A comparison between measurements of solar EUV spectral line intensities 
emitted by C, N, O, and S ions and theoretical calculations

Doschek, E. E.; Laming, J. M.; Doschek, G. A.; Feldman, U.; Wilhelm, K.

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A comparison between measurements of solar EUV spectral line intensities emitted by C, N, O, and S ions and theoretical calculations

Doschek, E. E., Laming, J. M., Doschek, G. A., Feldman, U., & Wilhelm, K. (1999). A comparison between measurements of solar EUV spectral line intensities emitted by C, N, O, and S ions and theoretical calculations. Astrophysical Journal, 518, 909-917.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-DBBF-6 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-DBC0-D

Genre: Journal Article

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Doschek, E. E., Author
Laming, J. M., Author
Doschek, G. A., Author
Feldman, U., Author
Wilhelm, K.^{1, 2}, Author

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1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289

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MPIS_GROUPS: Sun and Heliosphere

MPIS_PROJECTS: SOHO: SUMER

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Dates: Date issued: 1999

Publication Status: Issued

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Rev. Type: Peer

Identifiers: BibTex Citekey: Doschek:1999-054

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Title: Astrophysical Journal

Source Genre: Journal

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Pages: - Volume / Issue: 518 Sequence Number: - Start / End Page: 909 - 917 Identifier: -