Handbook of Ionization Spectra
CONTENT
PREFACE
 
1. PHYSICAL ASPECTS OF IONIZATION SPECTROSCOPY TECHNIQUE
1.1. The nature of ionization spectra
1.2. The role of elastic scattering in ionization spectrum formation for reflection geometry
1.3. Inelastic electron scattering
1.4. IL contour
1.5. Fine structure of ionization spectrum
1.6. Ionization losses
1.7. Opportunities of ionization spectroscopy
 
2. IONIZATION SPECTROSCOPY EQUIPMENT
2.1. Electron spectrometer
2.2. Electron gun
 
3. IL DETECTION
3.1. Detection specifics
3.2. Acceleration voltage fluctuations
3.3. Auger lines suppression
 
4. ADJUSTMENT OF SPECTROMETER'S ELECTRON OPTICS
 
5. SPECTROMETER CALIBRATION
5.1. The goal of calibration
5.2. Calibration of kinetic energy scale
5.3. Electron energy loss scale
5.4. Inspection of spectrometer’s adjustment and calibration
 
6. INTENSITY OF IONIZATION LINES
6.1. IL intensity
6.2. Primary electron energy selection
 
7. SURFACE ANALYSIS BY MEANS OF IS
7.1. Qualitative composition analysis technique
7.2. Standard samples technique
7.3. Elemental sensitivity coefficients technique
7.4. Analysis depth
7.5. Investigation of chemical bonding between the atoms
 
References
Ionisation Spectroscopy: Physical Background and Usage (Contents) On-line Library of IS spectra Info System Software and Library   About Authors

1. PHYSICAL ASPECTS OF IONIZATION SPECTROSCOPY TECHNIQUE

1.3. Inelastic electron scattering

While moving through the substance, the primary electron can take part various inelastic scattering events corresponding to excitation of surface and bulk plasmons, interband electron transitions from core to empty levels. These processes exclude the electron from the group which forms the IL. As long as elementary acts of inelastic scattering are considered to be statistically independent, the decay of IL electrons current is described by exponent: exp(-z/l), where z – traversed length, Lambda(E) - mean free path of the electron with energy E between inelastic collisions. A detailed review of Lambda(E) and corresponding references can be found in [Ref 3] and [Ref 5].

The electrons, which form the IL, cross the presurface layer twice (before and after the inelastic scattering). That’s why the length at which electron can be inealstically scattered is at least two times bigger than the thickness of this layer. Therefore, effective analysis depth effective analysis depth A in the IS technique is approximately twice smaller than Lambda. It is noteworthy that in Auger electron spectroscopy (AES) and X-ray photoelectron spectroscopy (XPS) the effective analysis depth is approximately equal Lambda [Ref 3].

The contributions of inelastic scattering mechanisms into the value of depend on energy in different ways for different substances, but in the region of E >100 eV a general tendency of Lambda(E) increase is observed. This increase is very important in IS, since changing Ep, it is possible to select the kinetic energy E of IL electrons (formula 1.1.2). This allows to adjust their mean free pass. This opens a possibilty to select such an important parameter as effective analysis depth, not an option in other techniques.


Look further: 1.4. IL contour

"Handbook of Ionization Spectra"
ISBN 966-02-1954-7
© T. Afanasieva, I. Koval,V. Lysenko, P. Mel'nik, N. Nakhodkin, M. Pyatnitsky
Ukrainian National Academy of Science, Ukrainian Ministry of Education and Science
Taras Schevchenko University, Radiophysical department
tel.: +38(044)526-05-60
e-mail: afanasieva@univ.kiev.ua