Fig. 6
Radio emission on the planet day side (A) and in reconnection region of the magnetotail on the planet night side (B) with radio efficiency parameters (a = 0, b = 2 × 10-3) for models with different IMF orientation and modules from 10 to 30 nT. The reference case without IMF is included. Bx orientations (black line), By orientations (red line) and Bz orientation (blue line).
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