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128 papers
An optically thin view of the solar chromosphere from observations of the O I 1355Å spectral line
Mats Carlsson, Bart De Pontieu
The O I 1355Å spectral line is one of the only optically thin lines that are both routinely observed and thought to be formed in the chromosphere. We present analysis of a variety…
Damping of coronal oscillations in self-consistent 3D radiative MHD simulations of the solar atmosphere
P. Kohutova, P. Antolin, M. Szydlarski +1
Oscillations are abundant in the solar corona. Coronal loop oscillations are typically studied using highly idealised models of magnetic flux tubes. In order to improve our underst…
Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage
Stephanie L. Yardley, Christopher J. Owen, David M. Long +76
The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilise the extensive suite of remote sensing and in situ instruments on board the ESA…
The F-CHROMA grid of 1D RADYN flare models
Mats Carlsson, Lyndsay Fletcher, Joel Allred +6
Context: Solar flares are the result of the sudden release of magnetic energy in the corona. Much of this energy goes into accelerating charged particles to high velocity. These pa…
Comparison of chromospheric diagnostics in a 3D model atmosphere: H linewidth and mm continua
Sneha Pandit, Sven Wedemeyer, Mats Carlsson +1
The Ha line, one of the most studied chromospheric diagnostics, is a tracer for magnetic field structures, while its line core intensity provides an estimate of the mass density. T…
Quiet Sun flux rope formation via incomplete Taylor relaxation
Rebecca Robinson, Guillaume Aulanier, Mats Carlsson
Low-altitude twisted magnetic fields may be relevant to atmospheric heating in the quiet Sun, but the exact role, topology, and formation of these twisted fields remains to be stud…