RPC-MIP observations at comet 67P/Churyumov-Gerasimenko explained by a model including a sheath and two populations of electrons

¹ Laboratoire Plasma et Conversion d’Energie (LAPLACE), Université de Toulouse, CNRS, 31062 Toulouse, France
e-mail: gaetan.wattieaux@laplace.univ-tlse.fr
² Laboratoire de Physique et Chimie de l’Environnement et de l’Espace (LPC2E), CNRS, 45071 Orléans, France

Received: 14 December 2018
Accepted: 2 March 2019

Abstract

The response of the mutual impedance probe RPC-MIP on board Rosetta orbiter electrostatically modeled considering an unmagnetized and collisionless plasma with two Maxwellian electron populations. A vacuum sheath surrounding the probe was considered in our model in order to take the ion sheath into account that is located around the probe, which is immersed in the cometary plasma. For the first time, the simulated results are consistent with the data collected around comet 67P/Churyumov-Gerasimenko (67P), but strong discrepancies were identified with the previous simulations that neglected the plasma sheath around the probe. We studied the influence of the sheath thickness and of the electron populations. This work helps to better understand the initially unexpected responses of the mutual impedance probe that were acquired during the Rosetta mission. It suggests that two electron populations exist in the cometary plasma of 67P.