Reconstruction of Interstellar Cosmic Ray Anisotropy via Heliospheric Propagation Modeling and SVD Inversion

arXiv:2610.18384 · astro-ph.HE, astro-ph.IM · Submitted 2026-10-13 · Read on arXiv

astro-ph.HE, astro-ph.IM

Submitted: 2026-10-13

Updated: 2026-10-13

Comments: Proceedings of the 36th Annual Wisconsin Space Conference

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Anisotropy — 1× in this paper · explained in 4 episodes

Related papers

• Accreting Neutron Stars in Low-Mass X-ray Binaries
• Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
• Impact of the equation of state on core collapse supernovae I: the low- T/W instability
• Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2
• Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
• Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants