Three-dimensional solutions of the magnetohydrostatic equations for rigidly rotating magnetospheres in cylindrical coordinates

DOI10.1080/03091929.2017.1404594zbMath1499.76146arXiv1711.03755OpenAlexW2767755390WikidataQ114640110 ScholiaQ114640110MaRDI QIDQ5063511

No author found.

Publication date: 21 March 2022

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1711.03755

zbMATH Keywords

analytical solutionsmagnetohydrodynamicsthree-dimensional equilibriarotating magnetospheres

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05)

Uses Software

• DLMF

Cites Work

• Unnamed Item
• Unnamed Item
• Recent applications of fractional calculus to science and engineering
• Three-dimensional solutions of the magnetohydrostatic equations: rigidly rotating magnetized coronae in cylindrical geometry
• Stellar coronal magnetic fields and star-planet interaction
• A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum
• On fractional calculus and fractional multipoles in electromagnetism
• Three-dimensional analytical magnetohydrostatic equilibria of rigidly rotating magnetospheres in cylindrical geometry

This page was built for publication: Three-dimensional solutions of the magnetohydrostatic equations for rigidly rotating magnetospheres in cylindrical coordinates