dorsal/arxiv
View SchemaExact solutions for magnetic annihilation in curvilinear geometry
| Authors | E. Tassi, V. S. Titov, G. Hornig |
|---|---|
| Categories | |
| ArXiv ID | physics/0212017 |
| URL | https://arxiv.org/abs/physics/0212017 |
| DOI | 10.1016/S0375-9601(02)01174-X |
| Journal | Physics Letters A 302 (5-6) (2002) pp. 313-317 |
Abstract
New exact solutions of the steady and incompressible 2D MHD equations in polar coordinates are presented. The solutions describe the process of reconnective magnetic annihilation in a curved current layer. They are particularly interesting for modeling magnetic reconnection in solar flares caused by the interaction of three photospheric magnetic sources.
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"abstract": "New exact solutions of the steady and incompressible 2D MHD equations in\npolar coordinates are presented. The solutions describe the process of\nreconnective magnetic annihilation in a curved current layer. They are\nparticularly interesting for modeling magnetic reconnection in solar flares\ncaused by the interaction of three photospheric magnetic sources.",
"arxiv_id": "physics/0212017",
"authors": [
"E. Tassi",
"V. S. Titov",
"G. Hornig"
],
"categories": [
"physics.plasm-ph",
"physics.space-ph"
],
"doi": "10.1016/S0375-9601(02)01174-X",
"journal_ref": "Physics Letters A 302 (5-6) (2002) pp. 313-317",
"title": "Exact solutions for magnetic annihilation in curvilinear geometry",
"url": "https://arxiv.org/abs/physics/0212017"
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