Observation and Modeling of the Circular Polarization of the Cr i Magnetic-field-induced Transition at 533.03 nm
| Autor: | Hao Li, Tanausú del Pino Alemán, Javier Trujillo Bueno, Franziska Zeuner |
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| Jazyk: | angličtina |
| Rok vydání: | 2024 |
| Předmět: | |
| Zdroj: | The Astrophysical Journal, Vol 964, Iss 2, p 155 (2024) |
| Druh dokumentu: | article |
| ISSN: | 1538-4357 05683513 |
| DOI: | 10.3847/1538-4357/ad2fbb |
| Popis: | We study the circular polarization of the magnetic-field-induced transition (MIT) between the 3 d ^5 ( ^6 S )4 d ^7 D _2 and 3 d ^5 ( ^6 S )4 p ^7 P _4 ° states of Cr i at 533.03 nm (wavelength in air). The fractional circular polarization V / I of this spectral line resulting from the solution of the radiation transfer problem in a sunspot model permeated by a homogeneous magnetic field of 3 kG shows amplitudes of about 2%. Spectropolarimetric observations of two sunspots were obtained with the Zurich Imaging Polarimeter-3 at the Istituto ricerche solari Aldo e Cele Daccò observatory in Locarno, Switzerland. The observed V / I profiles show approximately antisymmetrical shapes with an amplitude of around 0.1% and 0.2% for the two sunspots. The center of this profile coincides with the wavelengths predicted for the abovementioned MIT. We apply an inversion code to the spectropolarimetric data of the Cr i -permitted lines at 532.91 and 532.98 nm, as well as to the MIT line at 533.03 nm, to infer a stratification of the emitting atmosphere. We compare the V / I profiles synthesized in the inferred atmosphere models with the observations, showing that the observed signal likely corresponds to the MIT line. |
| Databáze: | Directory of Open Access Journals |
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