Diagnosing the solar atmosphere through the Mg I b2 5173 Å line: I. Nonlocal thermodynamic equilibrium inversions versus traditional inferences
Aims. We examined the capabilities of methods based on the weak-field approximation and line bisectors to extract fast and reliable information about the height stratification of the magnetic field and line-of-sight velocities, respectively, from high spatial resolution observations of the Mg I b2 l...
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/389421 |
| Acceso en línea: | http://hdl.handle.net/10261/389421 |
| Access Level: | acceso abierto |
| Palabra clave: | Polarization Sun: chromosphere Sun: magnetic fields |
| Sumario: | Aims. We examined the capabilities of methods based on the weak-field approximation and line bisectors to extract fast and reliable information about the height stratification of the magnetic field and line-of-sight velocities, respectively, from high spatial resolution observations of the Mg I b2 line at 5173 Å. |
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