Table 1
Fitted power-law coefficients α, normalised likelihood ratio R, corresponding p-value, and lower bound for the inertial range x1 for the cumulative distribution flare energy subsets.
| α | R | p-value | x1 [log erg] | |
|---|---|---|---|---|
| Simple flares | 2.08 ± 0.10 | −0.59 | 0.56 | 32.9 |
| Complex flare components | 2.24 ± 0.09 | −0.59 | 0.56 | 32.7 |
| Partially convective stars | 2.32 ± 0.16 | −0.51 | 0.61 | 33.1 |
| Fully convective stars | 2.18 ± 0.09 | −0.09 | 0.93 | 32.8 |
| All stars | 2.06 ± 0.06 | −1.27 | 0.21 | 32.7 |
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.