Effect of the exoplanet magnetic field topology on its magnetospheric radio emission

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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

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

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