Transformation of solar wind energy and helicity spectra in the frame of magnetohydrodynamics shell modeling

arXiv:2606.17351 · astro-ph.SR · Submitted 2026-06-15 · Read on arXiv

I. Dukanov, E. Yushkov, P. Frick, D. Sokoloff

astro-ph.SR

Submitted: 2026-06-15

Comments: Received 26 November, 2025 Revised 20 March, 2026 Accepted 16 April, 2026 Published 12 May, 2026

Journal ref: Phys. Rev. E 113, 055208, Published 12 May, 2026, Vol. 113, Iss. 5, May 2026

DOI: 10.1103/9wh1-7ntq

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

Terminology

• Conservation Laws — 5× in this paper · explained in 3 episodes
• Anisotropy — 2× in this paper · explained in 3 episodes
• Initial Data — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Degeneracy — 1× in this paper · explained in 3 episodes
• Homogeneity — 1× in this paper · explained in 2 episodes
• Magnetohydrodynamics (MHD) — 1× in this paper · explained in 3 episodes
• PSP Solar Wind Electrons Alphas and Protons — 1× in this paper
• alpha — 1× in this paper · explained in 1 episode

Sources

• Galactic foreground and CMB emissions randomization due to chaotic/turbulent dynamics of magnetized plasma dominated by magnetic helicity

Related papers

• HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
• Effect of Neutron Star Jets on Common Envelope Evolution
• Constraining the origin of magnetic white dwarfs
• JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
• Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
• Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?