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Fig. 1. | Earth, Planets and Space

Fig. 1.

From: Upper ionosphere of Mars is not axially symmetrical

Fig. 1.

From top to bottom: (a) height profiles of the electron number density measured by MARSIS, blue and red symbols correspond to the measurements made on the inbound and outbound orbital legs, respectively; (b) solar zenith angles (solid curves) and the value of the model crustal magnetic field; (c) fluxes of 20ā€“40 eV electrons. Dashed vertical lines show the positions of the induced magnetospheric boundary on inbound and oubound orbital pathes determined from the drop of fluxes of the magnetosheath-like electrons.

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