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Satellite Orbit and Ephemeris Determination using Inter Satellite Links

Satellite Orbit and Ephemeris Determination using Inter Satellite Links

Satellite Orbit and Ephemeris Determination using Inter Satellite Links

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<strong>Inter</strong> <strong>Satellite</strong> <strong>Links</strong>Simulations <strong>and</strong> Results6.2.5 Pure LEO Constellation6.2.5.1 Ground Tracking with Full NetworkIn this scenario, orbit determination for the LEO constellation has been done <strong>using</strong> groundmeasurements only, but with a large scale network of ground stations. Using the DORISnetwork provides a good tracking accuracy for LEO satellites. This is due to the large numberof tracking stations, distributed over the world. A radial accuracy of better than 30 cm can bereached most of the time. Although LEO satellites have a higher along track error due to theuncertainty in the high altitude air density, a LEO satellite tracked by a large ground networkcan be seen from more than 5 stations the whole time. Due to the low altitude, the trackinggeometry is also good.Radial Error [cm] 1998 07 02 05:24 - 1998 07 09 11:2450.025.0Radial Std. Dev. [cm] 1998 07 02 05:24 - 1998 07 09 11:2432.0016.0-25.0-50.0[h]41 82 123 1640[h]40 80 120 160Along Track Error [cm] 1998 07 02 05:24 - 1998 07 09 11:2498.049.0Along Track Std. Dev. [cm] 1998 07 02 05:24 - 1998 07 09 11:2444.0022.0-49.0-98.0[h]41 82 123 1640[h]40 80 120 160Cross T rack Error [cm] 1998 07 02 05:24 - 1998 07 09 11:2434.017.0Cross Track Std. Dev. [cm] 1998 07 02 05:24 - 1998 07 09 11:2416.008.0-17.0-34.0[h]41 82 123 1640[h]40 80 120 160Figure 6-30 Tracking Accuracy of LEO <strong>using</strong> DORIS Network onlyR. Wolf Page 125

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