Abstract
The Mark II W-band (94 GHz) EPR spectrometer with a low-noise millimeter-wave amplifier is described. The microwave bridge is of a high-sensitivity homodyne design. Signal-to-noise ratios were measured for a number of detectors with and without the low-noise amplifier. The signal-to-noise ratio was determined not only by the type of detector but also how well it was matched. Without a microwave preamplifier, a hot-electron bolometer provides the best signal-to-noise ratio. Addition of a low-noise microwave preamplifier to the CW homodyne bridge gives a 10 dB improvement in the noise figure of the receiver at a modulation frequency of 100 kHz. A greater improvement in the signal-to-noise ratio is seen at low modulation frequencies (1–10 kHz), making the low-noise amplifier useful for systems with large linewidths. This allows larger modulation amplitudes to be used without causing significant cavity heating or microphonics. The W-band spectrometer is capable of rapid sweeps from 0 to 7 T, as well as narrower (0.1 T) high-resolution sweeps. It is suitable for a wide variety of samples including liquids and samples cooled to sub-liquid-helium temperatures.
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Nilges, M.J., Smirnov, A.I., Clarkson, R.B. et al. Electron paramagnetic resonance W-band spectrometer with a low-noise amplifier. Appl. Magn. Reson. 16, 167–183 (1999). https://doi.org/10.1007/BF03161932
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DOI: https://doi.org/10.1007/BF03161932