Undersampling effects on observed periods of coronal oscillations

Context. Recent observations of decayless transverse oscillations have revealed two branches in the relationship between period and loop length. One is a linear relationship, interpreted as a standing mode, while the other shows almost no correlation and has not yet been interpreted conclusively. Aims. We investigated the undersampling effect on observed periods of decayless oscillations. Methods. We considered oscillating coronal loops that closely follow the observed loop length distribution. Assuming that all oscillations are standing waves, we modelled a signal that represents decayless oscillations where the period is proportional to the loop length and the amplitude and phase are randomly drawn. We generated a downsampled signal from the original signal by considering different sample rates that mimic temporal cadences of telescopes, and analysed the periods for sampled signals using the fast Fourier transform. Results. When the sampling cadence approaches the actual oscillation period, there is a greater tendency to overestimate the periods in short loops. We find the same two branches in the relationship between loop length and period of the sampled signals as those seen in the observations. Conclusions. We find that long periods of decayless oscillations occurring in short loops could be the result of undersampling.

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2024-10-09
DOI
https://doi.org/10.1051/0004-6361/202451684/pdf
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
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article

Undersampling effects on observed periods of coronal oscillations

Springer Link (Chiba Institute of Technology)
Solar and Space Plasma Dynamics
article

Undersampling effects on observed periods of coronal oscillations

article en

Abstract

Context. Recent observations of decayless transverse oscillations have revealed two branches in the relationship between period and loop length. One is a linear relationship, interpreted as a standing mode, while the other shows almost no correlation and has not yet been interpreted conclusively. Aims. We investigated the undersampling effect on observed periods of decayless oscillations. Methods. We considered oscillating coronal loops that closely follow the observed loop length distribution. Assuming that all oscillations are standing waves, we modelled a signal that represents decayless oscillations where the period is proportional to the loop length and the amplitude and phase are randomly drawn. We generated a downsampled signal from the original signal by considering different sample rates that mimic temporal cadences of telescopes, and analysed the periods for sampled signals using the fast Fourier transform. Results. When the sampling cadence approaches the actual oscillation period, there is a greater tendency to overestimate the periods in short loops. We find the same two branches in the relationship between loop length and period of the sampled signals as those seen in the observations. Conclusions. We find that long periods of decayless oscillations occurring in short loops could be the result of undersampling.

Springer Link (Chiba Institute of Technology)
National Aeronautics and Space Administration, UK Space Agency, European Commission, Belgian Federal Science Policy Office, Centre National d’Etudes Spatiales, Fonds Wetenschappelijk Onderzoek, KU Leuven, China Scholarship Council, Latvijas Zinātnes Padome, Bundesministerium für Wirtschaft und Energie, Vlaamse regering, HORIZON EUROPE Framework Programme, Science and Technology Facilities Council
Openalex Percentile: Top 68%
Solar and Space Plasma Dynamics
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Undersampling effects on observed periods of coronal oscillations · Springer Link (Chiba Institute of Technology) (2024) | TGRS Research Map | TGRS