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Title: Electron-density-sensitive Line Ratios of Fe xiii– xvi from Laboratory Sources Compared to CHIANTI

Journal Article · · The Astrophysical Journal (Online)
 [1]; ORCiD logo [1];  [1];  [1];  [2]
  1. Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
  2. Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)

Research Organization:
Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States); Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Fusion Energy Sciences (FES); USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC02-09CH11466; AC52-07NA27344
OSTI ID:
1432662
Alternate ID(s):
OSTI ID: 1463031
Report Number(s):
LLNL-JRNL-737511; TRN: US1802661
Journal Information:
The Astrophysical Journal (Online), Vol. 854, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 3 works
Citation information provided by
Web of Science

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Cited By (3)

Solar UV and X-ray spectral diagnostics journal August 2018
Electron-density-sensitive Line Ratios of Fe XIII--XVI from Laboratory Sources Compared to CHIANTI dataset January 2018
Solar UV and X-Ray Spectral Diagnostics text January 2018

Figures / Tables (11)