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Additions to the Spectrum of Fe IX in the 110–200 Å RegionThe spectrum of eight-times ionized iron, Fe IX , was studied in the 110–200 Å region. A low inductance vacuum
spark and a 3 m grazing incidence spectrograph were used for the excitation and recording of the spectrum.
Previous analyses of Fe IX have been greatly extended and partly revised. The number of known lines in the
3p^(5)3d–3p^(5)4f and 3p^(5)3d–3p^(4)3d^(2) transition arrays is extended to 25 and 81, respectively. Most of the identifications
of the Fe IX lines from the 3p^(5)3d–3p^(4)3d^(2) transition array in the solar spectrum have been confirmed and several
new identifications are suggested.
Document ID
20230001382
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Alexander N. Ryabtsev ORCID
(Institute of Spectroscopy Moscow, Russia)
Edward Y. Kononov
(Institute of Spectroscopy Moscow, Russia)
Peter R Young ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
January 27, 2023
Publication Date
August 30, 2022
Publication Information
Publication: Astrophysical Journal
Publisher: IOP Publishing
Volume: 936
Issue: 1
Issue Publication Date: September 1, 2022
ISSN: 0004-637X
e-ISSN: 1538-4357
Subject Category
Astrophysics
Funding Number(s)
WBS: 944022.02.01.03.21
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
Keywords
atmoic spectroscopy
spectroscopy
line intensities
solar extreme ultraviolet emission
solar atmosphere
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