Polarization in spectral lines

By E. L. Degl'innocenti. 2004

611 citations recorded by the source corpus.

Subfields: Atmospheric Science, Atomic and Molecular Physics, and Optics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/cd7c339d794a4d879bad91e84a44bf4d20920795

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Atmospheric Science

1. S. Solanki
2. J. C. D. T. Iniesta
3. T. Wiegelmann
4. T. Sakurai

In Atomic and Molecular Physics, and Optics

1. T. Wiegelmann
2. T. Sakurai
3. S. Solanki
4. J. C. D. T. Iniesta
5. Laurent Gizon

In Spectroscopy

1. J. C. D. T. Iniesta
2. T. Wiegelmann
3. T. Sakurai

Citations in the corpus

• Least-squares deconvolution of the stellar intensity and polarization spectra (2010, neutral): “…intrinsic width of the spectral lines determined by the thermal Doppler broadening∆λD, one can derive approximate expressions relating intensity (StokesI ) with the Stokes parameters characterizing circular (StokesV) and linear (StokesQU) polarization (e.g., Landi Degl’Innocenti & Landolfi 2004).”
• Solar Force-free Magnetic Fields (2012, methodology): “Within this work we only outline the main steps and refer to del Toro Iniesta and Ruiz Cobo (1996), del Toro Iniesta (2003) and Landi Degl’Innocenti and Landolfi (2004) for details.”
• The Polarimetric and Helioseismic Imager on Solar Orbiter (2019, methodology): “Then, B, γ, φ are obtained through the weak-field approximation (Landi Degl’Innocenti & Landolfi 2004).”