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Bernese GPS Software Version 5.0 - Bernese GNSS Software

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5.4 Preparation of Precise Orbit Information<br />

Figure 5.6: Options for numerical integration in program ORBGEN.<br />

Up to nine radiation pressure parameters may be adjusted per satellite and satellite arc.<br />

They refer to the CODE Extended Radiation Pressure Model [Beutler et al., 1994], see<br />

Section 2.2.2.3. The user has to select the radiation pressure model parameters that have to<br />

be adjusted in panel “ORBGEN 4: Parameter Selection”, see Figure 5.5. We will give different<br />

recommendations below for different types of tabular positions (broadcast or precise).<br />

The standard options for the numerical integration of <strong>GNSS</strong> orbits are displayed in Figure<br />

5.6 (see Section 2.2.3). In general, two iterations are sufficient. In the case of <strong>GPS</strong> and<br />

GLONASS satellites, a subinterval length of 1 hour and a polynomial degree (or integration<br />

order) of q = 10 results in an accumulated approximation error after three days which is still<br />

below 1 mm in satellite position. For the integration of a LEOthe integration subinterval<br />

length has to be reduced at least to 0.05 hours (corresponds to 3 minutes).<br />

Program ORBGEN will always produce a summary concerning the fit of the tabular orbit<br />

positions. If you were using tabular or precise orbit files stemming from broadcast messages,<br />

such a summary (in the second iteration step) will look roughly as in Figure 5.7. The<br />

table shows that the internal consistency of the broadcast orbits is around 1 meter (the<br />

actual accuracy is around three meters). It was produced by adjusting only two radiation<br />

pressure parameters, namely “D0” (direct) and “Y0” (y-bias) in panel “ORBGEN 4: Parameter<br />

Selection” (see Figure 5.5) which is sufficient to accommodate broadcast orbits. Bulletin A<br />

Earth orientation information was used.<br />

Figure 5.8 shows that the fit is of the order of 1 cm if a precise IGS ephemerides file is<br />

used together with the corresponding Earth orientation parameters and adjusting all nine<br />

radiation pressure parameters to generate the standard orbit. This means that the force<br />

<strong>Bernese</strong> <strong>GPS</strong> <strong>Software</strong> <strong>Version</strong> <strong>5.0</strong> Page 95

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