Great ellipse


A great ellipse is an ellipse passing through two points on a spheroid and having the same center as that of the spheroid. Equivalently, it is an ellipse on the surface of a spheroid and centered on the origin, or the curve formed by intersecting the spheroid by a plane through its center.
For points that are separated by less than about a quarter of the circumference of the earth, about, the length of the great ellipse connecting the points is close to the geodesic distance.
The great ellipse therefore is sometimes proposed as a suitable route for marine navigation.
The great ellipse is special case of an earth section path.

Introduction

Assume that the spheroid, an ellipsoid of revolution, has an equatorial radius and polar semi-axis. Define the flattening, the eccentricity, and the second eccentricity. Consider two points: at latitude and longitude and at latitude and longitude. The connecting great ellipse has length and has azimuths and at the two endpoints.
There are various ways to map an ellipsoid into a sphere of radius in such a way as to map the great ellipse into a great circle, allowing the methods of great-circle navigation to be used:
The last method gives an easy way to generate a succession of way-points on the great ellipse connecting two known points and. Solve for the great circle between and and find the way-points on the great circle. These map into way-points on the corresponding great ellipse.

Mapping the great ellipse to a great circle

If distances and headings are needed, it is simplest to use the first of the mappings. In detail, the mapping is as follows :
The "inverse problem" is the determination of,, and, given the positions of and. This is solved by computing and and solving for the great-circle between and.
The spherical azimuths are relabeled as . Thus,, and and the spherical azimuths at the equator and at and. The azimuths of the endpoints of great ellipse, and, are computed from and.
The semi-axes of the great ellipse can be found using the value of.
Also determined as part of the solution of the great circle problem are the arc lengths, and, measured from the equator crossing to and. The distance is found by computing the length of a portion of perimeter of the ellipse using the formula giving the meridian arc in terms the parametric latitude. In applying this formula, use the semi-axes for the great ellipse and substitute and for.
The solution of the "direct problem", determining the position of given,, and, can be similarly be found. This also enables way-points to be found in the solution of the inverse problem.