caa a22 4500 467987440 CHVBK 20180323112536.0 cr unu---uuuuu 170328e19901201xx s 000 0 eng 10.1007/BF00049391 doi (NATIONALLICENCE)springer-10.1007/BF00049391 Tesseral harmonic perturbations in radial transverse and binormal components [Elektronische Daten] [Edwin Wnuk, Slawomir Breiter] The formulae for the perturbations in radial, transverse and binormal components of the Earth artificial satellite motion have been derived. Perturbations due to the tesseral part of the geopotential are considered. The geopotential expressed in terms of the orbital elements has the form proposed by Wnuk (1988). The formulae for the perturbations have been obtained using the Hori (1966) method. They can be effectively applied in calculation of the perturbations in the components including the coefficients of the high order and degree tesseral harmonics. The derived formulae reveal no singularities at zero eccentricity. Kluwer Academic Publishers, 1990 Wnuk Edwin Astronomical Observatory of the A. Mickiewicz University, Poznah, Poland aut Breiter Slawomir Astronomical Observatory of the A. Mickiewicz University, Poznah, Poland aut Celestial Mechanics and Dynamical Astronomy Kluwer Academic Publishers 48/4(1990-12-01), 375-385 0923-2958 48:4<375 1990 48 10569 https://doi.org/10.1007/BF00049391 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/BF00049391 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Wnuk Edwin Astronomical Observatory of the A. Mickiewicz University, Poznah, Poland aut NATIONALLICENCE 700 1- Breiter Slawomir Astronomical Observatory of the A. Mickiewicz University, Poznah, Poland aut NATIONALLICENCE 773 0- Celestial Mechanics and Dynamical Astronomy Kluwer Academic Publishers 48/4(1990-12-01), 375-385 0923-2958 48:4<375 1990 48 10569 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer