Free Access
Table 3.
Estimated proton fluxes in pfu of observed stellar flares of the M-dwarf stars GJ876 (observed in June 2015, IX = 1.1 × 10−1 W m−2, see Youngblood et al. 2016), Proxima Centauri (observed in March 2016, IX = 6.02 W m−2, see Howard et al. 2018), and AD Leonis (observed in April 1989, IX = 9 W m−2, see Segura et al. 2010).
| Previous studies |
This work |
|||||||
|---|---|---|---|---|---|---|---|---|
| BE05 | BE07 | CL12 | RMA | Best case | DPL mean | Worst case | ||
| GJ876 | 3.88 × 106 | 1.10 × 104 | 5.86 × 106 | 8.07 × 104 | 8.93 × 104 | 1.26 × 107 | 1.45 × 109 | |
| Proxima Centauri | 3.72 × 108 | 4.41 × 105 | 3.40 × 109 | 3.67 × 106 | 1.78 × 107 | 1.23 × 1010 | 6.97 × 1012 | |
| ADLeonis | 5.88 × 108 | 6.41 × 105 | 6.45 × 109 | 5.39 × 106 | 3.03 × 107 | 2.45 × 1010 | 1.63 × 1013 | |
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.