James B J, Strohbehn J W, Mechling J A, Trembly B S
Thayer School of Engineering, Dartmouth College, Hanover, NH 03755.
Int J Hyperthermia. 1989 Nov-Dec;5(6):733-47. doi: 10.3109/02656738909140498.
Interstitial microwave antenna array hyperthermia (IMAAH) is presently used clinically in the treatment of cancer. This paper presents the theoretical specific absorption rate (SAR) patterns of 915 MHz microwave antenna arrays for varying insertion depths. The antennas were oriented in a 2 x 2 cm square array. Insertion depth, defined as distance from skin to antenna tip, ranged from 5.9 to 17.6 cm. Two different antenna configurations were considered. In the first the antenna had a distal section a quarter-wavelength long (resonant case), while the second had a distal section approximately 13% longer than a quarter-wavelength (non-resonant case). SAR patterns were calculated from theoretical expressions, and displayed as lines of constant SAR normalized to the maximum SAR value in the array. The results show that regions of concentrated power deposition or 'hotspots' occurred in the centre of the array and moved in a complex but predictable fashion as insertion depth was varied. For insertion depths shorter than a resonant half-wavelength, there occurred one hotspot distal to the antenna junctions. As insertion depth was increased beyond a resonant half-wavelength, the hotspot moved proximal to the antenna junctions and eventually split in two. For depths very much longer than a resonant half-wavelength a hotspot centred about the antenna junction dominated the SAR pattern. For the resonant case the maximum SAR was often along the central axis of the array, while for the non-resonant case the maximum SAR was at the antennas with a local maximum on the central axis.
间质微波天线阵列热疗(IMAAH)目前在临床上用于癌症治疗。本文介绍了915 MHz微波天线阵列在不同插入深度下的理论比吸收率(SAR)模式。天线排列成2×2平方厘米的方阵。插入深度定义为从皮肤到天线尖端的距离,范围为5.9至17.6厘米。考虑了两种不同的天线配置。第一种情况下,天线的远端部分为四分之一波长(谐振情况),而第二种情况下,远端部分比四分之一波长约长13%(非谐振情况)。SAR模式由理论表达式计算得出,并显示为以阵列中最大SAR值归一化的恒定SAR线。结果表明,集中功率沉积区域或“热点”出现在阵列中心,并随着插入深度的变化以复杂但可预测的方式移动。对于小于谐振半波长的插入深度,在天线节点远端出现一个热点。当插入深度增加到超过谐振半波长时,热点向天线节点近端移动并最终分裂为两个。对于远大于谐振半波长的深度,以天线节点为中心的热点主导了SAR模式。对于谐振情况,最大SAR通常沿阵列中心轴,而对于非谐振情况,最大SAR位于天线处,在中心轴上有局部最大值。