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

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 4.

Scatter plots between period and loop length of decayless oscillations analysed in the current work (CW) and previous studies (from top to bottom in the legend; Wang et al. 2012; Nisticò et al. 2013; Anfinogentov et al. 2013, 2015; Duckenfield et al. 2018; Anfinogentov & Nakariakov 2019; Gao et al. 2022; Zhong et al. 2022a, 2022b, 2023a; Mandal et al. 2022; Li & Long 2023; Petrova et al. 2023; Shrivastav et al. 2024). The scatter plots for ARs (middle panel) and QS (right panel) are presented in log scales.

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