activity
20182023
most citedIon velocity and electron temperature inside and around the diamagnetic cavity of comet 67P

47 citations · 140 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2023

The source of electrons at comet 67P

P. Stephenson, A. Beth, J. Deca +8

We examine the origin of electrons in a weakly outgassing comet, using Rosetta mission data and a 3D collisional model of electrons at a comet. We have calculated a new dataset of…

astro-ph.EP2019★ 11 cited

The evolution of the electron number density in the coma of comet 67P at the location of Rosetta from 2015 November through 2016 March

Erik Vigren, Niklas J. T. Edberg, Anders I. Eriksson +6

A comet ionospheric model assuming the plasma to move radially outward with the same bulk speed as the neutral gas and not being subject to severe reduction through dissociative re…

physics.space-ph2018★ 42 cited

Solar wind interaction with comet 67P: impacts of corotating interaction regions

Niklas J. T. Edberg, A. I. Eriksson, E. Odelstad +18

We present observations from the Rosetta Plasma Consortium of the effects of stormy solar wind on comet 67P/Churyumov-Gerasimenko. Four corotating interaction regions (CIRs), where…

physics.space-ph2018★ 47 cited

Ion velocity and electron temperature inside and around the diamagnetic cavity of comet 67P

Elias Odelstad, Anders I. Eriksson, Fredrik L. Johansson +7

A major point of interest in cometary plasma physics has been the diamagnetic cavity, an unmagnetized region in the inner-most part of the coma. Here, we combine Langmuir and Mutua…

astro-ph.EP2018★ 7 cited

Solar wind dynamics around a comet: The paradigmatic inverse-square-law model

Melaine Saillenfest, Benoît Tabone, Etienne Behar

Aims. Observations of solar protons near comet 67P/Churyumov-Gerasimenko (67P) by the Rosetta spacecraft can be modelled by the planar motion in an effective magnetic field proport…

astro-ph.EP2018★ 33 cited

Solar wind dynamics around a comet - A 2D semi-analytical kinetic model

E. Behar, B. Tabone, M. Saillenfest +5

We aim at analytically modelling the solar wind proton trajectories during their interaction with a partially ionised cometary atmosphere, not in terms of bulk properties of the fl…