Irreversibility and Energy Transfer at Non-MHD Scales in a Magnetospheric Current Disruption Event
Irreversibility and the processes occurring at ion and sub-ion scales are key challenges in understanding energy dissipation in non-collisional space plasmas. Recent advances have significantly improved the characterization of irreversibility and energy transfer across scales in turbulent fluid-like media, using high-order correlation functions and testing the validity of certain fluctuation relations. In this study, we explore irreversibility at non-MHD scales during a magnetospheric current disruption event. Our approach involves analyzing the asymmetric correlation function, assessing the validity of a fluctuation relation, and investigating delayed coupling between different scales to reveal evidence of a cascading mechanism. The results clearly demonstrate the irreversible nature of fluctuations at ion and sub-ion scales. Additionally, we provide potential evidence for an energy cascading mechanism occurring over short time delays.
Authors
- Giuseppe Consolini (ORCID: https://orcid.org/0000-0002-3403-647X)
- Paola De Michelis (ORCID: https://orcid.org/0000-0002-2708-0739)
Institutions
- Istituto Nazionale di Geofisica e Vulcanologia (IT)
- Institute for Space Astrophysics and Planetology (IT)
Publication Details
- Journal
- Entropy
- Published
- 2025-03-01
- DOI
- https://doi.org/10.3390/e27030260
- Citations
- 2
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- article
- Field-Weighted Citation Impact
- 2.31