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Faculté des Sciences
Faculté des Sciences
MASTER THESIS
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Investigation of unidentified lines in optical cometary spectra

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Blond Hanten, Elsa ULiège
Promotor(s) : Jehin, Emmanuel ULiège
Date of defense : 5-Sep-2024/6-Sep-2024 • Permalink : http://hdl.handle.net/2268.2/21661
Details
Title : Investigation of unidentified lines in optical cometary spectra
Translated title : [fr] Etude des raies non identifiées dans les spectres optiques de comètes
Author : Blond Hanten, Elsa ULiège
Date of defense  : 5-Sep-2024/6-Sep-2024
Advisor(s) : Jehin, Emmanuel ULiège
Committee's member(s) : Hutsemekers, Damien ULiège
Grodent, Denis ULiège
de Keyser, Johan 
Language : English
Number of pages : 103
Keywords : [en] comet
[en] cometary atlas
[en] spectrum
[en] fluorescence
[en] UVES
Discipline(s) : Physical, chemical, mathematical & earth Sciences > Space science, astronomy & astrophysics
Target public : Researchers
Professionals of domain
Student
Institution(s) : Université de Liège, Liège, Belgique
Degree: Master en sciences spatiales, à finalité approfondie
Faculty: Master thesis of the Faculté des Sciences

Abstract

[en] The first objective of this thesis focuses on enhancing the Atlas of cometary lines developed
by Hardy and the ULiège COMETA team in 2022. This Atlas is based on the spectra of
comets C/2002 T7 (LINEAR), C/2016 R2 (PANSTARRS), C/2002 X5 (Kudo-Fujikawa), and
8P/Tuttle obtained by the ULiège team using the high-resolution Ultraviolet and Visual Echelle
Spectrograph (UVES). The use of spectra that are centred and offset in the tail direction allows
the identification of new lines, especially ionic ones. A total of 579 new lines have been identified
in the spectra, among which 57 were previously unidentified lines in the Atlas. The remaining 522
lines are new lines that had not previously been detected in the version of the Atlas developed by
Hardy. The second objective of the thesis focuses on developing a fluorescence model of imidogen (NH). We describe how the model was set up, and then present the results obtained from the model. The thesis ends with numerous perspectives on continuing the identification of new lines using different comparison techniques.


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Author

  • Blond Hanten, Elsa ULiège Université de Liège > Master sc. spatiales, fin approf.

Promotor(s)

Committee's member(s)

  • Hutsemekers, Damien ULiège Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Space sciences, Technologies and Astroph. Research (STAR)
    ORBi View his publications on ORBi
  • Grodent, Denis ULiège Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP)
    ORBi View his publications on ORBi
  • de Keyser, Johan Institut royal d'Aéronomie Spatiale de Belgique (BIRA-IASB), Belgium > Space Physics department
  • Total number of views 22
  • Total number of downloads 14










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