Great ellipse explained

right|150px|thumb|A spheroid

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.[1] For points that are separated by less than about a quarter of the circumference of the earth, about

10000km

, the length of the great ellipse connecting the points is close (within one part in 500,000) to the geodesic distance.[2] [3] [4] 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

a

and polar semi-axis

b

. Define the flattening

f=(a-b)/a

, the eccentricity

e=\sqrt{f(2-f)}

, and the second eccentricity

e'=e/(1-f)

. Consider two points:

A

at (geographic) latitude

\phi1

and longitude

λ1

and

B

at latitude

\phi2

and longitude

λ2

. The connecting great ellipse (from

A

to

B

) has length

s12

and has azimuths

\alpha1

and

\alpha2

at the two endpoints.

There are various ways to map an ellipsoid into a sphere of radius

a

in such a way as to map the great ellipse into a great circle, allowing the methods of great-circle navigation to be used:

\phi

on the ellipsoid to a point on the sphere with latitude

\beta

, the parametric latitude.

\phi

on the ellipsoid to a point on the sphere with latitude

\theta

, the geocentric latitude.

a2/b

and then mapped radially onto the sphere; this preserves the latitude - the latitude on the sphere is

\phi

, the geographic latitude.

The last method gives an easy way to generate a succession of way-points on the great ellipse connecting two known points

A

and

B

. Solve for the great circle between

(\phi1,λ1)

and

(\phi2,λ2)

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.[5] In detail, the mapping is as follows (this description is taken from [6]):

\phi

on the ellipsoid maps to the parametric latitude

\beta

on the sphere, where

a\tan\beta=b\tan\phi.

λ

is unchanged.

\alpha

on the ellipsoid maps to an azimuth

\gamma

on the sphere where

\begin{align} \tan\alpha&=

\tan\gamma
\sqrt{1-e2\cos2\beta
}, \\\tan\gamma &= \frac,\end
and the quadrants of

\alpha

and

\gamma

are the same.

a

are parametrized by arc length

\sigma

measured from the northward crossing of the equator. The great ellipse has a semi-axes

a

and

a\sqrt{1-e2\cos

2\gamma
0}
, where

\gamma0

is the great-circle azimuth at the northward equator crossing, and

\sigma

is the parametric angle on the ellipse.

(A similar mapping to an auxiliary sphere is carried out in the solution of geodesics on an ellipsoid. The differences are that the azimuth

\alpha

is conserved in the mapping, while the longitude

λ

maps to a "spherical" longitude

\omega

. The equivalent ellipse used for distance calculations has semi-axes

b\sqrt{1+e'2\cos

2\alpha
0}
and

b

.)

Solving the inverse problem

The "inverse problem" is the determination of

s12

,

\alpha1

, and

\alpha2

, given the positions of

A

and

B

. This is solved by computing

\beta1

and

\beta2

and solving for the great-circle between

(\beta1,λ1)

and

(\beta2,λ2)

.

The spherical azimuths are relabeled as

\gamma

(from

\alpha

). Thus

\gamma0

,

\gamma1

, and

\gamma2

and the spherical azimuths at the equator and at

A

and

B

. The azimuths of the endpoints of great ellipse,

\alpha1

and

\alpha2

, are computed from

\gamma1

and

\gamma2

.

The semi-axes of the great ellipse can be found using the value of

\gamma0

.

Also determined as part of the solution of the great circle problem are the arc lengths,

\sigma01

and

\sigma02

, measured from the equator crossing to

A

and

B

. The distance

s12

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 (instead of for the meridian) and substitute

\sigma01

and

\sigma02

for

\beta

.

The solution of the "direct problem", determining the position of

B

given

A

,

\alpha1

, and

s12

, can be similarly be found (this requires, in addition, the inverse meridian distance formula). This also enables way-points (e.g., a series of equally spaced intermediate points) to be found in the solution of the inverse problem.

See also

External links

Notes and References

  1. .
  2. 10.1007/BF02521760. The direct and inverse solutions for the great elliptic line on the reference ellipsoid. Bulletin Géodésique. 58. 1. 101 - 108. 1984. Bowring . B. R.. 1984BGeod..58..101B. 123161737.
  3. 10.1017/S0373463300013333. The Great Ellipse on the Surface of the Spheroid. Journal of Navigation. 49. 2. 229 - 234. 1996. Williams . R. . 1996JNav...49..229W.
  4. 10.1017/S0373463399008516. The Great Ellipse Solution for Distances and Headings to Steer between Waypoints. Journal of Navigation. 52. 3. 421 - 424. 1999. Walwyn . P. R.. 1999JNav...52..421W.
  5. 10.2478/v10156-011-0040-9. Solutions to the direct and inverse navigation problems on the great ellipse. Journal of Geodetic Science. 2. 3. 2012c. 200 - 205. Sjöberg . L. E.. 2012JGeoS...2..200S. free.
  6. Web site: 2014. Great ellipses. Karney . C. F. F.. . From the documentation of GeographicLib 1.38..