From the 1 of 3 papers with an AI index.
- Centre of Plasma Physics - Institute for Plasma ResearchIN1 paper
- Earth-Life Science Institute1 paper
- Institute of Science Tokyo1 paper
- Institute of Solar-Terrestrial PhysicsRU1 paper
- Instituto de Astrofísica de AndalucíaES1 paper
- Keio UniversityJP1 paper
- Life Science InstituteJP1 paper
- The University of TokyoJP1 paper
- Tohoku UniversityJP1 paper
- Toronto Metropolitan UniversityCA1 paper
- UCLouvainBE1 paper
- University of WashingtonUS1 paper
3 papers
astro-ph.EP2026
Oxygen isotope fractionation in the Martian atmosphere induced by CO photolysis and O formation
Tatsuya Yoshida, Shohei Aoki, Hiromu Nakagawa +8
The paper presents a 1D photochemical model of the Martian atmosphere that quantifies oxygen isotope fractionation caused by CO₂ photolysis and ozone formation, matching observed i…
astro-ph.SR2026
Formation of Suprathermal Electron Populations in the Expanding, Turbulent Solar Wind
Maximilien Péters de Bonhome, Fabio Bacchini, Luca Pezzini +1
Nonthermal features are ubiquitously observed in electron velocity distribution functions in the solar wind, yet their origin in the collisionless, turbulent, expanding solar-wind…
physics.space-ph2026
High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields
Daniela Maci, Rony Keppens, Fabio Bacchini
The understanding and modeling of high-energy particles transport in turbulent magnetic fields is an important open question in space- and astrophysics. The multiscale, nonlinear n…