Math 2.0

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 Ω>0\Omega > 0 about the zz-axis, and use spherical coordinates (r,θ,ϕ)(r, \theta, \phi) in an inertial frame centred on the star. Assume that beyond a sphere of radius r0r_0 the plasma moves radially with a constant speed v>0v > 0, 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 r=r0r = r_0 with colatitude θ0\theta_0 that has longitude ϕ0+Ωt\phi_0 + \Omega t at time tt. The Parker spiral through this footpoint at time tt is the curve θ=θ0,ϕ=ϕ0+Ωt−Ωv(r−r0),r≥r0.\theta = \theta_0, \qquad \phi = \phi_0 + \Omega t - \frac{\Omega}{v} (r - r_0), \qquad r \ge r_0.

Remarks

The plasma that sits at radius rr at time tt left the footpoint at time t′=t−(r−r0)/vt' = t - (r - r_0)/v, when the footpoint had longitude ϕ0+Ωt′\phi_0 + \Omega t'; this gives the formula. At fixed tt, rr is an affine function of ϕ\phi, so the curve is an Archimedean spiral, and its turns are spaced by 2πv/Ω2\pi v/\Omega in rr. The field components are Br=B0(r0/r)2B_r = B_0 (r_0/r)^2 and Bϕ=−Br Ω(r−r0)sin⁡θ/vB_\phi = -B_r \, \Omega (r - r_0) \sin\theta / v, so the angle ψ\psi between the field and the radial direction satisfies tan⁡ψ=Ω(r−r0)sin⁡θ/v\tan\psi = \Omega (r - r_0) \sin\theta / v.

Example: for the Sun, Ω≈2.7×10−6\Omega \approx 2.7 \times 10^{-6} per second, and at the Earth r≈1.5×108r \approx 1.5 \times 10^{8} kilometres with v≈400v \approx 400 kilometres per second. Then Ωr/v≈1\Omega r / v \approx 1, so ψ≈45\psi \approx 45 degrees in the equatorial plane.

Non-example: a logarithmic spiral r=r0ebϕr = r_0 e^{b\phi} is not a Parker spiral, because the distance between its successive turns grows with rr instead of staying equal to 2πv/Ω2\pi v/\Omega.

Reading path

To understand this page from the ground up, read these 96 pages in order. The foundations come first.

  1. Critical point concept
  2. Derivative concept
  3. Differential equation concept
  4. Euclidean space object
  5. Euclidean vector concept
  6. Euler equations concept
  7. Function concept
  8. Function composition concept
  9. Ideal MHD equations concept
  10. Infimum concept
  11. Interval concept
  12. Magnetohydrodynamics concept
  13. Ordinary differential equation concept
  14. Speed of sound concept
  15. Supremum concept
  16. Velocity concept
  17. Fréchet derivative definition
  18. Total derivative concept
  19. Cross product definition
  20. Ordinary differential equation definition
  21. Function of several variables concept
  22. Vector-valued function concept
  23. Lipschitz condition definition
  24. Classical mechanics concept
  25. Jordan measure definition
  26. Differentiable function of several variables concept
  27. Limit of a function of several variables concept
  28. Momentum concept
  29. Parametrised curve concept
  30. Vector field concept
  31. Iterated integral definition
  32. Partial derivative concept
  33. Solution of an ordinary differential equation definition
  34. Inertial frame of reference concept
  35. Continuity in R^n definition
  36. Differentiable function of several variables definition
  37. Gradient concept
  38. Partial derivative definition
  39. Curl concept
  40. Divergence concept
  41. Initial value problem definition
  42. Newton's laws of motion statement
  43. Differentiable on an open set definition
  44. Double integral definition
  45. Chain rule in several variables statement
  46. Higher partial derivatives definition
  47. Gradient definition
  48. Jacobian matrix definition
  49. Picard–Lindelöf hypotheses definition
  50. Iterated derivative definition
  51. Fubini's theorem statement
  52. Chain rule for a composition with a curve statement
  53. Triple integral definition
  54. Picard operator definition
  55. C^k function characterised by continuous derivatives statement
  56. An iterate of the Picard operator is a contraction statement
  57. Integral equation form of an initial value problem statement
  58. Differential form definition
  59. Parametrised curve definition
  60. Vector field definition
  61. Picard–Lindelöf theorem statement
  62. Wedge product of forms definition
  63. Closed curve definition
  64. Rectifiable curve definition
  65. Parametrised surface definition
  66. Conservative vector field definition
  67. Curl definition
  68. Divergence definition
  69. Tangent vector of a curve definition
  70. Classical mechanics definition
  71. Line integral of a scalar field definition
  72. Line integral of a vector field definition
  73. Tangent plane and normal vector of a surface definition
  74. Momentum definition
  75. Potential energy definition
  76. Regular curve definition
  77. Green's theorem statement
  78. One-form definition
  79. Angular momentum definition
  80. Surface area definition
  81. Arc length parametrisation definition
  82. Divergence theorem on a rectangle in the plane statement
  83. Surface integral definition
  84. Exterior derivative definition
  85. Line integral as an integral over the parameter interval statement
  86. Central force definition
  87. Orientable surface definition
  88. Gradient theorem statement
  89. Newton's law of universal gravitation statement
  90. Flux through a surface definition
  91. Parker solar wind model statement
  92. Divergence theorem statement
  93. Generalised Stokes theorem statement
  94. Stokes' theorem statement
  95. Alfvén's frozen-in flux theorem statement
  96. Parker spiral definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Heliospheric_current_sheet
About this page
TagWQRDJYHEW5
URIm2://WQRDJYHEW5
Kinddefinition
WritingW0 stub
MSC85A30, 76W05
DefinesParker spiral
UsesAlfvén's frozen-in flux theorem, Parker solar wind model
Changed3 November 2026

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