Instruments Method
of measurements of multiplier conversion losses
Method of measurements of multiplier
conversion losses
We have developed a series of multipliers based on planar Schottky diodes (Device 010) for primary sources radiation frequency multiplication. Multipliers are based on a ridged waveguide and/or waveguidefinlinewaveguide transition. Singlemode waveguides are used for 35178 GHz range multipliers (Device 016). Quasioptical construction is employed for higher frequency range (Device 007).
The multipliers were successfully used for extension of frequency range of high resolution microwave spectroscopy both with radio acoustical detector and LHe cooled bolometer up to 1.5 Teraherz [Ref. 3, 4 (1995), Ref. 8 (1999)].
While working on BWO radiation frequency multiplication and
precisely controlled using PLL system source of radiation
in the range of 13 mm we developed a universal method of measurement of conversion losses for every separate harmonic with numbers from 2 to 5 produced and radiated by the multiplier. The method is based on measurement of absorption of radiation in spectral lines with known intensity and acoustic detection of this absorption.
Blockdiagram of radiation frequency multiplication experiments.
The radiation of the source passed through the multiplier and containing both fundamental radiation and harmonics is directed into acoustic gas cell (radioacoustic detector  Device 004) commonly used in our spectroscopic experiments. The cell is filled by gas with well known spectrum. Observed spectral lines are recorded and analyzed by PC. The following properties of the acoustic detector in addition to its high sensitivity make it a crucial element of the method: (i) sensitivity of radioacoustic detector is independent of frequency range, polarization and space mode of the radiation; (ii) there is no signal from the acoustic detector if there is no absorption in the spectral line of gas inside the cell; (iii) output signal has linear dependence on the radiation power which was absorbed inside the gas cell. Thus a minor power of a few nanowatts at any particular harmonic may be detected in spite of the fact that at the same time hundreds of milliwatts of fundamental power and other harmonics are passing through the cell but do not produce any signal. So spectral lines of the gas the frequencyselective element which allows us to distinguishing one harmonic from another and the latters from the fundamental. The main criterion of identification of observed line is coincidence of its frequency with calculated line frequency taken from the spectrum data base. The use of PLL stabilization of the fundamental radiation source supports the method with such high accuracy of line frequency measurement that the line identification is undoubted. The observed spectral line width is an additional criterion for the line identification. Due to the principal of lines observation the frequency step of radiation scanning through a range is determined by frequency step of fundamental radiation, but for radiation at harmonics the value of the step should be multiplied by corresponding harmonic number. So if the harmonic number is higher, then narrower is the linewidth of observed line. The amplitude of the observed line is in direct proportion to the line intensity (except the case of too strong absorption which can be estimated beforehand) and to the power of radiation. So comparison of the amplitude of observed lines with known intensities allows quantitative comparison of power at different harmonics. In particular, such important characteristic of multiplier as conversion losses can be determined. Dynamic range of such measurements is limited by the acoustic sell sensitivity; in our experiment it was about 55 dB. Accuracy of the method is limited by variation of power of radiation inside the acoustic cell due to parasitic interference when radiation frequency changes from one line to another. In our experiments the accuracy of measurements was about 20%. Use of this method permitted for the first time to make tuning and adjusting of submillimeterwave multipliers at every harmonic
in real time.
MM radiation multipliers conversion losses measurement
SMM radiation multiplier conversion losses
measurement
See the paper [Ref. 1 (2000)] for more details on the
method and its applications.
