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.; Colter, R.; Lin, H.; Edmund, D.; Judge, P.

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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: https://hdl.handle.net/11858/00-001M-0000-0014-DEA5-4 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-DEA6-2

Genre: Journal Article

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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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MPIS_GROUPS: Sun and Heliosphere

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Dates: Date issued: 1999

Publication Status: Issued

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Rev. Type: Peer

Identifiers: BibTex Citekey: Mann:1999-359

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Title: Astrophysical Journal

Source Genre: Journal

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Pages: - Volume / Issue: 521 Sequence Number: - Start / End Page: 478 - 482 Identifier: -