Imaging Errors in telescopes, Seidel Theory

(after H. Nicklas, Optical Telescopes and Instrumentation, p. 59-136 in GD Roth ..)

Seidel (1821-96)

n_nu    refractive index
h_nu    incidence height
s_nu    intersect width
r_nu    curvature
d_nu    surface distance

  Abbe Invariant:
  Q_nu = n_nu (1/r_nu - 1/s_nu) = n'_nu (1/r'_nu - 1/s'_nu)

  Delta (1/ns)_nu = 1/(n'_nu * s'_nu) - 1/(n_nu * s_nu)

  h_nu/h_1 = (s_2 * s_3 * .. s_nu)/(s'_1 * s'_2 * .. s'_{nu-1})
           = Pi_j=2..nu (s_j/s'_{j-1})

  theta_nu = Sum_k=2..nu d_k/(n_k * (h_{k-1}/h_1) * (h_k/h_1)) - d_EP

  p_nu = 1/((h_nu/h_1)^2 * Q_nu) + theta_nu

  Petzval Sum:
  P_nu = - (1/r_nu) * (1/n'_nu - 1/n_nu)

Spherical Aberration
I_nu    = (h_nu/h_1)^4 Q_nu^2 Delta (1/ns)_nu

Coma
II_nu   = p_nu I_nu

Meridional astigmatism
III_nu  = 3 p_nu^2 I_nu + P_nu = 3 IIIa_nu + P_nu

Sagittal astigmatism
IV_nu   = p_nu^2 I_nu + P_nu = IIIa_nu + P_nu

Distortion
V_nu    = p_nu^3 I_nu + p_nu P_nu = p_nu (IIIa_nu + P_nu)

Astigmatic Difference
IIIa_nu = p_nu^2 I_nu = (III_nu - IV_nu)/2
                       
Mean Field Curvature
IVa_nu  = 2 p_nu^2 I_nu + P_nu = (III_nu + IV_nu)/2