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Secondary electron
yield
Factors affecting the yield, energy distribution and methods used
A talk given by
Muhammad Hassaan Saleem, Ali Raza, Adnan Ashraf, Naeemullah
What are secondary electrons
๏ƒ˜ Electrons resulting from ionization of the target material by primary
electrons.
๏ƒ˜ Their emission happens near the surface of the target material.
Secondary electron yield
Defined as
๐‘†๐‘’๐‘๐‘›๐‘‘๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘› ๐‘ฆ๐‘–๐‘’๐‘™๐‘‘ =
๐‘†๐‘’๐‘๐‘œ๐‘›๐‘‘๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘›๐‘  ๐‘’๐‘š๐‘–๐‘ก๐‘ก๐‘’๐‘‘
๐ผ๐‘›๐‘๐‘–๐‘‘๐‘’๐‘›๐‘ก ๐‘๐‘Ÿ๐‘–๐‘š๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘›๐‘ 
๏ƒ˜ Can be lesser than 1 and can be greater than 1
๏ƒ˜ If greater than 1 then it is sometimes brought to 1 by the positive charge
that is induced on the target surface.
๏ƒ˜ Depends on target material ( particularly on Z ) and primary electron energy
( i.e. accelerating voltage).
Dependence on incident energy
๏ƒ˜ Too low energies canโ€˜t ionize the atoms.
๏ƒ˜ Too high energies penetrate instead of ionizing.
๏ƒ˜ Most fruitful energies are around 100 to 500 eV (depends on target).
Secondary electron energy distribution
Typically the energy distribution of secondary electrons look like the following.
๏ƒ˜ The energy is around 30eV.
๏ƒ˜ The energy is significantly sharp for SE.
Why so sharp energy?
๏ƒ˜ The secondary electron energy is given as follows
๐‘†๐‘’๐‘๐‘œ๐‘›๐‘‘๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘› ๐‘’๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ
= ๐ผ๐‘›๐‘๐‘–๐‘‘๐‘’๐‘›๐‘ก ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘› ๐‘’๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ โˆ’ ๐ผ๐‘œ๐‘›๐‘–๐‘ ๐‘Ž๐‘ก๐‘–๐‘œ๐‘› ๐‘’๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ
๏ƒ˜ The little span in energies is because of the scattering with atoms in the
sample target.
๏ƒ˜ The span is little because secondary electrons come out near the surface.
Methods of measuring secondary electron yield
Everhart โ€“ Thornley detector
๏ƒ˜ The voltage of faraday cage is kept low so
only the SE are attracted.
๏ƒ˜ Back scattered electrons would not be
attracted (except the ones whose line of
travel takes them to the cage).
Disadvantage
Some BSE are detected, causing us to
overestimate the yield.
Methods of measuring secondary electron yield
๏ƒ˜ The contribution from BSE is
eliminated by taking two
measurements.
๏ƒ˜ Incident electron current is ๐ผ0
๏ƒ˜ A current ๐ผ+ is measured at a positive
potential (50 V)
๏ƒ˜ A current ๐ผโˆ’ is measured at negative
potential (-50 V)
* Image from โ€œMeasuring the back
scattering coefficient and secondary
electron yield in scanning microscopeโ€ by
L.Reimer and C.Tollkamp (online wiley)
Methods of measuring secondary electron yield
The secondary electron yield (๐›ฟ) is given as
๐›ฟ =
๐ผโˆ’โˆ’๐ผ+
๐ผ0
Where
๐ผโˆ’ is the current at negative bias
๐ผ+ is the current at positive bias
๐ผ0 is the incident current
Drawback
Auger electron measurement (partially)
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Secondary electron yield.pptx

  • 1. Secondary electron yield Factors affecting the yield, energy distribution and methods used A talk given by Muhammad Hassaan Saleem, Ali Raza, Adnan Ashraf, Naeemullah
  • 2. What are secondary electrons ๏ƒ˜ Electrons resulting from ionization of the target material by primary electrons. ๏ƒ˜ Their emission happens near the surface of the target material.
  • 3. Secondary electron yield Defined as ๐‘†๐‘’๐‘๐‘›๐‘‘๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘› ๐‘ฆ๐‘–๐‘’๐‘™๐‘‘ = ๐‘†๐‘’๐‘๐‘œ๐‘›๐‘‘๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘›๐‘  ๐‘’๐‘š๐‘–๐‘ก๐‘ก๐‘’๐‘‘ ๐ผ๐‘›๐‘๐‘–๐‘‘๐‘’๐‘›๐‘ก ๐‘๐‘Ÿ๐‘–๐‘š๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘›๐‘  ๏ƒ˜ Can be lesser than 1 and can be greater than 1 ๏ƒ˜ If greater than 1 then it is sometimes brought to 1 by the positive charge that is induced on the target surface. ๏ƒ˜ Depends on target material ( particularly on Z ) and primary electron energy ( i.e. accelerating voltage).
  • 4. Dependence on incident energy ๏ƒ˜ Too low energies canโ€˜t ionize the atoms. ๏ƒ˜ Too high energies penetrate instead of ionizing. ๏ƒ˜ Most fruitful energies are around 100 to 500 eV (depends on target).
  • 5. Secondary electron energy distribution Typically the energy distribution of secondary electrons look like the following. ๏ƒ˜ The energy is around 30eV. ๏ƒ˜ The energy is significantly sharp for SE.
  • 6. Why so sharp energy? ๏ƒ˜ The secondary electron energy is given as follows ๐‘†๐‘’๐‘๐‘œ๐‘›๐‘‘๐‘Ž๐‘Ÿ๐‘ฆ ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘› ๐‘’๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ = ๐ผ๐‘›๐‘๐‘–๐‘‘๐‘’๐‘›๐‘ก ๐‘’๐‘™๐‘’๐‘๐‘ก๐‘Ÿ๐‘œ๐‘› ๐‘’๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ โˆ’ ๐ผ๐‘œ๐‘›๐‘–๐‘ ๐‘Ž๐‘ก๐‘–๐‘œ๐‘› ๐‘’๐‘›๐‘’๐‘Ÿ๐‘”๐‘ฆ ๏ƒ˜ The little span in energies is because of the scattering with atoms in the sample target. ๏ƒ˜ The span is little because secondary electrons come out near the surface.
  • 7. Methods of measuring secondary electron yield Everhart โ€“ Thornley detector ๏ƒ˜ The voltage of faraday cage is kept low so only the SE are attracted. ๏ƒ˜ Back scattered electrons would not be attracted (except the ones whose line of travel takes them to the cage). Disadvantage Some BSE are detected, causing us to overestimate the yield.
  • 8. Methods of measuring secondary electron yield ๏ƒ˜ The contribution from BSE is eliminated by taking two measurements. ๏ƒ˜ Incident electron current is ๐ผ0 ๏ƒ˜ A current ๐ผ+ is measured at a positive potential (50 V) ๏ƒ˜ A current ๐ผโˆ’ is measured at negative potential (-50 V) * Image from โ€œMeasuring the back scattering coefficient and secondary electron yield in scanning microscopeโ€ by L.Reimer and C.Tollkamp (online wiley)
  • 9. Methods of measuring secondary electron yield The secondary electron yield (๐›ฟ) is given as ๐›ฟ = ๐ผโˆ’โˆ’๐ผ+ ๐ผ0 Where ๐ผโˆ’ is the current at negative bias ๐ผ+ is the current at positive bias ๐ผ0 is the incident current Drawback Auger electron measurement (partially)