activity
20102021
most citedDynamics of solar wind protons reflected by the Moon

52 citations · 107 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202135 cited

CME Magnetic Structure and IMF Preconditioning Affecting SEP Transport

Erika Palmerio, Emilia K. J. Kilpua, Olivier Witasse +15

Coronal mass ejections (CMEs) and solar energetic particles (SEPs) are two phenomena that can cause severe space weather effects throughout the heliosphere. The evolution of CMEs,…

astro-ph.EP202020 cited

Evolution of the Earth's Polar Outflow From Mid-Archean to Present

K. G. Kislyakova, C. P. Johnstone, M. Scherf +5

The development of habitable conditions on Earth is tightly connected to the evolution of its atmosphere which is strongly influenced by atmospheric escape. We investigate the evol…

astro-ph.EP2020

Stellar Driven Evolution of Hydrogen-Dominated Atmospheres from Earth-Like to Super-Earth-Type Exoplanets

K. G. Kislyakova, M. Holmström, H. Lammer +1

In the present chapter we present the results of evolutionary studies of exoplanetary atmospheres. We mostly focus on the sub- to super-Earth domain, although these methods are app…

astro-ph.EP2018

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

Mass-loading of the solar wind at 67P/Churyumov-Gerasimenko -- Observations and modelling

E. Behar, J. Lindkvist, H. Nilsson +4

Context. The first long-term in-situ observation of the plasma environment in the vicinity of a comet, as provided by the European Rosetta spacecraft. Aims. Here we offer character…

astro-ph.EP2018

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…