Variation of field enhancement factor near the emitter tip

Axial symmetry Variation (astronomy) Ellipsoid
DOI: 10.1016/j.ultramic.2017.10.016 Publication Date: 2017-10-31T20:30:19Z
ABSTRACT
The field enhancement factor at the emitter tip and its variation in a close neighbourhood determines the emitter current in a Fowler-Nordheim like formulation. For an axially symmetric emitter with a smooth tip, it is shown that the variation can be accounted by a $\cos{\tilde��}$ factor in appropriately defined normalized co-ordinates. This is shown analytically for a hemi-ellipsoidal emitter and confirmed numerically for other emitter shapes with locally quadratic tips.<br/>5 pages, 6 figures<br/>
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