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SU-E-T-126:高能光子剂量测定中典型辐射探测器的非参考条件校正因子KNR

SU-E-T-126: Non-Reference Condition Correction Factor KNR of Typical Radiation Detectors for the Dosimetry of High-Energy Photons.

作者信息

Chofor N, Poppe B, Harder D

机构信息

Pus Hospital Oldenburg.

Georg-August Universitaet Goettingen.

出版信息

Med Phys. 2012 Jun;39(6Part11):3732. doi: 10.1118/1.4735184.

Abstract

PURPOSE

To correct for the deviations of the detector response when typical radiation detectors are used under non-reference conditions, factor kNR was calculated from the known energy dependence of the detector response at photon energies from 10 keV upwards and from clinical photon spectra within a large water phantom beneath a Siemens Primus 6/15 MV linac. A Farmer type ion chamber (NE2571), two TLD detector types and two diodes were investigated.

METHODS

Factor kNR was obtained as the ratio of the weighted responses Yt of a given detector t under reference conditions xref (axial distance r = 0 cm, depth d = 10 cm, field size 10 × 10 cm and SSD = 100 cm) and that under non-reference conditions × (off-axis points and depths for various field sizes); kNR = Yt(xref)/Yt(x). For small field (SF) dosimetry, we evaluated correction factor kNRSF, which refers to small field reference conditions (4 × 4 cm field).

RESULTS

For all detectors investigated, the deviations of kNR from unity were highest outside the field, due to prevailing low-energy scatter contributions. For the Farmer chamber and EDP-10 diode, the kNR deviations did not exceed 2%, but were up to 60% for the EDD-5 diode, while kNR values for LiF:Mg,Cu,P and LiF:Mg,Ti deviated at most 15% and 5% respectively. kNR values appear as unique functions of the mean photon energy at the point of interest.

CONCLUSIONS

Air-filled ion chambers show only small kNR variations, while for non-water equivalent detectors, kNR variations depend on the detector response at low photon energy. kNR can be presented as a unique function of the mean photon energy at the point of interest. A 4 × 4 cm reference field is recommended for small fields, with correction factor kNRSF varying almost negligibly from kNR except for unshielded Si diodes.

摘要

目的

为校正典型辐射探测器在非参考条件下使用时的探测器响应偏差,根据探测器响应在10keV及以上光子能量下已知的能量依赖性以及西门子Primus 6/15MV直线加速器下方大水体模内的临床光子能谱,计算了因子kNR。研究了一种Farmer型电离室(NE2571)、两种TLD探测器类型和两种二极管。

方法

因子kNR通过给定探测器t在参考条件xref(轴向距离r = 0cm、深度d = 10cm、射野尺寸10×10cm且源皮距SSD = 100cm)下的加权响应Yt与非参考条件x(各种射野尺寸的离轴点和深度)下的加权响应Yt之比获得;kNR = Yt(xref)/Yt(x)。对于小射野剂量学,我们评估了校正因子kNRSF,它指的是小射野参考条件(4×4cm射野)。

结果

对于所有研究的探测器,由于主要是低能散射贡献,kNR与1的偏差在场外最高。对于Farmer电离室和EDP - 10二极管,kNR偏差不超过2%,但对于EDD - 5二极管高达60%,而LiF:Mg,Cu,P和LiF:Mg,Ti的kNR值分别最多偏差15%和5%。kNR值表现为感兴趣点处平均光子能量的独特函数。

结论

充气电离室的kNR变化很小,而对于非水等效探测器,kNR变化取决于探测器在低光子能量下的响应。kNR可表示为感兴趣点处平均光子能量的独特函数。对于小射野,建议使用4×4cm参考射野,除未屏蔽的硅二极管外,校正因子kNRSF与kNR的变化几乎可忽略不计。

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