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

Kuhn, J. R.; MacQueen, R. M.; Streete, J.; Tansey, G.; Mann, I.; Hillebrand, P.; Coulter, R.; Lin, H.

Local TagsRelease HistoryDetailsSummary

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

Kuhn, J. R., MacQueen, R. M., Streete, J., Tansey, G., Mann, I., 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.

Item is Released

show all hide all

Basic

show hide

Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-E1B6-B Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-E1B7-9

Genre: Journal Article

Files

show Files

Locators

show

Creators

show

hide

Creators:
Kuhn, J. R., Author
MacQueen, R. M., Author
Streete, J., Author
Tansey, G., Author
Mann, I.¹, Author
Hillebrand, P., Author
Coulter, R., Author
Lin, H., Author

Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291

Content

show

Details

show

hide

Language(s):

Dates: Date issued: 1999

Publication Status: Issued

Pages: -

Publishing info: -

Table of Contents: -

Rev. Type: Peer

Identifiers: BibTex Citekey: Kuhn:1999-418

Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show

hide

Title: Astrophysical Journal

Source Genre: Journal

Creator(s):

Affiliations:

Publ. Info: -

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