Deutsch
 
Hilfe Datenschutzhinweis Impressum
  DetailsucheBrowse

Datensatz

 
 
DownloadE-Mail
  Structural analysis of Athena WFI Large Detector Array

Frank, J., Beitler, C., Pietschner, D., Strecker, R., Antonelli, V., Plattner, M., et al. (2020). Structural analysis of Athena WFI Large Detector Array. In Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray. doi:10.1117/12.2560668.

Item is

Basisdaten

einblenden: ausblenden:
Genre: Konferenzbeitrag

Dateien

einblenden: Dateien
ausblenden: Dateien
:
Structural analysis of Athena WFI Large Detector Array.pdf (beliebiger Volltext), 2MB
 
Datei-Permalink:
-
Name:
Structural analysis of Athena WFI Large Detector Array.pdf
Beschreibung:
-
OA-Status:
Sichtbarkeit:
Privat
MIME-Typ / Prüfsumme:
application/pdf
Technische Metadaten:
Copyright Datum:
-
Copyright Info:
-
Lizenz:
-

Externe Referenzen

einblenden:

Urheber

einblenden:
ausblenden:
 Urheber:
Frank, Jintin1, Autor           
Beitler, Christian1, Autor           
Pietschner, Daniel1, Autor           
Strecker, Rafael1, Autor           
Antonelli, Valeria2, Autor           
Plattner, Markus2, Autor           
Meidinger, Norbert1, Autor           
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              
2MPI for Extraterrestrial Physics, Max Planck Society, ou_159888              

Inhalt

einblenden:
ausblenden:
Schlagwörter: -
 Zusammenfassung: The WFI instrument is designed for high-resolution X-ray imaging and spectroscopy with a large field of view. A movable mirror focuses the X-rays onto the focal plane detectors of the WFI. For design development of the instrument, structural analysis is performed from early project phases. The WFI project has entered phase B and the preliminary design is evolving towards a more detailed design including interface definitions. The focal plane of WFI consists of two detectors: Large Detector Array (LDA) and Fast Detector (FD). The LDA assembly is used for main observation modes, whereas FD is for very bright point sources. The complexity of the LDA design is due to the fact that it has to be compliant to contradictory requirements. Its sensors have to be thermally decoupled from the structure, but with a high stiffness to avoid relative displacement and deformation of sensitive components, e.g. bond wires. The LDA has an active area that is as large as ≈14x14 cm2 but the thermal gradient across it shall be below 2.5-3K. The LDA is optimized with respect to mechanical requirements for launch loads and operational conditions in space. In order to minimize mass while withstanding thermo-mechanical, static and dynamic loads, various design studies have been carried out. With the aim to develop a design, which meets all structural and functional requirements, various structural analyses are performed. In this paper, the structural design studies and the preliminary analysis results of the WFI Large Detector Array are presented

Details

einblenden:
ausblenden:
Sprache(n): eng - English
 Datum: 2020-12-13
 Publikationsstatus: Online veröffentlicht
 Seiten: -
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: DOI: 10.1117/12.2560668
 Art des Abschluß: -

Veranstaltung

einblenden:
ausblenden:
Titel: Conference on Space Telescopes and Instrumentation - Ultraviolet to Gamma Ray / SPIE Astronomical Telescopes + Instrumentation Conference
Veranstaltungsort: ELECTR NETWORK
Start-/Enddatum: 2020-12-14 - 2020-12-18

Entscheidung

einblenden:

Projektinformation

einblenden:

Quelle 1

einblenden:
ausblenden:
Titel: Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Genre der Quelle: Konferenzband
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: -
Seiten: - Band / Heft: 11444 Artikelnummer: 114443W Start- / Endseite: - Identifikator: -