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Table 3
Planetary and upper atmosphere input parameters at the height R0 η = 15%,η = 40% where the Kn = 0.1, as the starting point for the DSMC-code simulations for two heating efficiencies η = 15% and 40%.
| Exoplanet | R0 η = 15% [Rpl] | nη = 15% [cm-3] | Tη = 15% [K] | vflow η = 15% [km s-1] | R0 η = 40% [Rpl] | nη = 40% [cm-3] | Tη = 40% [K] | vflow η = 40% [km s-1] |
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| Kepler-11b | 6.7 | 7 × 105 | 1440 | 2.3 | 6.7 | 8.2 × 105 | 2230 | 4.0 |
| Kepler-11c | 5.0 | 1 × 106 | 1833 | 0.78 | 6.5 | 4.8 × 105 | 2582 | 1.7 |
| Kepler-11d | 6.4 | 5 × 105 | 1000 | 0.96 | 7.0 | 5.5 × 105 | 1453 | 2.1 |
| Kepler-11e | 6.5 | 4 × 105 | 770 | 0.75 | 7.5 | 3.78 × 105 | 1234 | 1.7 |
| Kepler-11f | 18 | 3.2 × 105 | 761 | 1.6 | 22 | 2.0 × 105 | 397 | 2.8 |
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