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ELECTRIC CURRENTS IN FLARE RIBBONS: OBSERVATIONS AND THREE-DIMENSIONAL STANDARD MODEL

The Astrophysical journal, 2014-06, Vol.788 (1), p.1-11

2014

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Magnetic field vector ambiguity resolution in a quiescent prominence observed on two consecutive days

Astronomy and astrophysics (Berlin), 2019-09, Vol.629, p.A138

2019

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Evolution of flare ribbons, electric currents, and quasi-separatrix layers during an X-class flare

Astronomy and astrophysics (Berlin), 2016-07, Vol.591, p.A141

2016

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The quiet Sun magnetic field: statistical description from THEMIS observations

Astronomy and astrophysics (Berlin), 2011-06, Vol.530, p.A51

Bommier, V.

2011

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Hard X-ray emitting energetic electrons and photospheric electric currents

Astronomy and astrophysics (Berlin), 2015-08, Vol.580, p.A106

2015

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Hanle effect from a dipolar magnetic structure: the case of the solar corona and the case of a star

Astronomy and astrophysics (Berlin), 2012-03, Vol.539, p.A122

Bommier, V.

2012

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24 synoptic maps of average magnetic field in 296 prominences measured by the Hanle effect during the ascending phase of solar cycle 21

Astronomy and astrophysics (Berlin), 2021-03, Vol.647, p.A60

2021

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Coexisting Flux Rope and Dipped Arcade Sections Along One Solar Filament

The Astrophysical journal, 2010-05, Vol.714 (1), p.343-354

2010

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Evidence for a Pre-Eruptive Twisted Flux Rope Using the Themis Vector Magnetograph

The Astrophysical journal, 2009-03, Vol.693 (1), p.L27-L30

2009

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Fast inversion of Zeeman line profiles using central moments: II. Stokes V moments and determination of vector magnetic fields

Astronomy and astrophysics (Berlin), 2016-07, Vol.591, p.A64

2016

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Topological Departures from Translational Invariance along a Filament Observed by THEMIS

Solar physics, 2008-03, Vol.248 (1), p.29-50

2008

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UNNOFIT inversion of spectro-polarimetric maps observed with THEMIS

Astronomy and astrophysics (Berlin), 2007-03, Vol.464 (1), p.323-339

2007

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Longitudinal magnetic field and velocity gradients in the photosphere inferred from THEMIS multiline observations

Astronomy and astrophysics (Berlin), 2013-04, Vol.552, p.np-np

2013

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Fast imaging spectroscopy with MSDP spectrometers. Vector magnetic maps with THEMIS/MSDP

Astronomy and astrophysics (Berlin), 2009-11, Vol.507 (1), p.531-539

2009

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Full non-LTE spectral line formation. III. The case of a two-level atom with broadened upper level

Astronomy and astrophysics (Berlin), 2024-08

2024

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Network velocity gradients in the photosphere I. Modeling

Astronomy and astrophysics (Berlin), 2011-07, Vol.531, p.A139

2011

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Fast inversion of Zeeman line profiles using central moments

Astronomy and astrophysics (Berlin), 2011-11, Vol.535, p.A45

2011

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The theoretical impact polarization of the O I 6300 Å red line of Earth aurorae

Annales geophysicae (1988), 2011, Vol.29 (1), p.71-79

2011

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Hanle effect from a dipolar magnetic structure: the case of the solar corona and the case of a star

Astronomy and astrophysics (Berlin), 2012-03, Vol.539, p.1-1

Bommier, V

2012

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Magnetic Causes of the Eruption of a Quiescent Filament

Solar physics, 2008-02, Vol.247 (2), p.321-333

2008

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Magnetic Field Structures in a Facular Region Observed by THEMIS and Hinode

Solar physics, 2010-03, Vol.262 (1), p.35-52

2010

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Interaction of magnetic field systems leading to an X1.7 flare due to large-scale flux tube emergence

Astronomy and astrophysics (Berlin), 2007-12, Vol.475 (3), p.1081-1091

2007

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Photospheric flows around a quiescent filament

Astronomy and astrophysics (Berlin), 2007-06, Vol.467 (3), p.1289-1298

2007

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The quiet Sun magnetic field observed with ZIMPOL on THEMIS★ I. The probability density function

Astronomy and astrophysics (Berlin), 2009-11, Vol.506 (3), p.1415-1428

2009

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A generalized $\sqrt{\epsilon}$-law: The role of unphysical source terms in resonance line polarization transfer and its importance as an additional test of NLTE radiative transfer codes

Astronomy and astrophysics (Berlin), 2007-06, Vol.468 (3), p.797-801

2007

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ELECTRIC CURRENTS IN FLARE RIBBONS: OBSERVATIONS AND THREE-DIMENSIONAL STANDARD MODEL

Magnetic field vector ambiguity resolution in a quiescent prominence observed on two consecutive days

Evolution of flare ribbons, electric currents, and quasi-separatrix layers during an X-class flare

The quiet Sun magnetic field: statistical description from THEMIS observations

Hard X-ray emitting energetic electrons and photospheric electric currents

Hanle effect from a dipolar magnetic structure: the case of the solar corona and the case of a star

24 synoptic maps of average magnetic field in 296 prominences measured by the Hanle effect during the ascending phase of solar cycle 21

Coexisting Flux Rope and Dipped Arcade Sections Along One Solar Filament

Evidence for a Pre-Eruptive Twisted Flux Rope Using the Themis Vector Magnetograph

Fast inversion of Zeeman line profiles using central moments: II. Stokes V moments and determination of vector magnetic fields

Topological Departures from Translational Invariance along a Filament Observed by THEMIS

UNNOFIT inversion of spectro-polarimetric maps observed with THEMIS

Longitudinal magnetic field and velocity gradients in the photosphere inferred from THEMIS multiline observations

Fast imaging spectroscopy with MSDP spectrometers. Vector magnetic maps with THEMIS/MSDP

Full non-LTE spectral line formation. III. The case of a two-level atom with broadened upper level

Network velocity gradients in the photosphere I. Modeling

Fast inversion of Zeeman line profiles using central moments

The theoretical impact polarization of the O I 6300 Å red line of Earth aurorae

Hanle effect from a dipolar magnetic structure: the case of the solar corona and the case of a star

Magnetic Causes of the Eruption of a Quiescent Filament

Magnetic Field Structures in a Facular Region Observed by THEMIS and Hinode

Interaction of magnetic field systems leading to an X1.7 flare due to large-scale flux tube emergence

Photospheric flows around a quiescent filament

The quiet Sun magnetic field observed with ZIMPOL on THEMIS★ I. The probability density function

A generalized $\sqrt{\epsilon}$-law: The role of unphysical source terms in resonance line polarization transfer and its importance as an additional test of NLTE radiative transfer codes

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