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POLARIZED LINE TRANSFER WITH F-STATE INTERFERENCE IN A NON-MAGNETIC MEDIUM: PARTIAL FREQUENCY REDISTRIBUTION EFFECTS IN THE COLLISIONLESS REGIME

The Astrophysical journal, 2012-10, Vol.758 (2), p.1-7

2012

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Using the infrared iron lines to probe solar subsurface convection

Astronomy and astrophysics (Berlin), 2019-10, Vol.630, p.A133

2019

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globin: A spectropolarimetric inversion code for the coupled inference of atomic line parameters

Astronomy and astrophysics (Berlin), 2024-06, Vol.686, p.A262

2024

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The influence of NLTE effects in Fe I lines on an inverted atmosphere

Astronomy and astrophysics (Berlin), 2020-01, Vol.633

2020

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Ti I lines at 2.2 μ m as probes of the cooler regions of sunspots

Astronomy and astrophysics (Berlin), 2021-09, Vol.653, p.A91

2021

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Quantum interference with angle-dependent partial frequency redistribution: solution of the polarized line transfer in the non-magnetic case

Monthly notices of the Royal Astronomical Society, 2013-02, Vol.429 (1), p.275-280

2013

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Radiative transfer with J-state interference in a two-term atom Partial frequency redistribution in the non-magnetic case

Astronomy and astrophysics (Berlin), 2011-11, Vol.535, p.A35

2011

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The influence of NLTE effects in Fe I lines on an inverted atmosphere: I. 6301 Å and 6302 Å lines formed in 1D NLTE

Astronomy and astrophysics (Berlin), 2020-01, Vol.633, p.A157

2020

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Non-LTE formation of the Fe I 6173 Å line in the solar atmosphere

Astronomy and astrophysics (Berlin), 2023-01, Vol.669, p.A144

2023

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The influence of NLTE effects in Fe I lines on an inverted atmosphere: II. 6301 Å and 6302 Å lines formed in 3D NLTE

Astronomy and astrophysics (Berlin), 2021-03, Vol.647, p.A46

2021

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The influence of NLTE effects in Fe I lines on an inverted atmosphere

Astronomy and astrophysics (Berlin), 2021-03, Vol.647

2021

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A revisit to model the Cr i triplet at 5204-5208 Å and the Ba ii D2 line at 4554 Å in the Second Solar Spectrum

Proceedings of the International Astronomical Union, 2014-12, Vol.10 (S305), p.372-376

2014

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Forward-scattering Hanle effect in the solar Ca i 4227 Å line

EAS publications series, 2012, Vol.55, p.59-63

2012

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THE QUANTUM INTERFERENCE EFFECTS IN THE SC II 4247 Å LINE OF THE SECOND SOLAR SPECTRUM

The Astrophysical journal, 2014-10, Vol.794 (1), p.30

2014

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THE QUANTUM INTERFERENCE EFFECTS IN THE SC II 4247 A LINE OF THE SECOND SOLAR SPECTRIM

The Astrophysical journal, 2014-01, Vol.794 (1), p.1-9

2014

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MODELING THE QUANTUM INTERFERENCE SIGNATURES OF THE Ba II D sub(2) 4554 [Angstrom] LINE IN THE SECOND SOLAR SPECTRUM

The Astrophysical journal, 2013-05, Vol.768 (2), p.1-8

2013

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MODELING THE QUANTUM INTERFERENCE SIGNATURES OF THE Ba II D 2 4554 Å LINE IN THE SECOND SOLAR SPECTRUM

The Astrophysical journal, 2013-04, Vol.768 (2), p.163

2013

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Radiative transfer with J-state interference in a two-term atom

Astronomy and astrophysics (Berlin), 2011-11, Vol.535

2011

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J-state interference signatures in the second solar spectrum

Astronomy and astrophysics (Berlin), 2012-05, Vol.541

2012

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J -state interference signatures in the second solar spectrum: Modeling the Cr i triplet at 5204–5208 Å

Astronomy and astrophysics (Berlin), 2012-05, Vol.541, p.A24

2012

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J-state interference signatures in the second solar spectrum: Modeling the CrI triplet at 5204―5208 A

Astronomy and astrophysics (Berlin), 2012, Vol.541

2012

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A revisit to model the Cr i triplet at 5204-5208 Å and the Ba ii D 2 line at 4554 Å in the Second Solar Spectrum

Proceedings of the International Astronomical Union, 2014-12, Vol.10 (S305), p.372-376

2014

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Observations of the forward scattering Hanle effect in the Cal 4227 A line

Astronomy and astrophysics (Berlin), 2011, Vol.530

2011

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Classroom

Resonance, 2007-12, Vol.12 (12), p.46-52

Smitha, H. N.

2007

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A revisit to model the Cr i triplet at 5204-5208 Aa and the Ba ii D sub(2) line at 4554 Aa in the Second Solar Spectrum

Proceedings of the International Astronomical Union, 2014-12, Vol.10 (S305), p.372-376

2014

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POLARIZED LINE TRANSFER WITH F-STATE INTERFERENCE IN A NON-MAGNETIC MEDIUM: PARTIAL FREQUENCY REDISTRIBUTION EFFECTS IN THE COLLISIONLESS REGIME

Using the infrared iron lines to probe solar subsurface convection

globin: A spectropolarimetric inversion code for the coupled inference of atomic line parameters

The influence of NLTE effects in Fe I lines on an inverted atmosphere

Ti I lines at 2.2 μ m as probes of the cooler regions of sunspots

Quantum interference with angle-dependent partial frequency redistribution: solution of the polarized line transfer in the non-magnetic case

Radiative transfer with J-state interference in a two-term atom Partial frequency redistribution in the non-magnetic case

The influence of NLTE effects in Fe I lines on an inverted atmosphere: I. 6301 Å and 6302 Å lines formed in 1D NLTE

Non-LTE formation of the Fe I 6173 Å line in the solar atmosphere

The influence of NLTE effects in Fe I lines on an inverted atmosphere: II. 6301 Å and 6302 Å lines formed in 3D NLTE

The influence of NLTE effects in Fe I lines on an inverted atmosphere

A revisit to model the Cr i triplet at 5204-5208 Å and the Ba ii D2 line at 4554 Å in the Second Solar Spectrum

Forward-scattering Hanle effect in the solar Ca i 4227 Å line

THE QUANTUM INTERFERENCE EFFECTS IN THE SC II 4247 Å LINE OF THE SECOND SOLAR SPECTRUM

THE QUANTUM INTERFERENCE EFFECTS IN THE SC II 4247 A LINE OF THE SECOND SOLAR SPECTRIM

MODELING THE QUANTUM INTERFERENCE SIGNATURES OF THE Ba II D sub(2) 4554 [Angstrom] LINE IN THE SECOND SOLAR SPECTRUM

MODELING THE QUANTUM INTERFERENCE SIGNATURES OF THE Ba II D 2 4554 Å LINE IN THE SECOND SOLAR SPECTRUM

Radiative transfer with J-state interference in a two-term atom

J-state interference signatures in the second solar spectrum

J -state interference signatures in the second solar spectrum: Modeling the Cr i triplet at 5204–5208 Å

J-state interference signatures in the second solar spectrum: Modeling the CrI triplet at 5204―5208 A

A revisit to model the Cr i triplet at 5204-5208 Å and the Ba ii D 2 line at 4554 Å in the Second Solar Spectrum

Observations of the forward scattering Hanle effect in the Cal 4227 A line

Classroom

A revisit to model the Cr i triplet at 5204-5208 Aa and the Ba ii D sub(2) line at 4554 Aa in the Second Solar Spectrum

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