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Fast integration of low orbiter's trajectory perturbed by the earth's non-sphericity

dc.citation.epage585en_US
dc.citation.spage578en_US
dc.citation.volume72en_US
dc.citation.woscount13en_US
dc.contributor.authorHwang, Cen_US
dc.contributor.authorLin, MJen_US
dc.contributor.department土木工程學系zh_TW
dc.contributor.departmentDepartment of Civil Engineeringen_US
dc.date.accessioned2019-04-02T05:59:33Z
dc.date.available2019-04-02T05:59:33Z
dc.date.issued1998-10-01en_US
dc.description.abstractA fast algorithm is proposed to integrate the trajectory of a low obiter perturbed by the earth's nonsphericity. The algorithm uses a separation degree to define the low-degree and the high-degree acceleration components, the former computed rigorously, and the latter interpolated from gridded accelerations. An FFT method is used to grid the accelerations. An optimal grid type for the algorithm depends on the trajectory's permissible error, speed, and memory capacity. Using the non-spherical accelerations computed from EGM96 to harmonic degree 360, orbit integrations were performed for a low orbiter at an altitude of 170 km. For a separation degree of 50, the new algorithm, together with the predict-pseudo correct method, speeds up the integration by 145 times compared to the conventional algorithm while keeping the errors in position and velocity below 10(-4) m and 10(-7) mis for a 3-day arc.en_US
dc.identifier.doi10.1007/s001900050196en_US
dc.identifier.issn0949-7714en_US
dc.identifier.journalJOURNAL OF GEODESYen_US
dc.identifier.urihttp://dx.doi.org/10.1007/s001900050196en_US
dc.identifier.urihttps://ir.lib.nycu.edu.tw/handle/11536/147669
dc.identifier.wosnumberWOS:000076660600002en_US
dc.language.isoen_USen_US
dc.subjectorbit integrationen_US
dc.subjectFFTen_US
dc.subjectperturbationen_US
dc.subjectspherical harmonicsen_US
dc.titleFast integration of low orbiter's trajectory perturbed by the earth's non-sphericityen_US
dc.typeArticleen_US

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