Abstract
This paper treats the prominence model of Low (1993) to examine more
complicated sheet currents than those used in the original model.
Nonlinear force-free field solutions, in Cartesian coordinates,
invariant in a given direction, are presented to show the possibility of
an inverse-polarity prominence embedded in a large twisted flux tube.
The force-free solution is matched to an external, unsheared, potential
coronal magnetic field. These new solutions are mathematically
interesting and allow an investigation of different profiles of the
current intensity, magnetic field vector and mass density in the sheet.
These prominence models show a general increase in magnetic field
strength with height in agreement with observations. Other prominence
properties are shown to match the observed values.
Original language | English |
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Pages (from-to) | 223-249 |
Journal | Solar Physics |
Volume | 157 |
DOIs | |
Publication status | Published - 1 Mar 1995 |
Keywords
- Current Sheets
- Magnetic Flux
- Mathematical Models
- Solar Physics
- Solar Prominences
- Sun
- Force-Free Magnetic Fields
- Polarity
- Solar Corona
- Solar Magnetic Field