Alfvén waves
The theoretical derivation of the existence of magnetohydrodynamic waves by Hannes Alfvén was recognized with the Nobel Prize for Physics in 1970. These Alfvén waves now play an important role in the physics of the solar atmosphere and magnetosphere as well as in fusion research. Soon after their prediction in 1942, Alfvén waves were first detected in liquid metal experiments and later studied in detail in complex plasma devices. While the speed of the Alfvén wave in liquid metals is usually significantly lower than the speed of sound, this relationship is reversed in plasma experiments. Conditions under which both speeds are equal have not yet been achieved in either type of experiment. However, this point in the solar atmosphere is crucial for heating the solar corona to temperatures of several million degrees. It is assumed that it is precisely here that sound waves are converted into Alfvén waves, which can then introduce sufficient "heating energy" into the corona.
This condition was achieved for the first time in an experiment at the Dresden High Magnetic Field Laboratory (HLD) using a pulsed field of up to 62 Tesla (Fig. 1). For liquid rubidium, the "magic point" corresponds to a field strength of 53 Tesla. By feeding an alternating current at the bottom of the container while simultaneously applying the pulsed magnetic field, Alfvén waves were generated in the melt, whose upward movement was measured at the expected speed. While up to a field strength of 53 Tesla all measurements were dominated by the frequency of the alternating current fed in, a new signal with a half frequency appeared at exactly this point (Fig. 2). This sudden period doubling was in perfect agreement with the theoretical predictions of a parametric resonance between sound and Alfvén waves.
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Stefani, F., Forbriger, J, Gundrum, Th., Herrmannsdörfer, Wosnitza, J.
Mode Conversion and Period Doubling in a Liquid Rubidium Alfvén-Wave Experiment with Coinciding Sound and Alfvén Speeds
Physical Review Letters 127 (2021), 275001