A Lagrange interpolation is used to compute the Xvt for times that are not in the table but do have sufficient data.
Definition in file TabularEphemerisStore.hpp.
#include <iostream>
#include "SatID.hpp"
#include "DayTime.hpp"
#include "XvtStore.hpp"
#include "SP3Data.hpp"
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Namespaces | |
| namespace | gpstk |
Classes | |
| class | TabularEphemerisStore |
| Store a tabular list of Xvt data (such as a table of precise ephemeris data in an SP3 file) and compute Xvt from this table. More... | |
1.3.9.1