The normal gravity field is a coarse approximation of the true gravity field of the Earth. It serves as a simple easy-to-compute model. In geodesy and geophysics we use rotationally symmetric normal gravity fields, where a surface of equal gravity potential (known as equipotential or level surface) coincides with a geodetic reference ellipsoid, e.g. GRS80 or
The value of the gravity acceleration in the normal gravity field is called normal gravity γ . It depends on the latitude φ and the ellipsoidal height h above the level ellipsoid. It decreases from the poles to the equator by about 0.052 m/s² and in vertical direction by about 0.003 m/s² per kilometre of altitude. The following normal gravity formulae are implemented:
γo(φ ) = γe·
(1+5.3024· 10-3· sin(φ )²
-5.8· 10-6· sin(2φ )²)
γ(φ ,h) = γo(φ )·
(1−2·(1+f+m−2·f·sin(2φ )²)·(h/a)+3·(h/a)²)
with γe = 9.780318 m/s²; a = 6378160 m;
f = 1.0/298.247167427;
m = 0.0034498014343
γo(φ ) =γe· (1+k· sin(φ )²)
(1-e²· sin(φ )²)-½
with values for
GRS80 | WGS84 | unit | |
---|---|---|---|
γe | 9.78032677153489285793 | 9.780325335903891718546 | m/s² |
k | 0.0019318513532606763607 | 0.0019318526524582735209 | - |
e² | 0.00669438002290341574957 | 0.006694379990141316996137 | - |
γ(φ ,h) = γo(φ )·
(1-(k1-k2·sin(φ )²)·h+k3·h²)
with values for
k1=3.15704· 10-7;
k2=2.10269· 10-9;
k3=7.37452· 10-14
and h in the unit metre.
We compute the normal gravity for the gravity benchmark at the geodetic laboratory of the
.
The ellipsoidal latitude equals 51.03361°. The height is 114 m
above the reference surface DHHN92.
The height of the reference surface DHHN92 above the ellipsoid WGS84 equals
35 m.
This results in a ellipsoidal height above WGS84 of about 149 m. We compute a value of
γ(φ ,h)= 9.811161 m/s².
By the way, an absolute gravity value measured at the geodetic laboratory is obtained as
9.811193 m/s² (rounded).
We further compute the vertical gradient of the normal gravity at this benchmark. For this purpose we use the utility with a height deviation of exactly 1 m. The deviation of gravity at a height deviation of 1 m equals the value of the vertical gradient (sign is always minus). The latitude is held fixed. In this case it is arbitrary if you specify the height deviation as a maximum or standard deviation. The value of 3.085·10-6s-2 is obtained.
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