Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI
- Authors:
-
[1];
- Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)
- Publication Date:
- Research Org.:
- Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Fusion Energy Sciences (FES); USDOE National Nuclear Security Administration (NNSA)
- OSTI Identifier:
- 1432662
- Alternate Identifier(s):
- OSTI ID: 1463031
- Report Number(s):
- LLNL-JRNL-737511
Journal ID: ISSN 1538-4357; TRN: US1802661
- Grant/Contract Number:
- AC02-09CH11466; AC52-07NA27344
- Resource Type:
- Accepted Manuscript
- Journal Name:
- The Astrophysical Journal (Online)
- Additional Journal Information:
- Journal Name: The Astrophysical Journal (Online); Journal Volume: 854; Journal Issue: 2; Journal ID: ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; atomic data; plasmas; stars: flare; Sun: UV radiation; techniques: spectroscopic; ultraviolet: stars; Physics - Plasma physics
Citation Formats
Weller, M. E., Beiersdorfer, P., Soukhanovskii, V. A., Scotti, F., and LeBlanc, B. P. Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI. United States: N. p., 2018.
Web. doi:10.3847/1538-4357/aaa5a1.
Weller, M. E., Beiersdorfer, P., Soukhanovskii, V. A., Scotti, F., & LeBlanc, B. P. Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI. United States. https://doi.org/10.3847/1538-4357/aaa5a1
Weller, M. E., Beiersdorfer, P., Soukhanovskii, V. A., Scotti, F., and LeBlanc, B. P. Thu .
"Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI". United States. https://doi.org/10.3847/1538-4357/aaa5a1. https://www.osti.gov/servlets/purl/1432662.
@article{osti_1432662,
title = {Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI},
author = {Weller, M. E. and Beiersdorfer, P. and Soukhanovskii, V. A. and Scotti, F. and LeBlanc, B. P.},
abstractNote = {},
doi = {10.3847/1538-4357/aaa5a1},
journal = {The Astrophysical Journal (Online)},
number = 2,
volume = 854,
place = {United States},
year = {2018},
month = {2}
}
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Figures / Tables:
Figure 1: Spectra collected with LoWEUS from NSTX-U discharge 205079 during 200-270 ms. An expanded spectrum is shown below for more clarity. Fe XIII-XVI lines are highlighted in black, while lines from all other elements are in gray.
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Works referencing / citing this record:
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Electron-density-sensitive Line Ratios of Fe XIII--XVI from Laboratory Sources Compared to CHIANTI
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- Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States)
Figures/Tables have been extracted from DOE-funded journal article accepted manuscripts.