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secondary emission : ウィキペディア英語版
secondary emission


Secondary emission in physics is a phenomenon where primary incident particles of sufficient energy, when hitting a surface or passing through some material, induce the emission of secondary particles. The term often refers to the emission of electrons when charged particles like electrons or ions in a vacuum tube strike a metal surface; these are called secondary electrons.〔R. Kollath, Secondary electron emission of solids irradiated by electrons, Encyclopedia of Physics (ed. S. Flügge) Vol. 21, p. 232 - 303 (1956, in German)〕 In this case, the number of secondary electrons emitted per incident particle is called secondary emission yield. If the secondary particles are ions, the effect is termed secondary ion emission. Secondary electron emission is used in photomultiplier tubes and image intensifier tubes to amplify the small number of photoelectrons produced by photoemission, making the tube more sensitive. It also occurs as an undesireable side effect in electronic vacuum tubes when electrons from the cathode strike the anode, and can cause parasitic oscillation.
== Applications ==


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