface structure analysis by time-of-flight ISS: influence of primary ion nature and energy for scattering on Cu(110)

L. Houssiau, Patrick Bertrand

Namur Research Institute for Life Sciences

Résultats de recherche: Contribution à un journal/une revue › Article › Revue par des pairs

Résumé

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.

langue originale	Anglais
Pages (de - à)	409-412
Nombre de pages	4
journal	Vacuum
Volume	45
Numéro de publication	4
Etat de la publication	Publié - 1 avr. 1994

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@article{cba14502e727412bb92ce78f0a43ebfd,

title = "Surface structure analysis by time-of-flight ISS: influence of primary ion nature and energy for scattering on Cu(110)",

abstract = "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.",

author = "L. Houssiau and Patrick Bertrand",

year = "1994",

month = apr,

day = "1",

language = "English",

volume = "45",

pages = "409--412",

journal = "Vacuum",

issn = "0042-207X",

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number = "4",

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T1 - Surface structure analysis by time-of-flight ISS

T2 - influence of primary ion nature and energy for scattering on Cu(110)

AU - Houssiau, L.

AU - Bertrand, Patrick

PY - 1994/4/1

Y1 - 1994/4/1

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=0028419304&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:0028419304

SN - 0042-207X

VL - 45

SP - 409

EP - 412

JO - Vacuum

JF - Vacuum

IS - 4

ER -

Surface structure analysis by time-of-flight ISS: influence of primary ion nature and energy for scattering on Cu(110)

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