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  Identification of spectral lines in the 500-1600 Å wavelength range of highly ionized Ne, Na, Ar, K, Ca, Ti, Cr, Mn, Fe, Co, and Ni emitted by flares (Te gt;= 3 × 106 K) and their potential use in plasma diagnostics

Feldman, U., Curdt, W., Landi, E., & Wilhelm, K. (2000). Identification of spectral lines in the 500-1600 Å wavelength range of highly ionized Ne, Na, Ar, K, Ca, Ti, Cr, Mn, Fe, Co, and Ni emitted by flares (Te gt;= 3 × 106 K) and their potential use in plasma diagnostics. Astrophysical Journal, 544, 508-521.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-E118-D Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-E119-B
Genre: Journal Article

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 Creators:
Feldman, U., Author
Curdt, W.1, 2, Author           
Landi, E.2, Author           
Wilhelm, K.1, 2, Author           
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: SOHO: SUMER
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 Dates: 2000
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: BibTex Citekey: Feldman:2000-097
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Title: Astrophysical Journal
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 544 Sequence Number: - Start / End Page: 508 - 521 Identifier: -