Math 2.0

Geophysics Definition

Vincenty's formulae

Builds on Geodesics on an ellipsoidFlatteningGeodetic coordinates

Definition

Let an ellipsoid have semi-major axis aa, flattening ff and semi-minor axis b=(1−f)ab = (1 - f)a. Let two points have geodetic coordinates (φ1,L1)(\varphi_1, L_1) and (φ2,L2)(\varphi_2, L_2), and set L=L2−L1L = L_2 - L_1. Their reduced latitudes are Ui=arctan⁡((1−f)tan⁡φi)U_i = \arctan\big((1 - f)\tan\varphi_i\big). Vincenty's inverse method starts from λ=L\lambda = L and repeats the following steps until λ\lambda stops changing: sin⁡σ=(cos⁡U2sin⁡λ)2+(cos⁡U1sin⁡U2−sin⁡U1cos⁡U2cos⁡λ)2,\sin\sigma = \sqrt{(\cos U_2 \sin\lambda)^2 + (\cos U_1 \sin U_2 - \sin U_1 \cos U_2 \cos\lambda)^2}, cos⁡σ=sin⁡U1sin⁡U2+cos⁡U1cos⁡U2cos⁡λ,σ=atan2⁡(sin⁡σ,cos⁡σ),\cos\sigma = \sin U_1 \sin U_2 + \cos U_1 \cos U_2 \cos\lambda, \quad \sigma = \operatorname{atan2}(\sin\sigma, \cos\sigma), sin⁡α=cos⁡U1cos⁡U2sin⁡λsin⁡σ,cos⁡2σm=cos⁡σ−2sin⁡U1sin⁡U2cos⁡2α,\sin\alpha = \frac{\cos U_1 \cos U_2 \sin\lambda}{\sin\sigma}, \quad \cos 2\sigma_m = \cos\sigma - \frac{2\sin U_1 \sin U_2}{\cos^2\alpha}, C=f16cos⁡2α (4+f(4−3cos⁡2α)),C = \frac{f}{16}\cos^2\alpha\,\big(4 + f(4 - 3\cos^2\alpha)\big), λ=L+(1−C)fsin⁡α(σ+Csin⁡σ(cos⁡2σm+Ccos⁡σ(−1+2cos⁡22σm))).\lambda = L + (1 - C) f \sin\alpha \Big(\sigma + C\sin\sigma\big(\cos 2\sigma_m + C\cos\sigma(-1 + 2\cos^2 2\sigma_m)\big)\Big). With the final values, set u2=cos⁡2α (a2−b2)/b2u^2 = \cos^2\alpha \,(a^2 - b^2)/b^2 and A=1+u216384(4096+u2(−768+u2(320−175u2))),B=u21024(256+u2(−128+u2(74−47u2))),A = 1 + \frac{u^2}{16384}\Big(4096 + u^2\big(-768 + u^2(320 - 175u^2)\big)\Big), \quad B = \frac{u^2}{1024}\Big(256 + u^2\big(-128 + u^2(74 - 47u^2)\big)\Big), Δσ=Bsin⁡σ(cos⁡2σm+B4(cos⁡σ(−1+2cos⁡22σm)−B6cos⁡2σm(−3+4sin⁡2σ)(−3+4cos⁡22σm))).\Delta\sigma = B\sin\sigma\Big(\cos 2\sigma_m + \frac{B}{4}\Big(\cos\sigma(-1 + 2\cos^2 2\sigma_m) - \frac{B}{6}\cos 2\sigma_m(-3 + 4\sin^2\sigma)(-3 + 4\cos^2 2\sigma_m)\Big)\Big). The output distance is s=bA(σ−Δσ)s = bA(\sigma - \Delta\sigma). The azimuth at the first point is α1=atan2⁡(cos⁡U2sin⁡λ,cos⁡U1sin⁡U2−sin⁡U1cos⁡U2cos⁡λ)\alpha_1 = \operatorname{atan2}(\cos U_2 \sin\lambda, \cos U_1 \sin U_2 - \sin U_1 \cos U_2 \cos\lambda). Vincenty's direct method solves the direct problem with the same series and an iteration on σ\sigma.

Remarks

Example: for f=0f = 0 one gets C=0C = 0, so λ=L\lambda = L after one step, and u=0u = 0 gives A=1A = 1, B=0B = 0; then s=aσs = a\sigma is the great-circle distance. Non-example: for some nearly antipodal pairs of points, the iteration on λ\lambda does not converge, so the method gives no answer. The variable α\alpha is the azimuth of the geodesic where it crosses the equator, and σ\sigma is the arc length on the auxiliary sphere. If cos⁡2α=0\cos^2\alpha = 0, both points lie on the equator and the term with cos⁡2σm\cos 2\sigma_m is dropped.

Reading path

To understand this page from the ground up, read these 7 pages in order. The foundations come first.

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Each page uses the pages above it. The colour of the bar on a box shows how strong the evidence is, and the box also gives it as text. The list has the same pages.
  • no evidence level
  1. Flattening concept
  2. Geodesic concept
  3. Geodetic coordinates concept
  4. Great-circle distance concept
  5. Reference ellipsoid concept
  6. Geodesics on an ellipsoid problem
  7. Vincenty's formulae definition

Further reading

  1. Web https://en.wikipedia.org/wiki/Vincenty%27s_formulae, Inverse problem
About this page
TagMB8EPS233V
URIm2://MB8EPS233V
Kinddefinition
WritingW0 stub
MSC86A30, 53A05
DefinesVincenty's formulae
UsesGeodesics on an ellipsoid, Flattening, Geodetic coordinates
Changed3 November 2026

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