Fe I line pairs with different magnetic sensitivity

Fe I line pairs with different magnetic sensitivity

We present a list of Fe I line pairs with different magnetic sensitivity which are suitable for measurement of solar magnetic fields using the Stokes V amplitude ratio. The list contains the spectral solar line data in the wavelength range λλ = 303–996 nm given by Gurtovenko and Kostyk.

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Veröffentlicht in:Kinematics and physics of celestial bodies 2009-12, Vol.25 (6), p.319-324
Hauptverfasser: Vasilyeva, I. E., Shchukina, N. G.
Format: Artikel
Sprache:eng
Schlagworte:
Astronomy
Astrophysics
Magnetic fields
Observations and Techniques
Physics
Physics and Astronomy
Solar Physics
Sun
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Beschreibung
Zusammenfassung:We present a list of Fe I line pairs with different magnetic sensitivity which are suitable for measurement of solar magnetic fields using the Stokes V amplitude ratio. The list contains the spectral solar line data in the wavelength range λλ = 303–996 nm given by Gurtovenko and Kostyk.
ISSN:0884-5913
1934-8401
DOI:10.3103/S0884591309060051