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Table 5
Expected radio emission on the exoplanet’s day side for different IMF orientations (a = 0, b = 2 × 10−3) and exoplanet magnetic field intensities.
| [P(DS)] (105 W) | ||||||
|---|---|---|---|---|---|---|
| Model | Bx | Bxneg | By | Byneg | Bz | Bzneg |
| Q02 | 3.33 | 4.40 | 19.1 | 16.9 | 9.43 | 33.5 |
| Q04 | 26.6 | 51.3 | 63.9 | 55.6 | 42.1 | 44.6 |
| Model / B6000 [P(DS)] ratio | ||||||
| Model | Bx | Bxneg | By | Byneg | Bz | Bzneg |
| Q02 | 0.77 | 1.05 | 0.55 | 0.52 | 0.64 | 0.46 |
| Q04 | 6.13 | 12.2 | 1.83 | 1.71 | 2.86 | 0.61 |
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