<?xml version="1.0" encoding="UTF-8"?>
<collection xmlns="http://www.loc.gov/MARC21/slim">
<record>
  <controlfield tag="001">108580</controlfield>
  <controlfield tag="005">20230519145357.0</controlfield>
  <datafield tag="024" ind1="7" ind2=" ">
    <subfield code="2">doi</subfield>
    <subfield code="a">10.1016/j.actaastro.2020.11.025</subfield>
  </datafield>
  <datafield tag="024" ind1="8" ind2=" ">
    <subfield code="2">sideral</subfield>
    <subfield code="a">122364</subfield>
  </datafield>
  <datafield tag="037" ind1=" " ind2=" ">
    <subfield code="a">ART-2021-122364</subfield>
  </datafield>
  <datafield tag="041" ind1=" " ind2=" ">
    <subfield code="a">eng</subfield>
  </datafield>
  <datafield tag="100" ind1=" " ind2=" ">
    <subfield code="a">Abad, A.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0002-5692-5876</subfield>
  </datafield>
  <datafield tag="245" ind1=" " ind2=" ">
    <subfield code="a">On the integration of Cid''s radial intermediary</subfield>
  </datafield>
  <datafield tag="260" ind1=" " ind2=" ">
    <subfield code="c">2021</subfield>
  </datafield>
  <datafield tag="506" ind1="0" ind2=" ">
    <subfield code="a">Access copy available to the general public</subfield>
    <subfield code="f">Unrestricted</subfield>
  </datafield>
  <datafield tag="520" ind1="3" ind2=" ">
    <subfield code="a">This paper deals with the integrations of homogeneous quasi-Keplerian Hamiltonians, that is, perturbed Kepler Hamiltonians which perturbation is of the form SUM j=2 N Aj/rj with Aj constant. Although there are many applications of these Hamiltonians in Physics, Astronomy and Astrodynamics, we focus our interest on a particular case in the core of Artificial Satellite Theory, the Cid's radial intermediary. For this problem, we integrate the equations of motion in two different ways, by means of the elliptic P-Weierstrass function and by using the Krylov–Bogoliubov averaging method to integrate a perturbed harmonic oscillator. In this case, the resulting solution is given in terms of the classical Kepler's equation, with no need of introducing more complex generalized Kepler's equation.</subfield>
  </datafield>
  <datafield tag="536" ind1=" " ind2=" ">
    <subfield code="9">info:eu-repo/grantAgreement/ES/DGA-FSE/E24-20R</subfield>
    <subfield code="9">info:eu-repo/grantAgreement/ES/DGA-FSE/E41-20R</subfield>
    <subfield code="9">info:eu-repo/grantAgreement/ES/MINECO/ESP2017-87113-R</subfield>
    <subfield code="9">info:eu-repo/grantAgreement/ES/MINECO/MTM2016-77735-C3-1-P</subfield>
  </datafield>
  <datafield tag="540" ind1=" " ind2=" ">
    <subfield code="9">info:eu-repo/semantics/openAccess</subfield>
    <subfield code="a">by-nc-nd</subfield>
    <subfield code="u">http://creativecommons.org/licenses/by-nc-nd/3.0/es/</subfield>
  </datafield>
  <datafield tag="590" ind1=" " ind2=" ">
    <subfield code="a">2.954</subfield>
    <subfield code="b">2021</subfield>
  </datafield>
  <datafield tag="591" ind1=" " ind2=" ">
    <subfield code="a">ENGINEERING, AEROSPACE</subfield>
    <subfield code="b">6 / 34 = 0.176</subfield>
    <subfield code="c">2021</subfield>
    <subfield code="d">Q1</subfield>
    <subfield code="e">T1</subfield>
  </datafield>
  <datafield tag="592" ind1=" " ind2=" ">
    <subfield code="a">1.0</subfield>
    <subfield code="b">2021</subfield>
  </datafield>
  <datafield tag="593" ind1=" " ind2=" ">
    <subfield code="a">Aerospace Engineering</subfield>
    <subfield code="c">2021</subfield>
    <subfield code="d">Q1</subfield>
  </datafield>
  <datafield tag="594" ind1=" " ind2=" ">
    <subfield code="a">5.7</subfield>
    <subfield code="b">2021</subfield>
  </datafield>
  <datafield tag="655" ind1=" " ind2="4">
    <subfield code="a">info:eu-repo/semantics/article</subfield>
    <subfield code="v">info:eu-repo/semantics/acceptedVersion</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Calvo, M.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0002-3312-5710</subfield>
  </datafield>
  <datafield tag="700" ind1=" " ind2=" ">
    <subfield code="a">Elipe, A.</subfield>
    <subfield code="u">Universidad de Zaragoza</subfield>
    <subfield code="0">(orcid)0000-0001-5208-4494</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="1">2005</subfield>
    <subfield code="2">595</subfield>
    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Matemática Aplicada</subfield>
    <subfield code="c">Área Matemática Aplicada</subfield>
  </datafield>
  <datafield tag="710" ind1="2" ind2=" ">
    <subfield code="1">2004</subfield>
    <subfield code="2">398</subfield>
    <subfield code="a">Universidad de Zaragoza</subfield>
    <subfield code="b">Dpto. Física Teórica</subfield>
    <subfield code="c">Área Física de la Tierra</subfield>
  </datafield>
  <datafield tag="773" ind1=" " ind2=" ">
    <subfield code="g">179 (2021), 519-524</subfield>
    <subfield code="p">Acta astronaut.</subfield>
    <subfield code="t">Acta Astronautica</subfield>
    <subfield code="x">0094-5765</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">296314</subfield>
    <subfield code="u">http://zaguan.unizar.es/record/108580/files/texto_completo.pdf</subfield>
    <subfield code="y">Postprint</subfield>
  </datafield>
  <datafield tag="856" ind1="4" ind2=" ">
    <subfield code="s">941836</subfield>
    <subfield code="u">http://zaguan.unizar.es/record/108580/files/texto_completo.jpg?subformat=icon</subfield>
    <subfield code="x">icon</subfield>
    <subfield code="y">Postprint</subfield>
  </datafield>
  <datafield tag="909" ind1="C" ind2="O">
    <subfield code="o">oai:zaguan.unizar.es:108580</subfield>
    <subfield code="p">articulos</subfield>
    <subfield code="p">driver</subfield>
  </datafield>
  <datafield tag="951" ind1=" " ind2=" ">
    <subfield code="a">2023-05-18-13:34:03</subfield>
  </datafield>
  <datafield tag="980" ind1=" " ind2=" ">
    <subfield code="a">ARTICLE</subfield>
  </datafield>
</record>
</collection>