Download Vacuum Ultraviolet Spectroscopy II by J.A.R. Samson and D.L. Ederer (Eds.) PDF
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 functions and are wanting picking the simplest form of sleek instrumentation. It presents first-hand wisdom of the state of the art apparatus assets and provides technical details on find out how to use it, in addition to a huge reference bibliography.
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Extra info for Vacuum Ultraviolet Spectroscopy II
Example text
15 [34, 35]. The system was originally designed for photoelectron emission microscopy (X-PEEM), applied to the study of magnetic materials. The materials of interest, the upper 3d transition metals (2p-3d edges) and up to the middle of the rare earths (3d-4f edges) have a relatively narrow band of energies from around 650-1300 eV. The PEEM itself requires an illuminated field of view of about 30 ~tm with maximum flux density. _. o') 0 180 . . I . . t . . I _ : . . I . . . . I . . .
I. 1 S C011 "-- - - - r Co2o - - -- Co22 -- 2 S S 1 4r 2 2r 3 Co31 - - 2 r 2 4a~o2 -- S 2 Co4o -- - ao4 cos - 8r Co42 - - ao4 cos ot ~ + 2r 2 3S 2 - 4ao22 +-- 16 r 3 3S 41-4 sin o~ C,oo = - s i n ot C1o2 -- C120 -- C122 -- S sin ot sin CIII --- 21- 2 2 ~ -- al2COSO/ 2r r al2 cos ot C131 "-- ~ r 2 + 3S sin ot 2r 3 --" 3 sin a 4r 3 2r 4 C2oo = 5 2r 3 T C2o2 3S cos ot 2r 2 T 1 Col 3 a12 c o s od s i n 2 c~ 4r 2 C211 - 2r 3 T s i n 2 c~ 2r 2 r3 T sin C300 = - a 3 0 cos ~ + C14o -- 2r 1 sin ot 2) --al4 COS ot + ~ (2ao2ai2 + a~2S cos a - ao4 sin 2 ~ ) + ~ - (4ag2 - 3S 2r 1 C22o = - a 2 2 cos ~ + ~ (4a2oao2 4r 1 S sin 2 TS - 2a12 sin 2 ~ ) + 1 2r 2 3 C222 = 2 r 2 a = cos ~ + 8 r 3 ( 3 S T - 4ao2a2o + 6a~2 sin 2 ~ ) + 4 r 4 ( T - 2S sin z ~ ) 3 sin 2 c~ r 5 1 C231 = - 7 C240 = a22 c o s o / + 1 ~( - 33S T 4 r + 4 a o 2 a 2 o - 6a12 sin 2c0 + 3S sin 2 r4 ~ a24 c o s ot 1 + ~ (a~2 sin2 c~ + 2aona2o + a22S cos ot + ao4 T c o s o t 2r + 1 2 (-4a~2 T- al4 sin 2c~ + 2ao2a22) 8ao2a2oS + 12a12S sin 2or + 3TS 2 + 16a02ai2 sin ot 16r sin 2 o~ -- 8ao4 sin 2 ~ ) + 4r 3 2) (2a22 -- 3S continues GRATING THEORY TABLE I.
The GRATING THEORY 23 need is for systems that are dedicated full time to analytical measurements, functioning rather like a standard instrument operating with a laboratory radiation source. This means that the performance, cost, and sample throughput capability must be assessed by comparison to commercial instruments. In the examples discussed later, we describe an SGM undulator beamline and two "application-specific" bending magnet beamlines for micro-XPS and X-PEEM. We first describe aberration theory of grazing-incidence mirrors and gratings and apply this in detail to the design of an ALS undulator beamline for ultra-high-resolution spectroscopy.