Page - 89 - in Contributions to GRACE Gravity Field Recovery - Improvements in Dynamic Orbit Integration, Stochastic Modelling of the Antenna Offset Correction, and Co-Estimation of Satellite Orientations
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0 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24
Time [h]
0.001
0.01
0.1
1
10
100
Osculating
Best-fit
Figure 7.3: Encke ratio over one orbit arc for osculating reference orbit (in pink) and
best-fit orbit (in green).
The Encke ratio for the best-fit orbit is in general much smaller, never increasing much
beyond 0.1%. The upper bound of 1% given by Lundberg, Bettadpur, and Eanes (2000)
is never reached. The Encke ratio shows approximately time-symmetric behaviour,
with the lowest ratio at the centre of the orbit arc, and the largest ratios at the beginning
and end. In absolute terms, the largest observed deviation of the best-fit ellipse from
the perturbed motion is 8.2km, a reduction of 99.3% from the osculating case.
7.3.2 Convergence
As outlined in section 7.1, the convergence of the dynamic orbit solution can be taken
as a benchmark indicating the correctness of the algorithm. To determine the number
of iterations necessary for convergence to occur, the simulated orbit was deteriorated
with Gaussian white noise. The standard deviation for the position component was set
toσr=50m, that for the velocity component toσr˙=0.5m/s.
The deteriorated orbit was inserted as the first approximate positionre into the orbit
integration routine. Then, 100 iterations of integration and correction were computed
for five configurations which differ in the choice and parametrisation of the refer-
ence trajectory. The first is a configuration with no reference motion, or f0 = 0 in
brown. The second pair consists of osculating reference ellipses, defined by∆y0=0,
parametrised in either Kepler elements (pink) or equinoctial elements (purple). The
last pair represents the best-fit ellipses with∆y0=∆yˆ0, also parametrised in either
Kepler elements (green) or equinoctial elements (orange). Figure 7.4 shows the root
mean square (RMS) of the corrections∆re applied for these five configurations in each
iteration cycle.
7.3 Results 89
Contributions to GRACE Gravity Field Recovery
Improvements in Dynamic Orbit Integration, Stochastic Modelling of the Antenna Offset Correction, and Co-Estimation of Satellite Orientations
- Title
- Contributions to GRACE Gravity Field Recovery
- Subtitle
- Improvements in Dynamic Orbit Integration, Stochastic Modelling of the Antenna Offset Correction, and Co-Estimation of Satellite Orientations
- Author
- Matthias Ellmerr
- Publisher
- Verlag der Technischen Universität Graz
- Location
- Graz
- Date
- 2018
- Language
- English
- License
- CC BY 4.0
- ISBN
- 978-3-85125-646-8
- Size
- 21.0 x 29.7 cm
- Pages
- 185
- Keywords
- Geodäsie, Gravitation, Geodesy, Physics, Physik
- Categories
- Naturwissenschaften Physik
- Technik