A Novel Investigation of the Small-scale Magnetic Activity of the Quiet Sun via the Hanle Effect in the Sr i 4607 Line

One of the key research problems in stellar physics is to decipher the small-scale magnetic activity of the quiet solar atmosphere. Recent magneto-convection simulations that account for small-scale dynamo action have provided three-dimensional (3D) models of the solar photosphere characterized by a...

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Veröffentlicht in:	The Astrophysical journal 2018-08, Vol.863 (2), p.164
Hauptverfasser:	del Pino Alemán, T., Trujillo Bueno, J., Št pán, J., Shchukina, N.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Atmospheric models Computer simulation Convection Depolarization Field strength Magnetic fields Photosphere Polarization Quiet Sun Radiative transfer Radiative transfer calculations Resonance lines Scattering Signal to noise ratio Solar atmosphere Solar telescopes Space telescopes Stellar physics Sun Sun: magnetic fields Sun: photosphere Telescopes Three dimensional models Variation
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