Spanish Clinical Research Network

most citedDiagnosing the solar atmosphere through the Mg I b

_{2}

5173 Å line. I. Nonlocal thermodynamic equilibrium inversions versus traditional inferences

6 citations

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2 papers

astro-ph.SR2025★ 4 cited

Diagnosing the solar atmosphere through the Mg I b $_{2}$ 5173 Å line. II. Morphological classification of the intensity and circular polarization profiles

A. L. Siu-Tapia, L. R. Bellot Rubio, D. Orozco Suárez +1

The Mg I b $_{2}$ line at 5173 Å is primarily magnetically sensitive to heights between the mid photosphere and the low chromosphere, a region that has not been sufficiently explored…

astro-ph.SR2025★ 6 cited

Diagnosing the solar atmosphere through the Mg I b $_{2}$ 5173 Å line. I. Nonlocal thermodynamic equilibrium inversions versus traditional inferences

A. L. Siu-Tapia, L. R. Bellot Rubio, D. Orozco Suárez

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 t…

Diagnosing the solar atmosphere through the Mg I b2​ 5173 Å line. II. Morphological classification of the intensity and circular polarization profiles

Diagnosing the solar atmosphere through the Mg I b2​ 5173 Å line. I. Nonlocal thermodynamic equilibrium inversions versus traditional inferences

Diagnosing the solar atmosphere through the Mg I b $_{2}$ 5173 Å line. II. Morphological classification of the intensity and circular polarization profiles

Diagnosing the solar atmosphere through the Mg I b $_{2}$ 5173 Å line. I. Nonlocal thermodynamic equilibrium inversions versus traditional inferences