NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Auger electron intensity variations in oxygen-charged silverAuger intensity variations over an oxygen-charged polycrystalline silver surface have been observed by studies of Auger images and line scans of selected adjacent grains which were determined to be the (421) and (221) orientations. The observed contrast (M4.5VV transition) between the grains is produced by the variation in the detected Auger electrons caused by the different directions (interatomic direction) of forward focusing in each grain. The contrast produced by the Ag Auger electrons was found to be strongly dependent on the surface order of the grains, but that of the O Auger electrons was not, presumably because the atoms were randomly distributed throughout the Ag surface or subsurface. The contrast observed between the grains at the lower Auger energies (N1VV and N1N2.3V transitions) appeared to be produced by constructive interference from multiple scattering. The N1N2.3V electrons at 29 eV, for example, gave higher contrast than that of the N1VV transition at 78 eV.
Document ID
19910061452
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Lee, W. S.
(Hampton University VA, United States)
Outlaw, R. A.
(NASA Langley Research Center Hampton, VA, United States)
Hoflund, G. B.
(Hampton Univ. VA, United States)
Davidson, M. R.
(Florida, University Gainesville, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1991
Publication Information
Publication: Applied Surface Science
Volume: 47
ISSN: 0169-4332
Subject Category
Solid-State Physics
Accession Number
91A46075
Funding Number(s)
CONTRACT_GRANT: NAG1-1110
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available