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  Probable detection of a bright infrared coronal emission line of Si IX near 3.93 microns

Mann, I., Kuhn, J. R., MacQueen, R. M., Streete, J., Tansey, G., Hillebrand, P., et al. (1999). Probable detection of a bright infrared coronal emission line of Si IX near 3.93 microns. Astrophysical Journal, 521, 478-482.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-DEA5-4 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-DEA6-2
Genre: Journal Article

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 Creators:
Mann, I.1, Author              
Kuhn, J. R., Author
MacQueen, R. M., Author
Streete, J., Author
Tansey, G., Author
Hillebrand, P., Author
Colter, R., Author
Lin, H., Author
Edmund, D., Author
Judge, P., Author
Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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Free keywords: -
 MPIS_GROUPS: Sun and Heliosphere
 Abstract: -

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 Dates: 1999
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: BibTex Citekey: Mann:1999-359
 Degree: -

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Title: Astrophysical Journal
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 521 Sequence Number: - Start / End Page: 478 - 482 Identifier: -