Do periods of decayless kink oscillations of solar coronal loops depend on noise?
Abstract
Decayless kink oscillations of solar coronal loops are studied in terms of a lowdimensional model based on a randomly driven Rayleigh oscillator with coefficients experiencing random fluctuations. The model considers kink oscillations as natural modes of coronal loops, decaying by linear resonant absorption. The damping is counteracted by random motions of the loop footpoints and the interaction of the loop with external quasisteady flows with random fluctuations. In other words, the model combines the selfoscillatory and randomly driven mechanisms for the decayless behaviour. The random signals are taken to be of the stationary red noise nature. In the noiseless case, the model has an asymptotically stationary oscillatory solution, i.e. a kink selfoscillation. It is established that the kink oscillation period is practically independent of noise. This finding justifies the seismological estimations of the kink and Alfvén speeds, and the magnetic field in an oscillating loop by kink oscillations, based on the observed oscillation period. The oscillatory patterns are found to be almost harmonic. Noisy fluctuations of external flows modulate the amplitude of the almost monochromatic oscillatory pattern symmetrically, while random motions of the loop footpoints cause antisymmetric amplitude modulation. Such modulations are also consistent with the observed behaviour.
 Publication:

Monthly Notices of the Royal Astronomical Society
 Pub Date:
 November 2022
 DOI:
 10.1093/mnras/stac2628
 arXiv:
 arXiv:2209.06343
 Bibcode:
 2022MNRAS.516.5227N
 Keywords:

 waves;
 Sun: corona;
 Sun: oscillations;
 Astrophysics  Solar and Stellar Astrophysics
 EPrint:
 Accepted for publication in MNRAS. 5 pages, 4 figures