“…The prolate spheroidal coordinate system is, therefore, ideal for modeling structures which can be approximated by hyperbolic or ellipsoidal surfaces of revolution, and has often been used for field emission problems [15,[105][106][107]. Recently, Forbes and Jensen [108] applied the methodology to emission from ellipsoids retaining the notation of Morse and Feshbach; the treatment here synopsizes that account, but will use the notation of earlier treatments [52,101].…”