Jackson Michael, Zink Lyndon R
Department of Physics, Central Washington University; College of Science and Technology, Millersville University;
Department of Physics, University of Wisconsin-La Crosse.
J Vis Exp. 2015 Dec 18(106):e53399. doi: 10.3791/53399.
The generation and subsequent measurement of far-infrared radiation has found numerous applications in high-resolution spectroscopy, radio astronomy, and Terahertz imaging. For about 45 years, the generation of coherent, far-infrared radiation has been accomplished using the optically pumped molecular laser. Once far-infrared laser radiation is detected, the frequencies of these laser emissions are measured using a three-laser heterodyne technique. With this technique, the unknown frequency from the optically pumped molecular laser is mixed with the difference frequency between two stabilized, infrared reference frequencies. These reference frequencies are generated by independent carbon dioxide lasers, each stabilized using the fluorescence signal from an external, low pressure reference cell. The resulting beat between the known and unknown laser frequencies is monitored by a metal-insulator-metal point contact diode detector whose output is observed on a spectrum analyzer. The beat frequency between these laser emissions is subsequently measured and combined with the known reference frequencies to extrapolate the unknown far-infrared laser frequency. The resulting one-sigma fractional uncertainty for laser frequencies measured with this technique is ± 5 parts in 10(7). Accurately determining the frequency of far-infrared laser emissions is critical as they are often used as a reference for other measurements, as in the high-resolution spectroscopic investigations of free radicals using laser magnetic resonance. As part of this investigation, difluoromethane, CH2F2, was used as the far-infrared laser medium. In all, eight far-infrared laser frequencies were measured for the first time with frequencies ranging from 0.359 to 1.273 THz. Three of these laser emissions were discovered during this investigation and are reported with their optimal operating pressure, polarization with respect to the CO2 pump laser, and strength.
远红外辐射的产生及后续测量已在高分辨率光谱学、射电天文学和太赫兹成像中得到了众多应用。在大约45年的时间里,一直通过光泵浦分子激光器来产生相干远红外辐射。一旦检测到远红外激光辐射,就使用三激光外差技术测量这些激光发射的频率。利用该技术,将光泵浦分子激光器的未知频率与两个稳定的红外参考频率之间的差频进行混频。这些参考频率由独立的二氧化碳激光器产生,每个激光器都利用来自外部低压参考池的荧光信号进行稳定化处理。已知和未知激光频率之间产生的拍频由金属-绝缘体-金属点接触二极管探测器进行监测,其输出在频谱分析仪上观察。随后测量这些激光发射之间的拍频,并与已知参考频率相结合,以推断未知的远红外激光频率。用该技术测量激光频率时,所得的一西格玛分数不确定度为±10⁷分之5。准确确定远红外激光发射频率至关重要,因为它们常被用作其他测量的参考,例如在使用激光磁共振对自由基进行高分辨率光谱研究中。作为该研究的一部分,二氟甲烷(CH₂F₂)被用作远红外激光介质。总共首次测量了八个远红外激光频率,频率范围为0.359至1.273太赫兹。在本次研究中发现了其中三种激光发射,并报告了它们的最佳工作压力、相对于二氧化碳泵浦激光的偏振以及强度。