Solar Coronal Line Profiles in the Extreme-Ultraviolet
The Astrophysical Journal, 1974 U. Feldman, W. E. Behring
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Solar Flares and the Yellow Coronal Line.
The Astrophysical Journal, 1954 Frederick P. Dolder +2 more
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Modeling Solar Spectral Irradiance (SSI) from Iron lines using the COronal DEnsity and Temperature (CODET) model version 1.1 [PDF]
Jenny Marcela Rodríguez Gómez
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Reconnection of Magnetic Field Lines near the Solar Surface during Coronal Mass Ejection Propagation [PDF]
, 2004 A. A. Reinard, L. A. Fisk
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Proposed Resolution to the Solar Open Magnetic Flux Problem
The Astrophysical JournalThe solar magnetic fields emerging from the photosphere into the chromosphere and corona are comprised of a combination of closed (field lines with both ends rooted at the Sun) and open (field lines with only one end at the Sun) fields.
C. Nick Arge +4 more
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Laboratory Identification of Temperature Diagnostic Si
, 1997 Ilmar Kink +5 more
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Non-thermal broadening of coronal emission lines in the onset phase of solar flares and CMEs [PDF]
, 2006 H. R. M. Kay +3 more
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Solar limb flares and the yellow coronal line.
The Astronomical Journal, 1953 Frederick P. Dolder, Walter Orr Roberts
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Filament Mass Losses Forced by Magnetic Reconnection in the Solar Corona
The Astrophysical JournalRecent observations of the solar atmosphere in cool extreme-ultraviolet lines have reported the prevalence of coronal rain falling from coronal cloud filaments that are associated with the magnetic dips of coronal X-point structures.
Craig D. Johnston +6 more
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Investigating the Effect of Opacity in Soft X‐Ray Spectral Lines Emitted by Solar Coronal Active Regions [PDF]
, 1997 J. T. Schmelz +3 more
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