492 citations
- W. Schmidt2 profiles80 · h 35
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- Instituto de Astrofísica de CanariasES144 papers
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18 papers · 2 filters
Two-fluid numerical model of chromospheric heating and plasma outflows in a quiet-Sun
K. Murawski, Z. E. Musielak, S. Poedts +2
\textbf{Purpose:} This paper addresses long-standing solar physics problems, namely, the heating of the solar chromosphere and the origin of the solar wind. Our aim is to reveal th…
Combining magneto-hydrostatic constraints with Stokes profiles inversions. III. Uncertainty in the inference of electric currents
J. M. Borrero, A. Pastor Yabar
Electric currents play an important role in the energy balance of the plasma in the solar atmosphere. They are also indicative of non-potential magnetic fields and magnetic reconne…
Characterization of magneto-convection in sunspots -- The Gough & Tayler stability criterion in MURaM sunspot simulations
M. Schmassmann, M. Rempel, N. Bello González +2
We analyse a sunspot simulation in an effort to understand the origin of the convective instabilities giving rise to the penumbral and umbral distinct regimes. We applied the crite…
Effects of solar evolution on finite acquisition time of Fabry-Perot-Interferometers in high resolution solar physics
Rolf Schlichenmaier, Daniel Pitters, Juan Manuel Borrero +1
The imaging spectro-polarimeter VTF (Visible Tunable Filter) will be operated at the Daniel K. Inouye Solar Telescope (DKIST). Due to its capability of resolving dynamic fine struc…
An innovative and automated method for vortex identification. I. Description of the SWIRL algorithm
José Roberto Canivete Cuissa, Oskar Steiner
Context. A universally accepted definition of what a vortex is has not yet been reached. Therefore, we lack an unambiguous and rigorous method for the identification of vortices in…
The Propagation of Coherent Waves Across Multiple Solar Magnetic Pores
S. D. T. Grant, D. B. Jess, M. Stangalini +9
Solar pores are efficient magnetic conduits for propagating magnetohydrodynamic wave energy into the outer regions of the solar atmosphere. Pore observations often contain isolated…