Abstract
The concept of hyperbolic flux tubes (HFTs) is a generalization of the concept of separator field lines for coronal magnetic fields with a trivial magnetic topology. An effective mechanism of a current layer formation in HFTs is proposed. This mechanism is called magnetic pinching, and it is caused by large-scale shearing motions applied to the photospheric feet of HFTs in a way as if trying to twist the HFT. It is shown that in the middle of an HFT such motions produce a hyperbolic flow that causes an exponentially fast growth of the current density in a thin force-free current layer. The magnetic energy associated with the current layer that is built up over a few hours is sufficient for a large are. Other implications of HFT pinching for solar flares are discussed as well.
| Original language | English |
|---|---|
| Pages (from-to) | 1172-1189 |
| Number of pages | 18 |
| Journal | Astrophysical Journal |
| Volume | 582 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 10 Jan 2003 |
Keywords
- MHD
- Sun : corona
- Sun : flares
- Sun : magnetic fields
- QUASI-SEPARATRIX LAYERS
- CURRENT SHEETS
- SOLAR-FLARES
- PARTICLE-ACCELERATION
- ACTIVE REGIONS
- RECONNECTION
- FIELDS
- POINTS
- FLOWS
- MODEL
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