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Table 6

Expected radio emission on the exoplanet’s day and night sides for different IMF orientations (a = 0, b = 2 × 10−3) and magnetic axis tilts.

[P(DS)] (105 W)
       
Model Bx Bxneg By Byneg Bz Bzneg
tilt30 55.1 19.6 87.3 80.1 7.36 49.9
tilt60 74.6 32.4 81.5 82.0 2.94 4.06
tilt90 18.7 57.6 10.8 7.87 19.1 60.1

Model / B6000 [P(DS)] ratio
             
Model Bx Bxneg By Byneg Bz Bzneg
tilt30 12.7 6.66 2.49 2.46 0.5 0.69
tilt60 17.2 7.70 2.33 2.52 0.20 0.06
tilt90 4.34 13.7 0.31 0.24 1.30 0.83

[P(NS)] (105 W)
             
Model Bx Bxneg By Byneg Bz Bzneg
tilt30 70.7 72.8 95 108 48.9 108
tilt60 98.3 89.8 114 119 62.1 192

XModel / B6000 [P(NS)] ratio
             
Model Bx Bxneg By Byneg Bz Bzneg
tilt30 6.93 7.14 6.01 6.59 6.31 5.29
tilt60 9.64 8.80 7.21 7.26 8.01 9.41

Notes. Results for an exoplanet with a radius of Rex = 2440 km.

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