Determining the incident electron fluence for Monte Carlo-based photon treatment planning using a standard measured data set Paul J. Keall,a) Jeffrey V. Siebers, Bruce Libby, and Radhe Mohan Department of Radiation Oncology, Virginia Commonwealth University, P.O. Box 980058, Richmond, Virginia 23298 !Received 5 September 2002; accepted for publication 28 January 2003; published 25 March 2003" An accurate dose calculation in phantom and patient geometries requires an accurate description of the radiation source. Errors in the radiation source description are propagated through the dose calculation. With the emergence of linear accelerators whose dosimetric characteristics are similar to within measurement uncertainty, the same radiation source description can be used as the input to dose calculation for treatment planning at many institutions with the same linear accelerator model. Our goal in the current research was to determine the initial electron fluence above the linear accelerator target for such an accelerator to allow a dose calculation in water to within 1% or 1 mm of the measured data supplied by the manufacturer. The method used for both the radiation source description and the patient transport was Monte Carlo. The linac geometry was input into the Monte Carlo code using the accelerator’s manufacturer’s specifications. Assumptions about the initial electron source above the target were made based on previous studies. The free parameters derived for the calculations were the mean energy and radial Gaussian width of the initial electron fluence and the target density. A combination of the free parameters yielded an initial electron fluence that, when transported through the linear accelerator and into the phantom, allowed a dose-calculation agreement to the experimental ion chamber data to within the specified criteria at both 6 and 18 MV nominal beam energies, except near the surface, particularly for the 18 MV beam. To save time during Monte Carlo treatment planning, the initial electron fluence was transported through part of the treatment head to a plane between the monitor chambers and the jaws and saved as phase-space files. These files are used for clinical Monte Carlo-based treatment planning and are freely available from the authors. © 2003 American Association of Physicists in Medicine. #DOI: 10.1118/1.1561623$ Key words: Monte Carlo, initial electron fluence, beam modeling I. INTRODUCTION Rigorous Monte Carlo treatment planning will transport particles from the entrance of the accelerator target until they and their progeny are absorbed in or exit the patient geometry or the patient. To obtain accurate dose calculation in the patient, the characteristics of the electron beam above the target need to be accurately modeled and the particles accurately transported through the beam-generating and beammodifying devices. Errors in determining the electron fluence incident on the target will directly cause a systematic error in every dose calculation, whether the dose calculation uses a phase-space file, or a source model based on the phase-space file. !The term phase-space file, as used here, means a list of particles specified at a plane with records describing the charge, energy, position and direction of each particle." For treatment planning, the ICRU1,2 reports suggest that the maximum error in dose calculation should be 2% of the absolute dose !or within 2 mm of the absolute dose in highdose gradient regions". This 2% error needs to be shared among many uncertainties, such as the radiation source determination !the subject of this article", the dosimetric effects of the CT number to density conversion and the accuracy of transport in the heterogeneous patient. Further Monte Carlospecific potential sources of error are energy cut-offs, 574 Med. Phys. 30 „4…, April 2003 density-to-material conversion, dose-to-material to dose-towater conversion, etc. Thus, in order to calculate dose to the patient to within 2% or 2 mm we estimate that the source modeling error should be within 1% or 1 mm. This value is below the estimated 1.5% uncertainty of absolute dosimetry protocols.3 The accurate characterization of linear acceleratorproduced radiation is becoming more appropriate now, due to the dosimetric similarity of modern machines produced by the same vendor with beam parameters with observed variations (between linear accelerators of the same vendor) being approximately equivalent to the precision of measurement.4 Indeed, one linear accelerator vendor is offering a CD containing a ‘‘standard’’ set of beam data for one type of linear accelerator. The data set contains depth-dose curves and dose profiles for a variety of field sizes including open field and wedged fields. This beam data was used as the measurement set for which the source modeling results were compared. Thus, one single source description can be used for dose calculation by many centers. Over the years, much effort has been devoted to Monte Carlo modeling of linear accelerators.5–34 Arguably, the most comprehensive studies have been performed by SheikhBagheri and Rogers,28,29 who have studied the sensitivity of photon beam simulations to the initial electron fluence pa- 0094-2405Õ2003Õ30„4…Õ574Õ9Õ$20.00 © 2003 Am. Assoc. Phys. Med. 574 575 Keall et al.: Determining the incident electron fluence rameters and characterized the phase space from nine megavoltage beams. They have concluded that the two most important parameters for simulating photon radiotherapy beams are the mean energy and the radial spread of the incident electron beam; these parameters comprise two of the three parameters being studied in this work !the other being target density". The niche of the current research is that unlike previous work, the beam modeling is for a standard data set and thus is widely applicable to the radiotherapy community. Our aims in this work were to !1" determine the electron fluence above the target that, when transported through the treatment head and used for dosimetric calculations, can reproduce a standard dosimetric measured data set in water to within 1% or 1 mm; !2" use this electron fluence to transport particles through the target, flattening filter, etc., and, up to the first treatment dependent component, i.e., the movable jaws, to create a patient independent phase-space file for use in Monte Carlo treatment planning; and !3" make this phasespace file available for use by other researchers. II. METHOD AND MATERIALS A. Accelerator The accelerator treatment head modeled here was that of type Varian Clinac 21EX !Varian Oncology Systems, Palo Alto, CA 94304 USA". This accelerator has a standing waveguide and a 270° bending magnet. Both photon modalities !6 and 18 MV" were investigated. B. Measured data Varian provides a measured data set for the 21EX !Varian Oncology Systems, Clinac EX Precommissioning Data Package". This data set contains depth-dose and lateral profile curves for a variety of field sizes and wedge angles. Measured data for our 21EX showed no significant difference to the Varian data set. For generality, we used the Varian data set, rather than our own measurements, as the calculation benchmark, so that the phase space developed in this work could be applicable to all accelerators of this type. The Varian measurements were performed in a 48 !48!48 cm3 water tank using a Wellhöfer IC15 ionization chamber !Scanditronix Wellhöfer, Bartlett, TN 38133". The SSD was 100 cm. Due to water tank size constraints, the largest beam with its central axis aligned with the tank center was 25!25 cm2 . C. Initial electron fluence assumptions The initial distribution of electrons, %!E,x,y,&,'", just above the target !known z-position" is a 5-dimensional function, which can be described by the variables E, the kinetic energy; x and y, the lateral positions !z is fixed"; &, the polar angle; and ', the azimuthal angle. To determine the electron distribution, four assumptions were made. These assumptions and their justifications are explained below. Medical Physics, Vol. 30, No. 4, April 2003 575 1.The x and y spatial distributions are Gaussian Karzmark et al.35 in their discussion of electron beam optics of magnet systems showed that the current density of the electron beam above the target is centrally peaked with tails distributed approximately normally on either side of the peak. Also, a Gaussian-shaped distribution can be observed in the results of Jaffray et al.,36 who measured the distribution of the bremsstrahlung focal radiation. The distribution of the bremsstrahlung focal radiation is a convolution of the initial electron distribution and the spread of the electrons before the bremsstrahlung events. Our Monte Carlo calculations for a monodirectional electron point source upon the target have determined that the full width half maximum !FWHM" of the spread of the electrons before the bremsstrahlung events is (5 )m at 6 MV and (20 )m at 18 MV. Because the spread of the electrons is small in comparison with the spot size !order of mm", we can conclude that the initial electron distribution is approximately equal to the bremsstrahlung radiation distribution. Thus, we can limit our allowable initial electron distributions to the limits measured by Jaffray et al.,36 i.e., 1.2 to 1.4 mm FWHM at 6 MV and 0.9 to 1.6 mm FWHM at 18 MV. Note that the values of Jaffray et al. measured from a 2100C and the 21EX are modeled here. However, due to similar accelerator and bending magnet structure design, the 2100C and 21EX initial electron distributions are expected to be similar. 2. The x and y spatial distributions are equal The measured data set contained only cross-plane !x" dose-profile curves. Thus, in the absence of more information here, we assumed that the x and y spatial distributions are equal. The results of Jaffray et al.37 indicate a reasonable degree of symmetry for the Varian 2100 linear accelerators, especially at low energy. Using this assumption, the x and y reduce to a single variable, r" !x 2 #y 2 , which determines the spatial distribution in the radial direction. 3. The electrons are monodirectional Karzmark et al.35 have provided the typical beam transport acceptance values for the initial electron angle as 1–5 mradian !0.06 –0.3 degrees". This angle is very close to 0 !cos 5 mradian"1.0000". Hence, we assume monodirectionality. 4. The spread of the electrons about the mean energy is Gaussian and has a FWHM of 3% Using a magnetic spectrometer, Tanabe and Hamm38 measured the electron spectrum from the accelerating waveguide for a Varian Clinac 1800 to have a FWHM of about 3% for both the 6 and 18 MV modes. It was assumed that the linear accelerator modeled here had a similar energy spread. This value may change with waveguide type and also between accelerators with bending magnets and those ‘‘in-line.’’ Using the assumptions above, the initial 5-dimensional electron fluence, %(E,x,y, & , ' ), is reduced to two dimensions, %„E ,G(r)…, where E is the mean electron energy Keall et al.: Determining the incident electron fluence 576 above the target, and G(r) is the initial electron radial Gaussian width, which can be characterized by FWHMrad. However, there is also variation in the density of the tungsten alloy used for the target !$ 0.5 g cm%3 ) given by the manufacturer. Thus, the third unknown to be determined is the target density, * target . The density and composition of the target backing and flattening filter are machined to tighter specifications than the target. We assume that all beam-collimating devices have been machined according to the engineering diagrams. ues for the target and backing were determined by plotting the energy of the parent particles against the last interaction point for the particle !zlast". An insignificant number of particles that contributed to the phase space were created from parent particles below the above-stated cut-offs. Thus, we felt it justified to set ECUT and PCUT to these new values. The reason for the cut-off value differences for the target and the backing between modalities !apart from the obvious energy difference" was the different target/backing thickness ratio. The increased energy cut-off reduced the calculation time for the creation of the patient independent phase space by approximately 40% for both energies. 576 D. Calculation details The EGS439 usercode BEAM20 !BEAM 97" was used for the beam-line particle transport. The geometry was input to BEAM from proprietary diagrams supplied by Varian for the Clinac 21EX. The entered geometry was checked visually for gross errors using the BEAM gui package and validated using the method of Libby et al.12 The EGS4 results were also validated using an independent Monte Carlo code,13 MCNP.40 BEAM was adapted to allow a Gaussian radial source and energy spread. Particles were transported through the x-ray target, flattening filter, and ionization chamber to obtain a phase space stored between the monitor chambers and the jaws. This phase space was then used as input to a second calculation that transported the particles through the air gap and jaws. Particles were then transported in a water phantom using the Cartesian geometry usercode DOSXYZ,41 and the dose deposition was tallied. As with the measurements, the water phantom used for the calculations was 48!48!48 cm3 . The field size chosen for the calculations to determine the electron fluence was 25!25 cm2 , the largest field for which the measured field central axis was aligned with the tank center. A large field was chosen because, in our !and others’" experience, matching calculations with measured data is more difficult for large fields than small fields. The SSD was 100 cm, and the voxel size was 2!2!2 cm3 . The voxel size was chosen such that the dose distribution did not change significantly over the voxel within the dose volume analyzed. For all calculations, the statistical uncertainties for the calculations were less than 2% of the D max dose. The statistical uncertainty used allowed the calculation of the depth dose and dose profile curves slopes !see Sec. II F" with a standard error of the slope significantly smaller than the acceptance criteria. The discrete threshold energies for electron and photon creation, AE and AP, were set to 0.70 MeV and 0.010 MeV, respectively. The electron and photon transport thresholds ECUT and PCUT were also set to 0.70 MeV and 0.010 MeV, respectively, except in the target where the values were increased to 1.5 MeV and 0.15 MeV for the 6 MV target and backing. For the 18 MV beam, the values in the target were 3.6 MeV and 0.15 MeV and 1.0 MeV and 0.15 MeV in the target backing. These energy cut-off values were determined using a method similar to that described by Schach von Wittenau et al.8 BEAM was modified to score the energy of the parent particles of those in the phase space. The cut-off valMedical Physics, Vol. 30, No. 4, April 2003 E. Determining the mean initial electron energy, the radial spread of these electrons and the target density The final dose distribution is a complex function of the mean electron energy, E , the radial spread of these electrons, FWHMrad and the target density, * target . Each of these parameters affects the depth-dose and lateral profile curves in different ways. Thus, sensitivity calculations were performed by varying one parameter and fixing the other two. For the calculations where the energy was varied, MWHMrad was 1.3 mm and * target was 18.0 g cm%3 . For the calculations where MWHMrad was varied, E was 6.0 MeV !6 MV" or 18.0 MeV !18 MV" and * target was 18.0 g cm%3 . For the calculations where the target density was varied, E was 6.0 MeV !6 MV" or 18.0 MeV !18 MV" and MWHMrad was 1.3 mm. F. Acceptance criteria As stated earlier, to achieve 2% accuracy in patient dose calculations, we estimate that in-water calculations should agree with measurements to within 1%. The measured data consists of depth-dose and dose-profile curves. Because each Monte Carlo-calculated dose point has statistical uncertainty and the uncertainty is inversely proportional to the square root of the number of uncorrelated events, the more points that are averaged over, the lower the overall uncertainty of the estimated value will be. For this reason, instead of comparing individual points on a depth-dose curve, the slope of the difference between the measured and calculated curves was used. Thus, if the slope of the difference between the measured and calculated data is zero, the two curves can be considered identical to within statistical error. This slope of the difference technique was applied to depth-dose and doseprofile curves. If we assume that the measured and calculated depth-dose and dose-profile curves have the same shape, then the measured and calculated curves can be compared by computing the slope of the difference of the curves. A large difference in slope will manifest itself as depth-dose/dose-profile curve discrepancies between calculated and measured data. Similarly, a small difference in slope will yield depth-dose and dose-profile curves that match each other. To obtain a difference of &1% for water over !0,40" cm depth, the slope of the difference between the measured and calculated depth-dose Keall et al.: Determining the incident electron fluence 577 TABLE I. Pass/fail results for acceptability of depth-dose and dose-profile curve comparisons for a nominal 6 MV beam as electron energy, electron FWHM and target density are varied. The fraction of the acceptance criteria is given in brackets. The bold numbers correspond with the parameter varied. The italicized fields correspond to the energy, electron FWHM and density combinations that are acceptable by both depth-dose and doseprofile criteria. TABLE II. Pass/fail results for acceptability of depth-dose and dose-profile curve comparisons for a nominal 18 MV beam as electron energy, electron FWHM and target density are varied. The fraction of the acceptance criteria is given in brackets. The bold numbers correspond with the parameter varied. The italicized fields correspond with energy, electron FWHM and density combinations that are acceptable by both depth-dose and dose-profile criteria. 577 Acceptable? !fraction of acceptance criteria" Acceptable? !fraction of acceptance criteria" Energy !MeV" Electron FWHM !mm" Target density !g cm%3 ) Depth dose Dose profiles Energy !MeV" Electron FWHM !mm" Target density !g cm%3 ) Depth dose Dose profiles 5.6 5.8 6.0 6.2 6.4 1.3 1.3 1.3 1.3 1.3 18 18 18 18 18 No !%1.33" Yes !%0.63" Yes !0.23" Yes !0.06" No !1.36" No !5.5" No !3.9" No !2.3" Yes !%0.68" No !%1.9" 17.0 17.5 18.0 18.5 19.0 1.3 1.3 1.3 1.3 1.3 18 18 18 18 18 Yes !%0.89" Yes !%0.97" Yes !%0.55" Yes !0.70" Yes !0.46" Yes !0.54" No !%1.4" No !%3.4" No !%6.0" No !%7.8" 6.0 6.0 6.0 1.2 1.3 1.4 18 18 18 Yes !%0.07" Yes !0.23" Yes !%0.24" No !2.5" No !2.3" No !2.0" 18.0 18.0 18.0 0.9 1.3 1.6 18 18 18 Yes !%0.76" Yes !%0.55" Yes !0.21" No !%2.3" No !%3.4" No !%5.1" 6.0 6.0 1.3 1.3 17 18 Yes !%0.07" Yes !0.23" Yes !0.59" No !2.3" 18.0 18.0 1.3 1.3 17 18 Yes !0.29" Yes !%0.55" No !%3.1" No !%3.4" curves must be less than 0.01 D max /(40/2), or 0.0005D max cm%1 . Similarly, to obtain a difference of &1% for water over a 40!40 cm2 field size, the slope of the difference of the dose-profile curves must be less than 0.01 !D max /(20/2), or 0.001D max cm%1 from the central axis. These values were used as the acceptance criteria. The ranges used to compute the slope difference between the measured and calculated data were #5,25$ cm for the depthdose curves and #0,10$ cm for the lateral dose-profile curves. The lower bound of the depth-dose curve range !5 cm" was chosen, as it is beyond the range of contaminant electrons at both 6 and 18 MV. !Build-up region discrepancies between measurement and Monte Carlo have plagued many researchers,6,26,28,29 and a recent article by Ding42 concludes ‘‘a new explanation for the unresolved discrepancy remains to be found.’’" The upper bound was limited by the maximum depth of the measured depth-dose curves. The doseprofile curve range was only out to 10 cm to ensure that the comparisons were in the umbral region of the 25!25 cm2 measured dose-profile curves, and thus not affected by electronic disequilibrium. The choice of the 25!25 cm2 is explained in Sec. II D. If an initial electron fluence distribution is found that, when transported into a phantom, yields both depth-dose curves and dose-profile curves within the acceptance criteria !see Table I and Table II", then we have determined an acceptable initial electron fluence, suitable for use for Monte Carlo-based treatment planning in clinics that have linear accelerators whose characteristics match those of the standard data set. G. Verification calculations The derived values of E , MWHMrad and * target were verified by comparing calculations at 6 MV and 18 MV for 5!5 Medical Physics, Vol. 30, No. 4, April 2003 cm2 and 10!10 cm2 open fields, and 10!10 cm2 60° wedged fields with measured results. The voxel size used for these calculations was 0.4!0.4!0.4 cm3 . This voxel size was chosen, since a 0.4!0.4 cm2 square has a similar effective cross-sectional area to that of the Farmer-type ionization chamber used for the measurements !Wellhöfer IC15". An absolute dose !cGy/MU" was calculated to allow a direct comparison with ionization chamber measurements. The wedges were calculated in the BEAM simulation with the wedge created by stacking layers of component module JAWS. The geometry for the wedges was based on engineering diagrams and material specifications provided by the manufacturer. Although calculations performed starting with the determined initial electron fluence are validated for several field sizes, full commissioning of Monte Carlo treatment planning !following the guidelines of, e.g., TG 5343" is outside the scope of this article. III. RESULTS A. Depth-dose results: Initial mean electron energy Figure 1 shows the measured and calculated depth-dose curves for both 6 and 18 MV. This figure highlights the insensitivity of the initial electron energy on the depth-dose curve past the depth of maximum dose. The use of the build-up region for energy determination is possible, however, due to the inability to accurately correlate the ion chamber reading with the dose in the build-up region, the accuracy of the results would be questionable. The differences between the various calculations and measurements are quantified in Table I !6 MV" and Table II !18 MV". Table I shows that the depth-dose curves from 5.8 to 6.2 MeV are within the acceptance criteria. As the initial 578 Keall et al.: Determining the incident electron fluence FIG. 1. A comparison of ion-chamber-measured 6 and 18 MV depth-dose curves with those calculated for !a" initial E values of 5.6 and 6.4 MeV, and !b" initial E values of 17.0 and 19.0 MeV. 578 FIG. 2. Comparisons of ion-chamber-measured 6 and 18 MV dose-profile curves at 10 cm depth with those calculated for !a" initial E values of 5.6 and 6.4 MeV, and !b" initial E values of 17.0 and 19.0 MeV. C. Dose-profile results: initial mean electron energy electron beam energy is increased from 5.6 MeV, the agreement with measurement improves until after 6.2 MeV, where the discrepancy increases. Table II shows that all the tested energies from 17.0 to 19.0 MeV yield acceptable depth-dose curves. B. Depth-dose results: initial electron radial FWHM and target material density Table I and Table II show the depth-dose curve comparisons, as the initial electron radial FWHM is varied for the 6 MV and 18 MV beams, respectively. Although the depthdose curve changes as the FWHM changes, the calculations agree with measurement to within the acceptance criteria. Similar conclusions can be drawn for the target material density. The change in density does affect the depth-dose curve, but this change is not significant. Due to the relative insensitivity of the depth-dose curves to the initial mean electron energy, radial FWHM and target density, dose profiles give a more sensitive determination of these parameters. Medical Physics, Vol. 30, No. 4, April 2003 Figure 2 shows the measured and calculated dose-profile curves for both 6 and 18 MV beam energies. Figures 2!a" and 2!b" show that the initial electron energy affects the shape of the dose-profile curve, both near the central axis of the beam and the edge of the field. The agreement between calculation and measurement for the dose profiles is quantified in Table I and Table II. Table I shows that, for the calculations where the energy was varied, the 6.2 MeV initial energy gives the only profile that is within the acceptance criteria. Similarly, in Table II, there is one energy value !17.0 MeV" that gives dose profiles within the acceptance criteria. D. Dose-profile results: Initial electron radial FWHM Table I and Table II show that for the electron beam FWHM radial calculations, none of the dose profiles are within the acceptance criteria, indicating that either the electron energy used !6.0 MeV and 18.0 MeV" or the target density !18.0 g cm%3 ) is incorrect. These results do show, however, that as the FWHM increases, the size of the doseprofile ‘‘horns’’ will decrease. This effect is the same as that 579 Keall et al.: Determining the incident electron fluence FIG. 3. A comparison of calculated !histograms" and ion-chamber-measured !symbols" depth-dose curves for 4!4 and 10!10 cm2 open fields and a 10!10 cm2 60° wedge field at !a" 6 MV and !b" 18 MV. The cross at !5,0.6" represents the acceptance criteria of $1 mm or $1% of d max dose. Inset is the same plot with the x-axis from 0 to 3 cm. For the inset, the box at !1.5,0.5" represents the acceptance criteria of $1 mm or $1% of d max dose. of increasing energy !see Table I, Table II and Fig. 2", where the size of the dose-profile horns decreases as energy increases. E. Dose-profile results: Target material density Table I and Table II show that for the calculations where the target density was varied, the 17.0 g cm%3 calculated profiles are acceptable at 6 MV, but not at 18 MV. For the 6 MV case, the higher target density resulted in larger horns, whereas at 18 MV, the higher target density resulted in smaller horns. This difference could be due to the energy dependent attenuation coefficient values resulting in the target hardening the beam at 6 MV and softening the beam at 18 MV. From Table I and Table II, of those tested, the best input parameters to use for the Monte Carlo calculations are E "6.2 MeV and 17.0 MeV !for the 6 and 18 MV beams, respectively" and FWHMrad"1.3 mm and * target"18.0 g cm%3 . These input parameters were used for the verification Medical Physics, Vol. 30, No. 4, April 2003 579 FIG. 4. A comparison of calculated !histograms" and ion-chamber-measured !symbols" dose-profile curves at 10 cm depth for 4!4 and 10!10 cm2 open fields and a 10!10 cm2 60° wedge field at !a" 6 MV and !b" 18 MV. The cross at !0,0.5" represents the acceptance criteria of $1 mm or $1% of d max dose. calculations. Note that for the 6 MV case, there were two acceptable energy, FWHM and density combinations to choose from. We chose the combination with * target"18.0 g cm%3 to be consistent between 6 and 18 MV, as obviously the target density is independent of beam energy. F. Verification calculations Figure 3 and Fig. 4 show a comparison of calculated and measured depth-dose and dose-profile curves. At 6 MV, the curves agree well with the experiment and are within the 1% or 1 mm criteria. For the 18 MV calculations, the curves agree to within the specified criteria after the contamination electron range, however, at the maximum electron range, the calculated results are higher than the experiment. There are several reasons for this difference. Sheikh-Bagheri et al.5 found that correcting for the effective point of measurement of the ion chamber reduces much of the discrepancy in the build-up region and up to 2 cm beyond d max for 10 and 20 MV beams. Part of the discrepancy is because the measured 580 Keall et al.: Determining the incident electron fluence 580 TABLE III. A comparison of this work with other studies that have used Monte Carlo methods to model Varian accelerators. Accelerator Nominal energy !MV" Mean electron energy !MeV" FWHM electron energy spread !% of mean" Ding !Ref. 26" 2100EX 6 6.02 17% Ding !Ref. 26" 2100EX 18 18.00 6% Clinac 2100C/D Clinac high energy 6 6 6.05 6.2 0 0 Clinac high energy 18 18.5 0 Liu et al. !Ref. 27" 2100C 6 6.5 0 Liu et al. !Ref. 27" 2100C 18 20.0 0 Clinac high energy 6 5.7 3% Clinac high energy 18 18.3 3% 2100EX 6 6.2 3% 2100EX 18 17.0 3% Author Fix et al. !Ref. 24" Hartmann-Siantar et al. !Ref. 6" Hartmann-Siantar et al. !Ref. 6" Sheikh-Bagheri and Rogers !Refs. 28 and 29" Sheikh-Bagheri and Rogers !Refs. 28 and 29" This work This work ionization curves have not been converted to dose using variable water/air stopping power ratios. This ratio is fairly constant after the build-up depth, however, at depths below this point, the stopping power ratios vary.44 IV. DISCUSSION The initial electron fluence above the linear accelerator target has been determined for two photon energies !6 and 18 MV" of one linear accelerator model that, when transported into phantoms, yields dose distributions within 1% or 1 mm of the experimental measurements, except near the surface. These initial electron fluences have been transported to a plane between the monitor chambers and the jaws of the linear accelerator and scored in the form of phase-space files. These phase-space files are used in the Monte Carlo system at our clinic for dosimetric verification of every IMRT patient treated, with the results documented, signed and included in the patient chart. These phase-space files have also formed the basis for Monte Carlo calculations of multileaf collimator transport, which have been experimentally verified in several publications.45– 47 The dosimetric effects of !1" the mean electron energy of the initial electron fluence, !2" the radial spread of the initial electron fluence and !3" the target density were studied. The initial electron energy, initial electron radial spread and target density all affect the depth-dose and dose-profile curves. An increase in beam energy increases the penetration of the depth-dose and decreases the horns of the dose-profile curves. An increase in the radial FWHM also decreases the Medical Physics, Vol. 30, No. 4, April 2003 Electron radial distribution 1.2 mm FWHM Gaussian function 1.5 mm FWHM Pencil beam 2 mm diameter cylindrical function 2 mm diameter cylindrical function 4 mm diameter cylindrical function 4 mm diameter cylindrical function 2.0 mm FWHM Gaussian function 1.1 mm FWHM Gaussian function 1.3 mm FWHM Gaussian function 1.4 mm FWHM Gaussian function Depth-dose agreement with measurement Good Measured dose high for large fields and shallow depths Good Good Measured dose high for large fields and shallow depths Not shown Not shown Good Measured dose high for shallow depths Good Measured dose high for shallow depths horns of the dose-profile curves. An increase in target density has the effect of hardening the 6 MV depth-dose curve and softening the 18 MV depth-dose curve. Based on our results of modeling the ‘‘standard’’ measured data set of the input variables tested, the best parameters to use for the EGS4 calculations to model the Cl21EX linear accelerator are initial mean electron energy 6.2 MeV and 17.0 MeV for 6 and 18 MV beams, respectively, with a FWHM of the radial spread of these electrons of 1.3 mm and a target density of 18.0 g cm%3 . Calculations performed using these phase-space files agree with measurements past the build-up region to within 1% or 1 mm over the 4!4 to 25!25 cm2 field size range tested. However, in the build-up region, the 18 MV depth-dose curves were significantly higher than those of the ion chamber measured curves. The disagreement between the measured data highlights the need for benchmark data sets, such as those to be conducted under the auspices of AAPM Task Group 67. A comparison of the derived parameters from this work with that of previous publications relating to the Monte Carlo modeling of Varian linear accelerators is shown in Table III. It is interesting to note that even though each approach is unique and the parameters used vary, the dosimetric results are similar. Each group achieved the 6 MV beam modeling, but none of the groups, as of yet, has accurately modeled the 18 MV beam for shallow depths and large field sizes. This inability to accurately model the high-energy beams could be due to several factors, such as the cross sections and transport methods used by the Monte Carlo codes, inaccurate geometrical specifications by the manufacturer, erroneous as- Keall et al.: Determining the incident electron fluence 581 sumptions of the initial electron fluence distribution above the target and the conversion from measured ionization to dose. Currently, the phase-space files store the particles below the monitor chamber. Thus, in our Monte Carlo implementation, we need to perform an empirical correction to account for the backscatter to the monitor chambers from the collimators.48 Future work will concentrate on storing the phase space above the monitor chambers so that the backscatter to the monitor chambers can be calculated directly. The final phase-space files are freely available from the authors !a 4-CD set". The 6 MV phase space contains 60 million particles, and the 18 MV phase space contains 45 million. Note that the phase spaces determined here have only been tested for the EGS4 Monte Carlo code. Other codes using different transport methodologies and cross sections may yield differing results. Carlo dose calculation code PEREGRINE,’’ presented at the XII International Conference on the Use of Computers in Radiotherapy, Salt Lake City, Utah, 1997. 10 R. Jeraj, D. Wenman, J. Balog, D. Pearson, G. Olivera, P. Reckwerdt, and R. 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