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{{for|the navigation on an ellipsoid|Geodesics on an ellipsoid}}
 
'''Great-circle navigation''' is the practice of [[navigation|navigating]] a vessel (a [[ship]] or [[aircraft]]) along a [[great circle]].  A great circle track is the shortest distance between two points on the surface of a sphere; the Earth isn't exactly spherical, but the formulas for a sphere are simpler and are often accurate enough for navigation (see the [[#A numerical example|numerical example]]).
 
==Course and distance==
 
[[File:Sphere geodesic 4sigma.svg|thumb|200px|right|Figure 1. The great circle path between (&phi;<sub>1</sub>,&nbsp;&lambda;<sub>1</sub>) and (&phi;<sub>2</sub>,&nbsp;&lambda;<sub>2</sub>).]]
The great circle path may be found using [[spherical trigonometry]]; this is the spherical version of the ''inverse geodesic problem''.
If a navigator begins at ''P''<sub>1</sub>&nbsp;=&nbsp;(&phi;<sub>1</sub>,&lambda;<sub>1</sub>) and plans to travel the great circle to a point at point ''P''<sub>2</sub>&nbsp;=&nbsp;(&phi;<sub>2</sub>,&lambda;<sub>2</sub>) (see Fig. 1, &phi; is the latitude, positive northward, and &lambda; is the longitude, positive eastward), the initial and final courses &alpha;<sub>1</sub> and &alpha;<sub>2</sub> are given by [[Solution of triangles#Two sides and the included angle given|formulas for solving a spherical triangle]]
:<math>\begin{align}
\tan\alpha_1&=\frac{\sin\lambda_{12}}{ \cos\phi_1\tan\phi_2-\sin\phi_1\cos\lambda_{12}},\\
\tan\alpha_2&=\frac{\sin\lambda_{12}}{-\cos\phi_2\tan\phi_1+\sin\phi_2\cos\lambda_{12}},\\
\end{align}</math>
where &lambda;<sub>12</sub>&nbsp;=&nbsp;&lambda;<sub>2</sub>&nbsp;&minus;&nbsp;&lambda;<sub>1</sub><ref group=note>In the article on [[great-circle distance]]s,
the notation &Delta;&lambda;&nbsp;=&nbsp;&lambda;<sub>12</sub>
and &Delta;&sigma;&nbsp;=&nbsp;&sigma;<sub>12</sub> is used.  The notation in this article is needed to
deal with differences between other points, e.g., &lambda;<sub>01</sub>.</ref>
and the quadrants of &alpha;<sub>1</sub>,&alpha;<sub>2</sub> are determined by the signs of the numerator and denominator in the tangent formulas (e.g., using the [[atan2]] function).
The [[central angle]] between the two points, &sigma;<sub>12</sub>, is given by
:<math>
\cos\sigma_{12}=\sin\phi_1\sin\phi_2+\cos\phi_1\cos\phi_2\cos\lambda_{12}.
</math>{{refn|group=note|If &sigma;<sub>12</sub> is less than 0.01&deg; (or more than 179.99&deg;) its cosine is 0.99999999 or more, leading to some inaccuracy. To avoid this, replace the usual formula with
:<math>\tan\sigma_{12}=\frac{\sqrt{(\cos\phi_1\sin\phi_2-\sin\phi_1\cos\phi_2\cos\lambda_{12})^2 + (\cos\phi_2\sin\lambda_{12})^2}}{\sin\phi_1\sin\phi_2+\cos\phi_1\cos\phi_2\cos\lambda_{12}}.</math>
The numerator of this formula contains the quantities that were used to determine
tan&alpha;<sub>1</sub>.}}{{refn|group=note|These equations for &alpha;<sub>1</sub>,&alpha;<sub>2</sub>,&sigma;<sub>12</sub> are suitable for implementation
on modern calculators and computers.  For hand computations with logarithms,
[[Delambre]]'s analogies<ref>{{cite book
|last = Todhunter
|first = I.
|authorlink = Isaac Todhunter
|title = Spherical Trigonometry
|year = 1871
|publisher = MacMillan
|edition = 3rd
|page = 26
|url = http://books.google.com/books?id=3uBHAAAAIAAJ&pg=PA26}}
</ref> were usually used:
:<math>
\begin{align}
\cos\tfrac12(\alpha_2+\alpha_1) \sin\tfrac12\sigma_{12} &= \sin\tfrac12(\phi_2-\phi_1) \cos\tfrac12\lambda_{12},\\
\sin\tfrac12(\alpha_2+\alpha_1) \sin\tfrac12\sigma_{12} &= \cos\tfrac12(\phi_2+\phi_1) \sin\tfrac12\lambda_{12},\\
\cos\tfrac12(\alpha_2-\alpha_1) \cos\tfrac12\sigma_{12} &= \cos\tfrac12(\phi_2-\phi_1) \cos\tfrac12\lambda_{12},\\
\sin\tfrac12(\alpha_2-\alpha_1) \cos\tfrac12\sigma_{12} &= \sin\tfrac12(\phi_2+\phi_1) \sin\tfrac12\lambda_{12}.
\end{align}
</math>
McCaw<ref>{{cite journal
|last = McCaw
|first = G. T.
|title = Long lines on the Earth
|journal = Empire Survey Review
|volume = 1
|number = 6
|pages = 259&ndash;263
|year = 1932}}</ref> refers to these equations as being in "logarithmic form", by which he means
that all the trigonometric terms appear as products; this minimizes the number of table lookups
required.  Furthermore, the redundancy in these formulas serves as a check in hand calculations. If using
these equations to determine the shorter path on the great circle, it is necessary to ensure
that |&lambda;<sub>12</sub>|&nbsp;&le;&nbsp;&pi; (otherwise the longer path is found).}}
The distance along the great circle will then be ''s''<sub>12</sub>&nbsp;=&nbsp;''R''&sigma;<sub>12</sub>, where ''R'' is the assumed radius
of the earth and &sigma;<sub>12</sub> is expressed in [[Radian#Conversions|radians]].
Using the [[Earth radius#Mean radius|mean earth radius]], ''R''&nbsp;=&nbsp;''R''<sub>1</sub>, yields results for
the distance ''s''<sub>12</sub> which are within 1% of the
[[Geodesics on an ellipsoid|geodesic distance]] for the [[WGS84]] ellipsoid.
 
==Finding way-points==
 
To find the way-points, that is the positions of selected points on the great circle between
''P''<sub>1</sub> and ''P''<sub>2</sub>, we first extrapolate the great circle back to its ''node'' ''A'', the point
at which the great circle crosses the
equator in the northward direction: let the longitude of this point be &lambda;<sub>0</sub> — see Fig&nbsp;1.  The azimuth at this point, &alpha;<sub>0</sub>, is given by the spherical sine rule:
:<math>
\sin\alpha_0 = \sin\alpha_1 \cos\phi_1.
</math>{{refn|group=note|To obtain accurate results in all cases, particularly when
&alpha;<sub>0</sub>&nbsp;&asymp;&nbsp;&plusmn;&frac12;&pi;, use instead
:<math>\tan\alpha_0 = \frac
{\sin\alpha_1 \cos\phi_1}{\sqrt{\cos^2\alpha_1 + \sin^2\alpha_1\sin^2\phi_1}}.</math>}}
Let the angular distances along the great circle from ''A''  to ''P''<sub>1</sub> and ''P''<sub>2</sub> be &sigma;<sub>01</sub> and &sigma;<sub>02</sub> respectively. Then using [[Spherical trigonometry#Napier's rules for quadrantal triangles|Napier's rules]] we have
:<math>
\tan\sigma_{01} = \frac{\tan\phi_1}{\cos\alpha_1}
\qquad</math>(If &phi;<sub>1</sub>&nbsp;=&nbsp;0 and &alpha;<sub>1</sub>&nbsp;=&nbsp;&frac12;&pi;, use &sigma;<sub>01</sub>&nbsp;=&nbsp;0).
 
This gives &sigma;<sub>01</sub>, whence &sigma;<sub>02</sub>&nbsp;=&nbsp;&sigma;<sub>01</sub>&nbsp;+&nbsp;&sigma;<sub>12</sub>.
 
The longitude at the node is found from
<!-- Don't simplify sin(sigma)/cos(sigma) to tan(sigma).  This gives the wrong quadrant for lambda. -->
:<math>
\begin{align}
\tan\lambda_{01} &= \frac{\sin\alpha_0\sin\sigma_1}{\cos\sigma_1},\\
\lambda_0 &= \lambda_1 - \lambda_{01}.
\end{align}
</math>
[[File:Sphere geodesic 2sigma.svg|thumb|200px|right|Figure 2. The great circle path between a node (an equator crossing) and an arbitrary point (&phi;,&lambda;).]]
Finally, calculate the position and azimuth at an arbitrary point, ''P'' (see Fig. 2), by  the spherical version of the ''direct geodesic problem''.{{refn|group=note|The direct geodesic problem, finding the position of ''P''<sub>2</sub> given ''P''<sub>1</sub>, &alpha;<sub>1</sub>,
and ''s''<sub>12</sub>, can also be solved by
[[Solution of triangles#Two sides and the included angle given|formulas for solving a spherical triangle]], as follows,
:<math>
\begin{align}
\sigma_{12} &= s_{12}/R,\\
\sin\phi_2 &= \sin\phi_1\cos\sigma_{12} + \cos\phi_1\sin\sigma_{12}\cos\alpha_1,\quad\text{or}\\
\tan\phi_2 &= \frac{\sin\phi_1\cos\sigma_{12} + \cos\phi_1\sin\sigma_{12}\cos\alpha_1}
{\sqrt{ (\cos\phi_1\cos\sigma_{12} - \sin\phi_1\sin\sigma_{12}\cos\alpha_1)^2 + (\sin\sigma_{12}\sin\alpha_1)^2 }},\\
\tan\lambda_{12} &= \frac{\sin\sigma_{12}\sin\alpha_1}
{\cos\phi_1\cos\sigma_{12} - \sin\phi_1\sin\sigma_{12}\cos\alpha_1},\\
\lambda_2 &= \lambda_1 + \lambda_{12},\\
\tan\alpha_2 &= \frac{\sin\alpha_1}
{\cos\sigma_{12}\cos\alpha_1 - \tan\phi_1\sin\sigma_{12}}.
\end{align}
</math>
The solution for way-points given in the main text is more general than this solution in that
it allows
way-points at specified longitudes to be found.  In addition, the solution for &sigma;
(i.e., the position of the node)
is needed when finding [[geodesics on an ellipsoid]] by means of the auxiliary sphere.}} Napier's rules give
:<math>
{\color{white}.\,\qquad)}\sin\phi = \cos\alpha_0\sin\sigma,</math>{{refn|group=note|To obtain accurate results in all cases, particularly when
&phi;&nbsp;&asymp;&nbsp;&plusmn;&frac12;&pi;, use instead
:<math>
\tan\phi = \frac
{\cos\alpha_0\sin\sigma}{\sqrt{\cos^2\sigma + \sin^2\alpha_0\sin^2\sigma}}.</math>}}
:<!-- Don't simplify sin(sigma)/cos(sigma) to tan(sigma).  This gives the wrong quadrant for lambda. --><math>
\begin{align}
\tan(\lambda - \lambda_0) &= \frac
{\sin\alpha_0\sin\sigma}{\cos\sigma},\\
\tan\alpha &= \frac
{\tan\alpha_0}{\cos\sigma}.
\end{align}
</math>
The [[atan2]] function should be used to determine
&sigma;<sub>01</sub>,
&lambda;, and &alpha;.
For example, to find the
midpoint of the path, substitute &sigma;&nbsp;=&nbsp;&frac12;(&sigma;<sub>01</sub>&nbsp;+&nbsp;&sigma;<sub>02</sub>); alternatively
to find the point a distance ''d'' from the starting point, take &sigma;&nbsp;=&nbsp;&sigma;<sub>01</sub>&nbsp;+&nbsp;''d''/''R''.
Likewise, the ''vertex'', the point on the great
circle with greatest latitude, is found by substituting &sigma;&nbsp;=&nbsp;+&frac12;&pi;.
It may be convenient to parameterize the route in terms of the longitude using
:<math>\tan\phi = \cot\alpha_0\sin(\lambda-\lambda_0).</math>
Latitudes at regular intervals of longitude can be found and the resulting positions transferred to the Mercator chart
allowing the great circle to be approximated by a series of [[rhumb line]]s.
 
These formulas apply to a spherical model of the earth.  They are also used in solving for the great circle
on the ''auxiliary sphere'' which is a device for finding the shortest path, or ''geodesic'', on
an ellipsoid of revolution; see
the article on [[geodesics on an ellipsoid]].
 
==Example==
 
Compute the great circle route from [[Valparaíso]],
&phi;<sub>1</sub>&nbsp;=&nbsp;&minus;33&deg;,
&lambda;<sub>1</sub>&nbsp;=&nbsp;&minus;71.6&deg;, to
[[Shanghai]],
&phi;<sub>2</sub>&nbsp;=&nbsp;31.4&deg;,
&lambda;<sub>2</sub>&nbsp;=&nbsp;121.8&deg;.
 
The formulas for course and distance give
&lambda;<sub>12</sub>&nbsp;=&nbsp;&minus;166.6&deg;,
&alpha;<sub>1</sub>&nbsp;=&nbsp;&minus;94.41&deg;,
&alpha;<sub>2</sub>&nbsp;=&nbsp;&minus;78.42&deg;, and
&sigma;<sub>12</sub>&nbsp;=&nbsp;168.56&deg;.  Taking the [[Earth radius#Mean radius|earth radius]] to be
''R''&nbsp;=&nbsp;6371&nbsp;km, the distance is
''s''<sub>12</sub>&nbsp;=&nbsp;18743&nbsp;km.
 
To compute points along the route, first find
&alpha;<sub>0</sub>&nbsp;=&nbsp;&minus;56.74&deg;,
&sigma;<sub>1</sub>&nbsp;=&nbsp;&minus;96.76&deg;,
&sigma;<sub>2</sub>&nbsp;=&nbsp;71.8&deg;,
&lambda;<sub>01</sub>&nbsp;=&nbsp;98.07&deg;, and
&lambda;<sub>0</sub>&nbsp;=&nbsp;&minus;169.67&deg;.
Then to compute the midpoint of the route (for example), take
&sigma;&nbsp;=&nbsp;&frac12;(&sigma;<sub>1</sub>&nbsp;+&nbsp;&sigma;<sub>2</sub>)&nbsp;=&nbsp;&minus;12.48&deg;, and solve
for
&phi;&nbsp;=&nbsp;&minus;6.81&deg;,
&lambda;&nbsp;=&nbsp;&minus;159.18&deg;, and
&alpha;&nbsp;=&nbsp;&minus;57.36&deg;.
 
If the geodesic is computed accurately on the [[WGS84]] ellipsoid,<ref>
{{cite journal
|first=C. F. F.
|last=Karney
|title=Algorithms for geodesics
|journal=J. Geodesy
|volume = 87
|number = 1
|year = 2013
|pages = 43&ndash;55
|accessdate=2012-07-14
|doi=10.1007/s00190-012-0578-z
|url=http://dx.doi.org/10.1007/s00190-012-0578-z
}}
</ref> the results
are &alpha;<sub>1</sub>&nbsp;=&nbsp;&minus;94.82&deg;, &alpha;<sub>2</sub>&nbsp;=&nbsp;&minus;78.29&deg;, and
''s''<sub>12</sub>&nbsp;=&nbsp;18752&nbsp;km.  The midpoint of the geodesic is
&phi;&nbsp;=&nbsp;&minus;7.07&deg;, &lambda;&nbsp;=&nbsp;&minus;159.31&deg;,
&alpha;&nbsp;=&nbsp;&minus;57.45&deg;.
 
==Gnomonic chart==
A straight line drawn on a [[Map projection#Gnomonic|Gnomonic chart]] would be a great circle track. When this is transferred to a [[Map projection#Mercator|Mercator]] chart, it becomes a curve. The positions are transferred at a convenient interval of [[longitude]] and this is plotted on the Mercator chart.
 
==See also==
* [[Great circle]]
* [[Great-circle distance]]
* [[Rhumb line]]
* [[Geographical distance]]
* [[Spherical Trigonometry]]
* [[Geodesics on an ellipsoid]]
 
==Notes==
{{reflist|group=note}}
 
==References==
{{reflist}}
 
==Resources==
* [http://www.greatcirclemapper.net The Great Circle Mapper] Displays Great Circle flight routes on a Map And calculates distance and duration
* [http://mathworld.wolfram.com/GreatCircle.html Great Circle &ndash; from MathWorld] Great Circle description, figures, and equations.  Mathworld, Wolfram Research, Inc. c1999
* [http://www.gcmap.com/ Great Circle Mapper]  Interactive tool for plotting great circle routes.
* [http://williams.best.vwh.net/gccalc.htm Great Circle Calculator] deriving (initial) course and distance between two points.
* [http://www.acscdg.com/ Great Circle Distance] Graphical tool for drawing great circles over maps.  Also shows distance and azimuth in a table.
 
[[Category:Navigation]]

Revision as of 01:39, 21 January 2013

28 year-old Painting Investments Worker Truman from Regina, usually spends time with pastimes for instance interior design, property developers in new launch ec Singapore and writing. Last month just traveled to City of the Renaissance.

Great-circle navigation is the practice of navigating a vessel (a ship or aircraft) along a great circle. A great circle track is the shortest distance between two points on the surface of a sphere; the Earth isn't exactly spherical, but the formulas for a sphere are simpler and are often accurate enough for navigation (see the numerical example).

Course and distance

Figure 1. The great circle path between (φ1, λ1) and (φ2, λ2).

The great circle path may be found using spherical trigonometry; this is the spherical version of the inverse geodesic problem. If a navigator begins at P1 = (φ11) and plans to travel the great circle to a point at point P2 = (φ22) (see Fig. 1, φ is the latitude, positive northward, and λ is the longitude, positive eastward), the initial and final courses α1 and α2 are given by formulas for solving a spherical triangle

where λ12 = λ2 − λ1[note 1] and the quadrants of α12 are determined by the signs of the numerator and denominator in the tangent formulas (e.g., using the atan2 function). The central angle between the two points, σ12, is given by

Template:RefnTemplate:Refn

The distance along the great circle will then be s12 = Rσ12, where R is the assumed radius of the earth and σ12 is expressed in radians. Using the mean earth radius, R = R1, yields results for the distance s12 which are within 1% of the geodesic distance for the WGS84 ellipsoid.

Finding way-points

To find the way-points, that is the positions of selected points on the great circle between P1 and P2, we first extrapolate the great circle back to its node A, the point at which the great circle crosses the equator in the northward direction: let the longitude of this point be λ0 — see Fig 1. The azimuth at this point, α0, is given by the spherical sine rule:

Template:Refn

Let the angular distances along the great circle from A to P1 and P2 be σ01 and σ02 respectively. Then using Napier's rules we have

(If φ1 = 0 and α1 = ½π, use σ01 = 0).

This gives σ01, whence σ02 = σ01 + σ12.

The longitude at the node is found from

Figure 2. The great circle path between a node (an equator crossing) and an arbitrary point (φ,λ).

Finally, calculate the position and azimuth at an arbitrary point, P (see Fig. 2), by the spherical version of the direct geodesic problem.Template:Refn Napier's rules give

Template:Refn

The atan2 function should be used to determine σ01, λ, and α. For example, to find the midpoint of the path, substitute σ = ½(σ01 + σ02); alternatively to find the point a distance d from the starting point, take σ = σ01 + d/R. Likewise, the vertex, the point on the great circle with greatest latitude, is found by substituting σ = +½π. It may be convenient to parameterize the route in terms of the longitude using

Latitudes at regular intervals of longitude can be found and the resulting positions transferred to the Mercator chart allowing the great circle to be approximated by a series of rhumb lines.

These formulas apply to a spherical model of the earth. They are also used in solving for the great circle on the auxiliary sphere which is a device for finding the shortest path, or geodesic, on an ellipsoid of revolution; see the article on geodesics on an ellipsoid.

Example

Compute the great circle route from Valparaíso, φ1 = −33°, λ1 = −71.6°, to Shanghai, φ2 = 31.4°, λ2 = 121.8°.

The formulas for course and distance give λ12 = −166.6°, α1 = −94.41°, α2 = −78.42°, and σ12 = 168.56°. Taking the earth radius to be R = 6371 km, the distance is s12 = 18743 km.

To compute points along the route, first find α0 = −56.74°, σ1 = −96.76°, σ2 = 71.8°, λ01 = 98.07°, and λ0 = −169.67°. Then to compute the midpoint of the route (for example), take σ = ½(σ1 + σ2) = −12.48°, and solve for φ = −6.81°, λ = −159.18°, and α = −57.36°.

If the geodesic is computed accurately on the WGS84 ellipsoid,[1] the results are α1 = −94.82°, α2 = −78.29°, and s12 = 18752 km. The midpoint of the geodesic is φ = −7.07°, λ = −159.31°, α = −57.45°.

Gnomonic chart

A straight line drawn on a Gnomonic chart would be a great circle track. When this is transferred to a Mercator chart, it becomes a curve. The positions are transferred at a convenient interval of longitude and this is plotted on the Mercator chart.

See also

Notes

43 year old Petroleum Engineer Harry from Deep River, usually spends time with hobbies and interests like renting movies, property developers in singapore new condominium and vehicle racing. Constantly enjoys going to destinations like Camino Real de Tierra Adentro.

References

43 year old Petroleum Engineer Harry from Deep River, usually spends time with hobbies and interests like renting movies, property developers in singapore new condominium and vehicle racing. Constantly enjoys going to destinations like Camino Real de Tierra Adentro.

Resources


Cite error: <ref> tags exist for a group named "note", but no corresponding <references group="note"/> tag was found

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