MOLYBDENUM, RHODIUM, AND TUNGSTEN ANODE SPECTRAL MODELS USING INTERPOLATING POLYNOMIALS WITH APPLICATION TO MAMMOGRAPHY

Citation
Jm. Boone et al., MOLYBDENUM, RHODIUM, AND TUNGSTEN ANODE SPECTRAL MODELS USING INTERPOLATING POLYNOMIALS WITH APPLICATION TO MAMMOGRAPHY, Medical physics, 24(12), 1997, pp. 1863-1874
Citations number
25
Journal title
ISSN journal
00942405
Volume
24
Issue
12
Year of publication
1997
Pages
1863 - 1874
Database
ISI
SICI code
0094-2405(1997)24:12<1863:MRATAS>2.0.ZU;2-X
Abstract
Computer simulation is a convenient and frequently used tool in the st udy of x-ray mammography, for the design of novel detector systems, th e evaluation of dose deposition, x-ray technique optimization, and oth er applications. An important component in the simulation process is t he accurate computer-generation of x-ray spectra. A computer model for the generation of x-ray spectra in the mammographic energy range from 18 kV to 40 kV has been developed. The proposed model requires no ass umptions concerning the physics of x-ray production in an x-ray tube, but rather makes use of x-ray spectra recently measured experimentally in the laboratories of the Center for Devices and Radiological Health . Using x-ray spectra measured for molybdenum, rhodium, and tungsten a node x-ray tubes at 13 different kV's (18, 20, 22,...,42 kV), a spectr al model using interpolating polynomials was developed. At each energy in the spectrum, the x-ray photon fluence was fit using 2, 3, or 4 te rm (depending on the energy) polynomials as a function of the applied tube voltage (kV). Using the polynomial fit coefficients determined at each 0.5 keV interval in the x-ray spectrum, accurate x-ray spectra c an be generated for any arbitrary kV between 18 and 40 kV. Each anode material (Mo, Rh, W) uses a different set of polynomial coefficients. The molybdenum anode spectral model using interpolating polynomials is given the acronym MASMIP, and the rhodium and tungsten spectral model s are called RASMIP and TASMIP, respectively. It is shown that the mea n differences in photon fluence calculated over the energy channels an d over the kV range from 20 to 40 kV were -0.073% (sigma= 1.58%) for M ASMIP, -0.145% (sigma= 1.263%) for RASMIP, and 0.611% (sigma= 2.07%) f or TASMIP. The polynomial coefficients for all three models are given in an Appendix. A short C subroutine which uses the polynomial coeffic ients and generates x-ray spectra based on the proposed model is avail able on the World Wide Web at http://www.aip.org/epaps/epaps.html. (C) 1997 American Association of Physicists in Medicine.