Volume 633, January 2020
|Number of page(s)||5|
|Section||Letters to the Editor|
|Published online||13 January 2020|
Letter to the Editor
First direct observation of a torsional Alfvén oscillation at coronal heights⋆
Rosseland Centre for Solar Physics, University of Oslo, PO Box 1029, Blindern 0315, Oslo, Norway
2 Institute of Theoretical Astrophysics, University of Oslo, PO Box 1029, Blindern 0315, Oslo, Norway
3 Centre for Fusion, Space and Astrophysics, Department of Physics, University of Warwick, Coventry CV4 7AL, UK
4 LPC2E, CNRS and University of Orléans, 3A avenue de la Recherche Scientifique, Orléans, France
Accepted: 7 December 2019
Context. Torsional Alfvén waves are promising candidates for the transport of energy across different layers of the solar atmosphere. They have been predicted theoretically for decades. Previous detections of Alfvén waves so far have however mostly relied on indirect signatures.
Aims. We present the first direct observational evidence of a fully resolved torsional Alfvén oscillation of a large-scale structure occurring at coronal heights.
Methods. We analysed IRIS imaging and spectral observation of a surge resulting from magnetic reconnection between active region prominence threads and surrounding magnetic field lines.
Results. The IRIS spectral data provide clear evidence of an oscillation in the line-of-sight velocity with a 180° phase difference between the oscillation signatures at opposite edges of the surge flux tube. This together with an alternating tilt in the Si IV and Mg II k spectra across the flux tube and the trajectories traced by the individual threads of the surge material provide clear evidence of torsional oscillation of the flux tube.
Conclusions. Our observation shows that magnetic reconnection leads to the generation of large-scale torsional Alfvén waves.
Key words: magnetohydrodynamics (MHD) / Sun: corona / Sun: oscillations / Sun: magnetic fields
Movies attached to Figs. 1 and 2 are available at https://www.aanda.org
© ESO 2020
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