Using the infrared iron lines to probe solar subsurface convection

Context. Studying the properties of solar convection using high-resolution spectropolarimetry began in the early 1990s with the focus on observations in the visible wavelength regions. Its extension to the infrared (IR) remains largely unexplored. Aims. The IR iron lines around 15 600 Å, most common...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2019-10, Vol.630, p.A133
Hauptverfasser:	Milić, I., Smitha, H. N., Lagg, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Diagnostic systems Fluid flow Iron Line of sight Line spectra line: profiles Magnetohydrodynamic simulation methods: data analysis Photosphere Solar convection (astronomy) Stray light Sun: infrared
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!