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Fernando Moreno Insertis

Spanish National Research Council
University of La Laguna

20

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441

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Self-Similar Approach for Rotating Magnetohydrodynamic Solar and Astrophysical Structures

2018 arXiv: Solar and Stellar Astrophysics
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ARE TORNADO-LIKE MAGNETIC STRUCTURES ABLE TO SUPPORT SOLAR PROMINENCE PLASMA?

2015 The Astrophysical Journal
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Continuum Intensity and [O I] Spectral Line Profiles in Solar 3D Photospheric Models: The Effect of Magnetic Fields

2015 The Astrophysical Journal
- Damian Fabbian
- Fernando Moreno Insertis
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MULTI-PARAMETRIC STUDY OF RISING 3D BUOYANT FLUX TUBES IN AN ADIABATIC STRATIFICATION USING AMR

2015 The Astrophysical Journal
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The power spectrum of solar convection flows from high-resolution observations and 3D simulations

2014 Astronomy and Astrophysics
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Twisting solar coronal jet launched at the boundary of an active region

2013 arXiv: Solar and Stellar Astrophysics
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Plasma Jets and Eruptions in Solar Coronal Holes: A Three-dimensional Flux Emergence Experiment

2013 The Astrophysical Journal
- Fernando Moreno Insertis
- Klaus Galsgaard
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Solar Fe abundance and magnetic fields - Towards a consistent reference metallicity

2012 arXiv: Solar and Stellar Astrophysics
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SOLAR ABUNDANCE CORRECTIONS DERIVED THROUGH THREE-DIMENSIONAL MAGNETOCONVECTION SIMULATIONS

2010 The Astrophysical Journal
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The effect of the relative orientation between the coronal field and new emerging flux: I Global Properties

2007 arXiv: Astrophysics
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