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Quiet-Sun imaging asymmetries in Na I D1 compared with other strong Fraunhofer lines
R.J. Rutten
, J. Leenaarts
, L.H.M. Rouppe van der Voort
, A.G. de Wijn
, M. Carlsson
, V. Hansteen
Dept of Physics
extern
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Keyphrases
D1 Line
100%
Quiet Sun
100%
Granulation
100%
Wing Display
100%
Fraunhofer Lines
100%
Magnetic Concentration
50%
Internetwork
50%
Solar Atmosphere
50%
Photosphere
50%
Spectral Lines
50%
Line Wings
50%
Shock
50%
Opacity
50%
Solar Telescope
50%
Common Format
50%
Blue Line
50%
Line Yield
50%
1D Modeling
50%
Core Formation
50%
Line Formation
50%
Magnetohydrodynamical Simulations
50%
Spectral Image
50%
Imaging Spectroscopy
50%
Dopplershifts
50%
Red Lines
50%
Earth and Planetary Sciences
Photosphere
100%
Solar Atmosphere
100%
Line Spectra
100%
Fraunhofer Line
100%
Physics
Quiet Sun
100%
Solar Atmosphere
50%
Solar Telescopes
50%
Photosphere
50%
Line Spectra
50%