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Cited article:
D. Orozco Suárez, L. R. Bellot Rubio, J. C. del Toro Iniesta
A&A, 518 (2010) A3
Published online: 2010-08-18
This article has been cited by the following article(s):
Milne-Eddington inversion of the Fe I line pair at 630 nm
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DOI: 10.1051/0004-6361/201014374
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High-resolution Observation of Moving Magnetic Features
Qin Li, Na Deng, Ju Jing, Chang Liu and Haimin Wang
The Astrophysical Journal 876 (2) 129 (2019)
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Inferring the magnetic field vector in the quiet Sun
J. M. Borrero and P. Kobel
Astronomy & Astrophysics 527 A29 (2011)
DOI: 10.1051/0004-6361/201015634
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THE DISTRIBUTION OF QUIET-SUN MAGNETIC FIELDS AT DIFFERENT HELIOCENTRIC ANGLES
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The Astrophysical Journal 746 (2) 182 (2012)
DOI: 10.1088/0004-637X/746/2/182
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Distribution of magnetic fields in the quiet Sun
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ANALYSIS OF QUIET-SUN INTERNETWORK MAGNETIC FIELDS BASED ON LINEAR POLARIZATION SIGNALS
D. Orozco Suárez and L. R. Bellot Rubio
The Astrophysical Journal 751 (1) 2 (2012)
DOI: 10.1088/0004-637X/751/1/2
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Empirical determination of the temperature stratification in the photosphere of the quiet Sun
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Comparison of inversion codes for polarized line formation in MHD simulations
J. M. Borrero, B. W. Lites, A. Lagg, R. Rezaei and M. Rempel
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Chromospheric observations and magnetic configuration of a supergranular structure
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Astronomy & Astrophysics 621 A1 (2019)
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Quiet Sun magnetic fields: an observational view
Luis Bellot Rubio and David Orozco Suárez
Living Reviews in Solar Physics 16 (1) (2019)
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Applicability of Milne-Eddington inversions to high spatial resolution observations of the quiet Sun
D. Orozco Suárez, L. R. Bellot Rubio, A. Vögler and J. C. del Toro Iniesta
Astronomy and Astrophysics 518 A2 (2010)
DOI: 10.1051/0004-6361/200913421
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On the effect of oscillatory phenomena on Stokes inversion results
P. H. Keys, O. Steiner and G. Vigeesh
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 379 (2190) 20200182 (2021)
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