Atomic Structure Calculations of Landé
(2021) In Astrophysical Journal 923(2).- Abstract
We perform a detailed theoretical study of the atomic structure of ions with ns 2 np m ground configurations and focus on departures from LS coupling, which directly affect the Landé g factors of magnetic dipole lines between levels of the ground terms. Particular emphasis is given to astrophysically abundant ions formed in the solar corona (those with n = 2,3) with M1 transitions spanning a broad range of wavelengths. Accurate Landé g factors are needed to diagnose coronal magnetic fields using measurements from new instruments operating at visible and infrared wavelengths, such as the Daniel K. Inouye Solar Telescope. We emphasize an explanation of the dynamics of atomic structure effects for nonspecialists.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/a203dfc5-77ba-41bf-b548-791076df0158
- author
- Schiffmann, Sacha LU ; Brage, Tomas LU ; Gordon Judge, Philip ; Paraschiv, Alin Razvan and Wang, Kai
- organization
- publishing date
- 2021-12-20
- type
- Contribution to journal
- publication status
- published
- subject
- in
- Astrophysical Journal
- volume
- 923
- issue
- 2
- article number
- 186
- publisher
- American Astronomical Society
- external identifiers
-
- scopus:85122917431
- ISSN
- 0004-637X
- DOI
- 10.3847/1538-4357/ac2cca
- language
- English
- LU publication?
- yes
- additional info
- Publisher Copyright: © 2021. The American Astronomical Society. All rights reserved.
- id
- a203dfc5-77ba-41bf-b548-791076df0158
- date added to LUP
- 2022-02-04 15:56:50
- date last changed
- 2022-04-21 23:04:51
@article{a203dfc5-77ba-41bf-b548-791076df0158, abstract = {{<p>We perform a detailed theoretical study of the atomic structure of ions with ns 2 np m ground configurations and focus on departures from LS coupling, which directly affect the Landé g factors of magnetic dipole lines between levels of the ground terms. Particular emphasis is given to astrophysically abundant ions formed in the solar corona (those with n = 2,3) with M1 transitions spanning a broad range of wavelengths. Accurate Landé g factors are needed to diagnose coronal magnetic fields using measurements from new instruments operating at visible and infrared wavelengths, such as the Daniel K. Inouye Solar Telescope. We emphasize an explanation of the dynamics of atomic structure effects for nonspecialists.</p>}}, author = {{Schiffmann, Sacha and Brage, Tomas and Gordon Judge, Philip and Paraschiv, Alin Razvan and Wang, Kai}}, issn = {{0004-637X}}, language = {{eng}}, month = {{12}}, number = {{2}}, publisher = {{American Astronomical Society}}, series = {{Astrophysical Journal}}, title = {{Atomic Structure Calculations of Landé}}, url = {{http://dx.doi.org/10.3847/1538-4357/ac2cca}}, doi = {{10.3847/1538-4357/ac2cca}}, volume = {{923}}, year = {{2021}}, }