Characteristics and energy flux distributions of decayless transverse oscillations depending on coronal regions

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 6.

Same as Figure 5 but for the oscillations including the decayless oscillations in this study and previous studies (Anfinogentov et al. 2013, 2015; Duckenfield et al. 2018; Gao et al. 2022; Zhong et al. 2022a,b; Petrova et al. 2023; Mandal et al. 2022; Li & Long 2023; Shrivastav et al. 2024). The oscillations from previous studies are the same as those listed in Table 1 in Lim et al. (2023). The power-law slopes are δ_QS = −1.56 ± 0.18, δ_AR = −1.20 ± 0.12, and δ_ALL = −1.31 ± 0.13, respectively.

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