Impact of the transport of magnetospheric electrons on the composition of the Triton atmosphere

Open Access

Fig. 6

Method used to couple our photochemical model of the Triton atmosphere and the electron transport code TRANSPlanets. R_i is the ionosphere radius, $‖ \vec{B} ‖$ $\left\| {\vec B} \right\|$ is the strength of the magnetic field at Triton, and m_orb is the orbital scaling factor.

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