Atmospheric escape processes and planetary atmospheric evolution
The habitability of the surface of any planet is determined by a complex evolution of its
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive …
Laboratory evidence for proton energization by collisionless shock surfing
Charged particles can be accelerated to high energies by collisionless shock waves in
astrophysical environments, such as supernova remnants. By interacting with the …
astrophysical environments, such as supernova remnants. By interacting with the …
The Impact of Radial and Non‐Radial IMF on the Earth's Magnetopause Size, Shape, and Dawn‐Dusk Asymmetry From Global 3D Kinetic Simulations
SM Baraka, O Le Contel, L Ben‐Jaffel… - Journal of …, 2021 - Wiley Online Library
The boundary between the solar wind and the Earth's magnetosphere, the magnetopause
(MP), is highly dynamic. Its location and shape depend on SW dynamic pressure and …
(MP), is highly dynamic. Its location and shape depend on SW dynamic pressure and …
The impact of Radial and Quasi-Radial IMF on the Earth's Magnetopause Size and Shape, and Dawn-Dusk Asymmetry from Global 3D Kinetic Simulations
S Baraka - Authorea Preprints, 2022 - authorea.com
The boundary between the solar wind (SW) and the Earth's magnetosphere, named the
magnetopause (MP), is highly dynamic. Its location and shape can vary as a function of …
magnetopause (MP), is highly dynamic. Its location and shape can vary as a function of …
Laser-driven shocks of astrophysical interest
A Fazzini - 2022 - theses.hal.science
The huge progress made over the last decades in the development of high-power lasers has
allowed the access, in the laboratory, to extreme physical conditions of astrophysical …
allowed the access, in the laboratory, to extreme physical conditions of astrophysical …