The secondary electron emission coefficient γ has been measured for clean Au, Pt, Ag, Mo, Cu, Ni, Zr, Ti and C surfaces bombarded with H1+, H2+ and H3+ ions of energies between 10 and 140 keV. Measurements of γ have been made within the monolayer adsorption time (similar 5 min) after flashing the targets to a high temperature in background pressures of approximately 10-8 mmHg. The measured values of γ intrinsic to clean metal surfaces are relatively low, e.g. γ = 1.5 for 100 keV protons incident on atomically clean molybdenum. A maximum in the yield curve for protons is found to occur in the velocity range 3 × 108-4 × 108 cm sec-1. The yield for H2+ ions is found to be almost twice that for protons at the same velocity and the yield for H3+ ions is only about 17% less than that for three protons at the same velocity. For a given ion, γ is found to vary little for the metals studied although the coefficient does increase slowly with atomic number. A few measurements involving D1+ and He+ ions show that the yield for D1+ is exactly the same as that for protons at the same velocity. The yield for He+ is approximately twice that for protons. The results are discussed in relation to a theory of secondary electron emission due to Sternglass. Partial agreement is observed.
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