International audienceThe Rosetta spacecraft rendezvoused with comet 67P/Churyumov-Gerasimenko in August 2014 and escorted it for two years until September 2016. The plasma surrounding the comet was probed by the Rosetta Plasma Consortium (RPC), comprising five instruments. The Langmuir Probe (RPC/LAP; Engelhardt et al., 2018) and Mutual Impedance Probe (RPC/MIP; Wattieaux et al, 2020; Gilet et al., 2020) measured a cold population of electrons ( 3 x 1027 s-1). However, the cold population was observed at large heliocentric distances (> 3.5 au) and very weak outgassing rates (Q < 1026 s-1).We have developed the first 3D collisional model of electrons at a comet, featuring a spherically symmetric coma of pure water. Electric and magnetic fie...
International audienceIn the ionosphere of the comet 67P/Churyumov-Gerasimenko, the Rosetta Plasma C...
Context. The Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboard the Rosetta...
International audienceThe Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboar...
International audienceThe Rosetta Mission rendezvoused with comet 67P/Churyumov-Gerasimenko in Augus...
virtual meetingInternational audienceThe plasma instruments, Mutual Impedance Probe (MIP) and Langmu...
International audienceContext. The electron temperature of the plasma is one important aspect of the...
International audienceCometary electrons are born at typical energies of order 10 eV, but can cool t...
We have developed the first 3D collisional model of electrons at a comet, which we use to examine th...
International audienceWe have developed the first 3D collisional model of electrons at a comet, whic...
International audienceWe examine the origin of electrons in a weakly outgassing comet, using Rosetta...
International audienceThe Rosetta spacecraft escorted comet 67P/Churyumov-Gerasimenko for two years ...
International audienceThe Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboar...
International audienceContext. Strong electron cooling on the neutral gas in cometary comae has been...
International audienceContext. Strong electron cooling on the neutral gas in cometary comae has been...
International audienceIn the ionosphere of the comet 67P/Churyumov-Gerasimenko, the Rosetta Plasma C...
Context. The Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboard the Rosetta...
International audienceThe Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboar...
International audienceThe Rosetta Mission rendezvoused with comet 67P/Churyumov-Gerasimenko in Augus...
virtual meetingInternational audienceThe plasma instruments, Mutual Impedance Probe (MIP) and Langmu...
International audienceContext. The electron temperature of the plasma is one important aspect of the...
International audienceCometary electrons are born at typical energies of order 10 eV, but can cool t...
We have developed the first 3D collisional model of electrons at a comet, which we use to examine th...
International audienceWe have developed the first 3D collisional model of electrons at a comet, whic...
International audienceWe examine the origin of electrons in a weakly outgassing comet, using Rosetta...
International audienceThe Rosetta spacecraft escorted comet 67P/Churyumov-Gerasimenko for two years ...
International audienceThe Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboar...
International audienceContext. Strong electron cooling on the neutral gas in cometary comae has been...
International audienceContext. Strong electron cooling on the neutral gas in cometary comae has been...
International audienceIn the ionosphere of the comet 67P/Churyumov-Gerasimenko, the Rosetta Plasma C...
Context. The Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboard the Rosetta...
International audienceThe Mutual Impedance Probe (MIP) of the Rosetta Plasma Consortium (RPC) onboar...