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'''Geopotential''' is the potential of the [[Earth]]'s [[gravity field]]. For convenience it is often defined as ''minus'' the [[potential energy]] per unit [[mass]], so that the gravity vector is obtained as the [[gradient]] of this potential, without the minus.
 
For [[geophysical]] applications, gravity is distinguished from gravitation. Gravity is defined as the resultant of [[gravitation]] and the [[centrifugal force (fictitious)|centrifugal force]] caused by the [[Earth's rotation]]. The [[Sea level|global mean sea surface]] is close to one of the equipotential surfaces of the geopotential of gravity. This equipotential surface, or surface of constant geopotential, is called the [[geoid]].
 
For the purpose of satellite [[orbital mechanics]], the geopotential is typically described by a series expansion into [[spherical harmonics]] ([[spectral]] representation). In this context the geopotential is taken as the potential of the gravitational field of the Earth, that is, leaving out the centrifugal potential.
 
Solving for geopotential (Φ):
:<math>\Phi(h) = \int_0^h g\,dz\ </math><ref>Holton, James R. ''An Introduction to Dynamic Meteorology''. 4th ed. Burlington: Elsevier, 2004. Print.</ref>
:<math>\Phi = \int_0^z \left[ \frac{Gm}{(a+z)^2} \right] dz</math>
 
Integrate to get
:<math>\Phi = Gm \left[\frac{1}{a} - \frac{1}{a+z} \right]</math>
 
where:
:G=6.673x10<sup>-11</sup> Nm<sup>2</sup>/kg<sup>2</sup> is the gravitational constant,
:m=5.975x10<sup>24</sup> kg is the mass of the earth,
:a=6.378x10<sup>6</sup> m is the average radius of the earth,
:z is the height in meters
:Φ is the geopotential at height z, which is in units of [m<sup>2</sup>/s<sup>2</sup>] or [J/kg].
 
==See also==
* [[Geoid]]
* [[Physical geodesy]]
* [[Geopotential height]]
* [[Geopotential model]]
 
==References==
{{Reflist}}
 
{{Geophysics-stub}}
[[Category:Gravimetry]]

Latest revision as of 11:33, 7 January 2015

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