Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT
  Methods for orbit optimization for the LISA gravitational wave observatory

Yi, Z., Li, G., Heinzel, G., Rüdiger, A., Jennrich, O., Wang, L., et al. (2008). Methods for orbit optimization for the LISA gravitational wave observatory. International Journal of Modern Physics D, 17(7), 1021-1042.

Item is

Dateien

einblenden: Dateien
ausblenden: Dateien
:
S021827180801267X.pdf (beliebiger Volltext), 849KB
Datei-Permalink:
-
Name:
S021827180801267X.pdf
Beschreibung:
-
OA-Status:
Sichtbarkeit:
Öffentlich
MIME-Typ / Prüfsumme:
application/pdf / [MD5]
Technische Metadaten:
Copyright Datum:
-
Copyright Info:
-
Lizenz:
-

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Yi, Zhaohua1, Autor
Li, Guangyu1, Autor
Heinzel, Gerhard2, Autor           
Rüdiger, Albrecht2, Autor           
Jennrich, Oliver2, Autor
Wang, Li1, Autor
Xia, Yan1, Autor
Zeng, Fei1, Autor
Zhao, Haibin1, Autor
Affiliations:
1External Organizations, ou_persistent22              
2Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, Hannover, DE, ou_24010              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 Zusammenfassung: The Laser Interferometer Space Antenna (LISA) mission is a joint ESA-NASA mission for detecting low-frequency gravitational waves in the frequency range from 0.1mHz to 1Hz, by using accurate distance measurements with laser interferometry between three spacecraft, which will be launched around 2015 and one year later reach their orbits around the Sun. In order to operate successfully, it is crucial for the constellation of the three spacecraft to have extremely high stability. In this paper, several problems of the orbit optimization of the LISA constellation are discussed by using numerical and analytical methods for satisfying the requirements of accuracy. On the basis of the coorbital restricted problem, analytical expressions of the heliocentric distance and the trailing angle to the Earth of the constellation's barycenter are deduced, with the result that the approximate analytical solution of first order will meet the accuracy requirement of the spacecraft orbit design. It is proved that there is a value of the inclination of the constellation plane that will make the variation of the arm-length a minimum. The principle for selecting the optimum starting elements of orbits at any epoch is proposed. The method and programming principles of finding the optimized orbits are also presented together with examples of the optimization design.

Details

einblenden:
ausblenden:
Sprache(n):
 Datum: 2008-05
 Publikationsstatus: Erschienen
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: eDoc: 398735
 Art des Abschluß: -

Veranstaltung

einblenden:
ausblenden:
Titel: 3rd International ASTROD Symposium
Veranstaltungsort: Beijing, CHINA
Start-/Enddatum: 2006-07-13 - 2006-07-16

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: International Journal of Modern Physics D
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: Singapore : World Scientific
Seiten: - Band / Heft: 17 (7) Artikelnummer: - Start- / Endseite: 1021 - 1042 Identifikator: ISSN: 0218-2718
CoNE: https://pure.mpg.de/cone/journals/resource/954925493947