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

Astrophysical Journal

Volumn 521, Issue 1 PART 1, 1999, Pages 478-482

  Kuhn, J R ^a   Macqueen, R M ^b   Streete, J ^b   Tansey, G ^b   Mann, I ^c   Hillebrand, P ^c   Coulter, R ^d   Lin, H ^d   Edmunds, D ^e   Judge, P ^f  

^a UNIVERSITY OF HAWAII   (United States)

^b RHODES COLLEGE   (United States)

^c MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^d NATIONAL SOLAR OBSERVATORY   (United States)

^e MICHIGAN STATE UNIVERSITY   (United States)

^f NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

Author keywords

Sun: corona; Sun: infrared; Sun: magnetic fields

Indexed keywords

EID: 0033542953     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/307529     Document Type: Article

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