<?xml version='1.0' encoding='UTF-8'?>
<OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd">
  <responseDate>2026-03-08T21:12:07Z</responseDate>
  <request metadataPrefix="jpcoar_1.0" identifier="oai:ir.soken.ac.jp:00003117" verb="GetRecord">https://ir.soken.ac.jp/oai</request>
  <GetRecord>
    <record>
      <header>
        <identifier>oai:ir.soken.ac.jp:00003117</identifier>
        <datestamp>2023-06-20T15:16:52Z</datestamp>
        <setSpec>2:427:13</setSpec>
      </header>
      <metadata>
        <jpcoar:jpcoar xmlns:datacite="https://schema.datacite.org/meta/kernel-4/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcndl="http://ndl.go.jp/dcndl/terms/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:jpcoar="https://github.com/JPCOAR/schema/blob/master/1.0/" xmlns:oaire="http://namespace.openaire.eu/schema/oaire/" xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:rioxxterms="http://www.rioxx.net/schema/v2.0/rioxxterms/" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns="https://github.com/JPCOAR/schema/blob/master/1.0/" xsi:schemaLocation="https://github.com/JPCOAR/schema/blob/master/1.0/jpcoar_scm.xsd">
          <dc:title>Design of Loose Spacecraft Formation Flying around Halo Orbits</dc:title>
          <dc:title xml:lang="en">Design of Loose Spacecraft Formation Flying around Halo Orbits</dc:title>
          <jpcoar:creator>
            <jpcoar:creatorName>SIMANJUNTAK, Triwanto</jpcoar:creatorName>
          </jpcoar:creator>
          <jpcoar:creator>
            <jpcoar:creatorName>シマンジュンタク, トリワント</jpcoar:creatorName>
          </jpcoar:creator>
          <jpcoar:creator>
            <jpcoar:creatorName xml:lang="en">SIMANJUNTAK, Triwanto</jpcoar:creatorName>
          </jpcoar:creator>
          <datacite:description descriptionType="Other">Two spacecraft or more are assumed to be in a state of loose formation flying around
a collinear Lagrangian point in the Sun-Earth Circular Restricted Three-Body Problem
(CRTBP) system. The orbit reference of choice for the leader is a Halo orbit and the
followers are assumed to follow nearby and be constrained either geometrically or in
size. This type of formation could be useful in the future for constructing space ports,
space telescopes, astronomical spacecraft requiring sun shields and, with greater num-
bers, spacecraft swarm missions. The formation design method is constructed by firstly
seeking the local coordinate system from the monodromy matrix through extraction of
the independent bases which span the space of the Halo orbit. To nullify diverging and
converging motion, we confine the relative motion to within the periodic subspaces. Two
types of formations are studied in this thesis, natural loose formations and periodic loose
formations with impulsive control. For natural formations, two modes of relative motion
within these subspaces, long-term and short-term motions. In this study, the long-term
motion is approximated by deriving a discrete formulation of independent directions
based on the eigenvectors of the monodromy matrix, while for the short-term motion
the fundamental set solutions are modeled using Fourier series and additional linear func-
tions. Since the size of the formation discussed is significantly smaller than that of the
Halo orbit, the formation design method can fundamentally be stated as a process of
linearly combining these approximations to achieve the desired formation. Consequently,
use of this approach transforms formation design from a differential equation problem
into an algebraic one, and furthermore enables the long-term and short-term motion
design problems to be handled either jointly or separately. To increase design degree of
freedom impulsive control is introduced to the formation problem. The use of single, two
and three impulses are specially discussed in detail. Design examples, both for natural
and with impulsive control formation are presented to demonstrate the validity of the
design method. Keywords: Restricted Circular Three-Body Problem, Loose Formation
Flying, Halo Orbits, Impulsive Control</datacite:description>
          <datacite:description descriptionType="Other">総研大甲第1490号</datacite:description>
          <dc:language>eng</dc:language>
          <dc:type rdf:resource="http://purl.org/coar/resource_type/c_46ec">thesis</dc:type>
          <jpcoar:identifier identifierType="URI">https://ir.soken.ac.jp/records/3117</jpcoar:identifier>
          <dcndl:degreeName>博士（工学）</dcndl:degreeName>
          <dcndl:dateGranted>2012-03-23</dcndl:dateGranted>
          <jpcoar:degreeGrantor>
            <jpcoar:degreeGrantorName>総合研究大学院大学</jpcoar:degreeGrantorName>
          </jpcoar:degreeGrantor>
          <jpcoar:file>
            <jpcoar:URI label="要旨・審査要旨">https://ir.soken.ac.jp/record/3117/files/甲1490_要旨.pdf</jpcoar:URI>
            <jpcoar:mimeType>application/pdf</jpcoar:mimeType>
            <jpcoar:extent>328.4 kB</jpcoar:extent>
            <datacite:date dateType="Available">2016-02-17</datacite:date>
          </jpcoar:file>
          <jpcoar:file>
            <jpcoar:URI label="本文">https://ir.soken.ac.jp/record/3117/files/甲1490_本文.pdf</jpcoar:URI>
            <jpcoar:mimeType>application/pdf</jpcoar:mimeType>
            <jpcoar:extent>3.2 MB</jpcoar:extent>
            <datacite:date dateType="Available">2016-02-17</datacite:date>
          </jpcoar:file>
        </jpcoar:jpcoar>
      </metadata>
    </record>
  </GetRecord>
</OAI-PMH>
