Hansen's problem

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In trigonometry, Hansen's problem is a problem in planar surveying, named after the astronomer Peter Andreas Hansen (1795–1874), who worked on the geodetic survey of Denmark. There are two known points Template:Mvar, and two unknown points Template:Math. From Template:Math and Template:Math an observer measures the angles made by the lines of sight to each of the other three points. The problem is to find the positions of Template:Math and Template:Math. See figure; the angles measured are Template:Math.

Since it involves observations of angles made at unknown points, the problem is an example of resection (as opposed to intersection).

Solution method overview

Define the following angles: γ=∠P1AP2,δ=∠P1BP2,ϕ=∠P2AB,ψ=∠P1BA. As a first step we will solve for Template:Mvar and Template:Mvar. The sum of these two unknown angles is equal to the sum of Template:Math and Template:Math, yielding the equation

ϕ+ψ=β1+β2.

A second equation can be found more laboriously, as follows. The law of sines yields

AB‾P2B‾=sin⁡α2sin⁡ϕ,P2B‾P1P2‾=sin⁡β1sin⁡δ.

Combining these, we get

AB‾P1P2‾=sin⁡α2sin⁡β1sin⁡ϕsin⁡δ.

Entirely analogous reasoning on the other side yields

AB‾P1P2‾=sin⁡α1sin⁡β2sin⁡ψsin⁡γ.

Setting these two equal gives

sin⁡ϕsin⁡ψ=sin⁡γsin⁡α2sin⁡β1sin⁡δsin⁡α1sin⁡β2=k.

Using a known trigonometric identity this ratio of sines can be expressed as the tangent of an angle difference:

tan⁡12(ϕ−ψ)=k−1k+1tan⁡12(ϕ+ψ).

Where k=sin⁡ϕsin⁡ψ.

This is the second equation we need. Once we solve the two equations for the two unknowns Template:Mvar, we can use either of the two expressions above for AB‾P1P2‾ to find Template:Tmath since Template:Overline is known. We can then find all the other segments using the law of sines.[1]

Solution algorithm

We are given four angles Template:Math and the distance Template:Overline. The calculation proceeds as follows:

  • Calculate γ=π−α1−β1−β2,δ=π−α2−β1−β2.
  • Calculate k=sin⁡γsin⁡α2sin⁡β1sin⁡δsin⁡α1sin⁡β2.
  • Let s=β1+β2,d=2arctan⁡(k−1k+1tan⁡12s) and then ϕ=s+d2,ψ=s−d2.

Calculate P1P2‾=AB‾ sin⁡ϕsin⁡δsin⁡α2sin⁡β1 or equivalently P1P2‾=AB‾ sin⁡ψsin⁡γsin⁡α1sin⁡β2. If one of these fractions has a denominator close to zero, use the other one.

See also

References

Template:Reflist

  1. ↑ Udo Hebisch: Ebene und Sphaerische Trigonometrie, Kapitel 1, Beispiel 4 (2005, 2006)[1] Template:Webarchive