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魔角旋转动态核极化 NMR 探头中的微波场分布。

Microwave field distribution in a magic angle spinning dynamic nuclear polarization NMR probe.

机构信息

Plasma Science and Fusion Center, Massachusetts Institute of Technology, Cambridge, MA 02139, USA.

出版信息

J Magn Reson. 2011 May;210(1):16-23. doi: 10.1016/j.jmr.2011.02.001. Epub 2011 Mar 5.

DOI:10.1016/j.jmr.2011.02.001
PMID:21382733
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC3081422/
Abstract

We present a calculation of the microwave field distribution in a magic angle spinning (MAS) probe utilized in dynamic nuclear polarization (DNP) experiments. The microwave magnetic field (B(1S)) profile was obtained from simulations performed with the High Frequency Structure Simulator (HFSS) software suite, using a model that includes the launching antenna, the outer Kel-F stator housing coated with Ag, the RF coil, and the 4mm diameter sapphire rotor containing the sample. The predicted average B(1S) field is 13μT/W(1/2), where S denotes the electron spin. For a routinely achievable input power of 5W the corresponding value is γ(S)B(1S)=0.84MHz. The calculations provide insights into the coupling of the microwave power to the sample, including reflections from the RF coil and diffraction of the power transmitted through the coil. The variation of enhancement with rotor wall thickness was also successfully simulated. A second, simplified calculation was performed using a single pass model based on Gaussian beam propagation and Fresnel diffraction. This model provided additional physical insight and was in good agreement with the full HFSS simulation. These calculations indicate approaches to increasing the coupling of the microwave power to the sample, including the use of a converging lens and fine adjustment of the spacing of the windings of the RF coil. The present results should prove useful in optimizing the coupling of microwave power to the sample in future DNP experiments. Finally, the results of the simulation were used to predict the cross effect DNP enhancement (ϵ) vs. ω(1S)/(2π) for a sample of (13)C-urea dissolved in a 60:40 glycerol/water mixture containing the polarizing agent TOTAPOL; very good agreement was obtained between theory and experiment.

摘要

我们呈现了一种在魔角旋转(MAS)探针中微波场分布的计算,该探针用于动态核极化(DNP)实验。微波磁场(B(1S))分布是通过高频结构模拟器(HFSS)软件套件进行的模拟得到的,使用的模型包括发射天线、涂有 Ag 的外 Kel-F 定子外壳、RF 线圈和包含样品的 4mm 直径蓝宝石转子。预测的平均 B(1S)场为 13μT/W(1/2),其中 S 表示电子自旋。对于通常可实现的 5W 输入功率,相应的值为 γ(S)B(1S)=0.84MHz。这些计算提供了对微波功率与样品耦合的深入了解,包括来自 RF 线圈的反射和通过线圈传输的功率的衍射。还成功模拟了增强与转子壁厚的变化。使用基于高斯光束传播和菲涅耳衍射的单通模型进行了第二次简化计算。该模型提供了额外的物理见解,并与完整的 HFSS 模拟很好地吻合。这些计算表明了增加微波功率与样品耦合的方法,包括使用会聚透镜和微调 RF 线圈绕组的间距。这些结果应该有助于优化未来 DNP 实验中微波功率与样品的耦合。最后,模拟结果用于预测溶解在含有极化剂 TOTAPOL 的 60:40 甘油/水混合物中的 (13)C-尿素样品的交叉效应 DNP 增强(ϵ)与 ω(1S)/(2π)的关系,理论与实验之间非常吻合。

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