By J.A.R. Samson and D.L. Ederer (Eds.)
This quantity is for practitioners, experimentalists, and graduate scholars in utilized physics, fairly within the fields of atomic and molecular physics, who paintings with vacuum ultraviolet purposes and are short of selecting the simplest kind of sleek instrumentation. It presents first-hand wisdom of the state of the art apparatus resources and provides technical details on tips to use it, in addition to a large reference bibliography.
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G. Fastie, J. Opt. Soc. Am. 42, 647-651 (1952). 38. W. T. Welford, "Aberration theory of gratings and grating mountings," in Progress in Optics (E. ), Vol. IV, pp. 243-279. North-Holland, Amsterdam (1965). 39. H. Yoshinaga, B. Okazaki, and S. Tatsuoka, J. Opt. Soc. Am. 50, 437-445 (1060). 40. G. S. Monk, J. Opt. Soc. Am. 17, 358-364 (1928). 41. A. H. C. P. Gillieson, J. Sci. Instr. 26, 335-339 (1949). 42. T. Namioka and M. Seya, Appl. Opt. 9, 459--464 (1970). 43. T. Kaneko, T. Namioka, and M. Seya, Appl.
Taking a grating of length 150 mm and width 44 mm, Fig. 4 m. The same thing is shown in Fig. 5 except that r' has been set for focus. This also brings about consequential changes in aberrations other than defocus, including a shift of the coma zero. Note that, in both these plots, the spherical aberration and line curvature terms are scaled by 10• and 1000• respectively. The defocus curve goes through two zeroes, as expected, and the coma curve goes through one. 5). The individual aberrations are shown in their signed form, meaning that the signs are those of !
4 Calculation of Ray Aberrations In an aberrated system, the outgoing ray will arrive at the Gaussian image plane at a point BR displaced from Bo by the ray aberrations Ay' and zXz' (Fig. 1) which we would like to calculate [28]. To do so, consider a Gaussian reference sphere with center Bo and radius ~ (