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By E. König, G. Ritter (auth.), Irwin J. Gruverman, Carl W. Seidel, David K. Dieterly (eds.)

This is the 9th quantity of a continual sequence meant to supply a discussion board for book of improve­ ments in Mossbauer impression method and in spectroscopy and its functions. Mossbauer impact technique, quantity nine, documents the complaints of the 9th Symposium on Mossbauer influence method. The symposium was once backed through the hot England Nuclear company and curiosity used to be targeting spectroscopy and functions, with greater than traditional emphasis on new technique. The symposium was once held within the Palmer residence in Chicago on February three, 1974. Dr. Stanley Hanna presided over the afternoon and night periods. Attendance used to be less than traditional; approximately 100 members have been current. this can mirror the continu­ ing strain of trip price range obstacles. Contributing Sponsors have been Austin technology affiliates, El Scint, Inc., Nuclear technological know-how tools and Ranger Electronics. those firms proven their items for Mossbauer purposes. the continued advancements within the spectrometers and their adjuncts used to be obtrusive. the choice Committee back had a so much tough activity, and was once obliged to just accept in simple terms approximately half the submitted papers. A best workforce of papers on purposes and spectroscopy featured experiences on digital leisure phenomena, magnetic part and spin changes, photochromism in strontium titanate, lattice stories, and section selection via Kossel research. the superb method consultation integrated displays on information research strategies for spectral folding, hyperfine interplay research and recoil-free fraction dimension, a backscatter spectrometer and a file on a Selective Excitation Double Mossbauer way to learn time-dependent phenomena.

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20. Price, B. , Radiation Shielding, Pergamon Press, New York (1957). SELF-ABSORPTION MOSSBAUER INVESTIGATION 51 21. Meghreblian, R. V. and Holmes, D. , New York (1960). 22. Soltesz, R. , WANL - TMI - 1967, Oak Ridge National Laboratory, CCC-82-F (April 1969). MOSSBAUER SPECTROSCOPY OF APPLICATIONS 125 Te - SOME NEW RESULTS AND P. Boolchand, * B. B. Triplett and S. S. Hanna Department of Physics Stanford University t Stanford, California 94305 and J. P. deNeufville Energy Conversion Devices, Inc.

_ f=O. 85,C(=18 - f=O. 70,~=1l Krypton ice source thickness (em) Figure 9. Ratios of Kr x-ray to Kr ~-ray intensity from transport equation predictions (solid and dashed lines) with experimental data points superimposed. 46 J. B. BROWN, JR. Curves depicting x-ray to Y-ray ratios as a function of Kr source thickness as calculated from transport-equation predictions are superimposed to depict their relationship with experimental results. 2 x 10- 2 cm thickness. Although this does not represent a wide range of source thicknesses, experiments with thinner or thicker sources pose problems.

20). 3 KeV gamma ray current as a function of source thickness, Figure 4. Transport Description The most complete manner of specifying a photon beam is to describe how many photons are going in a particular direction with a particular energy at a particular point in space. ), call it angular number flux. n. gives the number of photons at r , with energy E aboutd~, going in the direction specified by the unit vector,~ , within the element of solid angle d"'{)'" , which cross in unit time a unit differential element of area whose normal is in the direction JL • Before going to the equations that describe ¢«('~3~)' consider the two transport problems of interest to the selfabsorption problem.

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