Upper Hybrid Resonance and Waves
The upper hybrid frequency is a resonance phenomenon for electromagnetic waves with E perpendicular to B, propagating across the static magnetic field B0. A resonance (infinite k) is a layer of strong wave absorption. Vice versa, it is a region of strong thermal emission. Furthermore, warm plasma modes play a role and there is the possibility of mode conversion when both modes have the same resonance. These phenomena have been studied experimentally. The findings offer interesting diagnostic applications for perturbation-free and sensitive density and temperature measurements.
The experimental setup shown in Fig. 1 is relatively simple. A pulsed rf discharge is created in a glass tube aligned along an external magnetic field. it passes through the sides of a rectangular S-band waveguide so as to interact with electromagnetic waves with polarization of extraordinary modes. However, the plasma dimension is small compared to the electromagnetic wavelength, hence is nearly an interaction in a capacitor field. The measurement setup uses a radiometer, which contains a sensitive receiver and measures in alternating pulses the signal with and without plasma. The absorption of the plasma is found to be nearly total when the plasma provides an upper hybrid resonance at the test wave frequency.
Figure 2 shows the condition for the upper hybrid resonance in a nonuniform plasma column. The radial density profile is parabolic and decays in the afterglow of the pulsed discharge. The upper hybrid frequency is shown in a graph of density vs magnetic field for a constant signal frequency. At the highest density in the plasma center the upper hybrid resonance occurs at the lowest magnetic field. Vice versa, at the lowest density (column edge) the upper hybrid frequency coincides with the cyclotron resonance.
measurements of the absorption coefficient are shown in Fig. 3a. throughout the range of upper hybrid resonances there is strong absorption. The onset of absorption occurs at the highest density, hence yields the density in the column center. With increasing afterglow time the onset shifts from which one can obtain the peak density decay as shown in Fig. 3b.
By Kirchhoff's law a medium with high absorption coefficient will also be a strong emitter of thermal radiation. This is verified with a sensitive radiometer, which compares the thermal emission from the plasma with a calibrated blackbody radiation source. Since an afterglow plasma has a Maxwellian distribution the radiation temperature is the electron temperature. In Fig. 4a the radiation temperature is plotted vs magnetic field for different afterglow times. For the lowest magnetic field the resonance lies in the column center, hence the temperature refers to r=0. Near cyclotron resonance the temperature is that at the column edge. In between the traces show the radial temperature profiles. The peak electron temperature decay is shown in Fig. 4b. Electron temperatures can almost be resolved to room temperature. This temperature diagnostics is both non-perturbing and very sensitive.
So far the upper hybrid layer has been inferred externally. In the next experiment is made visible by electron heating with a strong "test" wave. Figure 6a shows electron temperature measurements made with the radiometer after the end of a short heating pulse. The electron temperature is locally raised, where the radial position is obtained from the magnetic field dependence (Fig. 5a). Further increase in rf power creates light emission at the upper hybrid layer (Fig. 5b). An axial view of the normally dark afterglow plasma shows a bright ring whose radius varies with frequency or magnetic field. It follows the position of the upper hybrid resonance layer measured without the heating pulse. It provides a visual confirmation that the upper hybrid layer is a localized region of strong absorption and emission.
It has been pointed out that the upper hybrid frequency is a resonance for both cold plasma waves (extraordinary em waves) and warm plasma modes (electron cyclotron harmonic waves). The latter form radial standing waves in the plasma interior which can be seen in absorption measurements shown in Fig. 7a. Resonant oscillations are seen as the density decays in the afterglow and the number of standing waves changes. The observed mode spacing in density for different magnetic fields has been compared with theory and shown good agreement (Fig. 7b).
References
- Microwave Scattering and Noise Emission from Afterglow Plasmas in a Magnetic Field, F. A. Blum, L. O. Bauer, R. W. Gould and R. L. Stenzel, Phys. Fluids 12, 1018-1027 (1969). [Link to original publication.]
- Afterglow Plasma Diagnostics with a Microwave Sampling Radiometer, R. L. Stenzel and R. W. Gould, Rev. Sci. Instrum. 40, 1461-1466 (1969). [Link to original publication.]
- Upper-Hybrid Resonance Absorption, Emission and Heating of an Afterglow Plasma Column, R. L. Stenzel and R. W. Gould, J. Appl. Phys. 42, 4225-4235 (1971). [Link to original publication.]
- Longitudinal Oscillations in Bounded Magnetoplasmas, R. L. Stenzel and R. W. Gould, Phys. Fluids 14, 187-188 (1971). [Link to original publication.]