Menura: a code for simulating the interaction between a turbulent solar wind and solar system bodies
Etienne Behar, Shahab Fatemi, Pierre Henri, Mats Holmstrom

TL;DR
Menura is a novel numerical code that enables self-consistent, global simulations of the interaction between turbulent solar wind and solar system bodies, bridging planetary science and plasma physics.
Contribution
It introduces a new 2-step algorithm for simulating solar wind interactions with celestial bodies, advancing the integration of planetary science and plasma physics.
Findings
First example: solar wind interaction with a comet
Demonstrates the code's ability to model turbulence effects
Provides a foundation for future complex simulations
Abstract
Despite the close relationship between planetary science and plasma physics, few advanced numerical tools allow to bridge the two topics. The code Menura proposes a breakthrough towards the self-consistent modelling of these overlapping field, in a novel 2-step approach allowing for the global simulation of the interaction between a fully turbulent solar wind and various bodies of the solar system. This article introduces the new code and its 2-step global algorithm, illustrated by a first example: the interaction between a turbulent solar wind and a comet.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
