Head scatter off‐axis for megavoltage x rays

Our objective in this study has been to investigate how head scatter varies with the off‐axis position in a 6 MV x‐ray beam. We define the head‐scatter off‐axis ratio, HOA, as the ratio of the kerma due to head‐scatter photons at the off‐axis position x to the kerma from direct primary photons on the central axis. “Direct primary” are those photons that come from the source without interactions in the intervening structures. We determined HOA from measurements with an ionization chamber in a miniphantom. Head‐scatter and direct primary photons contribute to a measurement of the ionization per mu Q ( x ) at the off‐axis position x in the open field cx × cy . The ionization per mu QP ( x ) , measured in the same position but with the field collimated to the smallest possible opening ( cx × 3   cm ) , is intended to include only direct primary photons. Head‐scatter photons cannot be completely eliminated, and the errors due to remaining head scatter and radiation backscattered by the movable collimators into the monitor were estimated. For normalization of the final results, ionization due to direct primary photons was also measured on the central axis, QP ( 0 ) . HOA was derived from these three measurements as HOA ( cx , cy , x ) = ( Q ( cx , cy , x ) − QP ( cx , cy , x ) ) / QP ( cx , cy , 0 ) . On the central axis ( x = y = 0 ) , HOA represents the “scatter‐to‐primary ratio” between head scatter and the direct primary dose. Monte Carlo simulations were made to help with the interpretation and evaluation of the results. HOA could be fitted to a Gaussian model with two components corresponding to sources of widths 1.8 and 14 cm, projected on a plane 5 cm below the x‐ray source. The narrow Gaussian component is interpreted as the source of photons scattered in the flattening filter and the primary collimator. The broad component is attributed to photons scattered in the secondary (variable) collimators. Conventional head‐scatter models (e.g., a single Gaussian source model) do not fit the measured HOA data for large collimator settings ( c > 20   cm ) or outside beam collimation. The full width at half‐maximum (FWHM) of HOA ( x ) across the field increased with the field width ( cx ) in the direction of the measurements in a manner consistent with the field of view of the two sources. It was not sensitive to the field measure in the orthogonal direction ( cy ). Head scatter outside the field also increased with field size, reflecting an increased contribution of photons scattered at large angles. It exceeds the leakage through the collimator 2 cm outside the edge for square fields c > 10   cm . Monte Carlo calculations showed considerably less head scatter outside the field than measurements.