Astronomy and astrophysics Definition
Parker spiral
Builds on Alfvén's frozen-in flux theoremParker solar wind model
Definition
Let a star rotate with constant angular velocity about the -axis, and use spherical coordinates in an inertial frame centred on the star. Assume that beyond a sphere of radius the plasma moves radially with a constant speed , as in the Parker solar wind model. Assume that the magnetic field is frozen into the plasma. Let a field line be anchored at the point of the sphere with colatitude that has longitude at time . The Parker spiral through this footpoint at time is the curve
Remarks
The plasma that sits at radius at time left the footpoint at time , when the footpoint had longitude ; this gives the formula. At fixed , is an affine function of , so the curve is an Archimedean spiral, and its turns are spaced by in . The field components are and , so the angle between the field and the radial direction satisfies .
Example: for the Sun, per second, and at the Earth kilometres with kilometres per second. Then , so degrees in the equatorial plane.
Non-example: a logarithmic spiral is not a Parker spiral, because the distance between its successive turns grows with instead of staying equal to .
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- Line integral as an integral over the parameter interval statement
- Central force definition
- Orientable surface definition
- Gradient theorem statement
- Newton's law of universal gravitation statement
- Flux through a surface definition
- Parker solar wind model statement
- Divergence theorem statement
- Generalised Stokes theorem statement
- Stokes' theorem statement
- Alfvén's frozen-in flux theorem statement
- Parker spiral definition
Further reading
About this page
| Tag | WQRDJYHEW5 |
|---|---|
| URI | m2://WQRDJYHEW5 |
| Kind | definition |
| Writing | W0 stub |
| MSC | 85A30, 76W05 |
| Defines | Parker spiral |
| Uses | Alfvén's frozen-in flux theorem, Parker solar wind model |
| Changed | 3 November 2026 |
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