We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic field configuration of an entire prominence obtained from non-linear force-free field simulations, with a detailed description of the prominence plasma. The plasma is located in magnetic dips in hydrostatic equilibrium and is distributed along multiple fine structures within the 3D magnetic model. Through the use of a novel radiative transfer visualization technique for the Hα line such plasma loaded magnetic field model produces synthetic images of the modeled prominence comparable with high-resolution observations. This allows us for the first time to use a single technique to consistently study, in both emission on the limb and absorption agai...
In this paper we construct theoretical models for vertical prominence threads which are in magnetohy...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
We investigate the properties of a "solar tornado" observed on 2014 July 15, and aim to link the beh...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
We use the new three-dimensional (3D) whole-prominence fine structure model to study the evolution o...
Aims. We analyze distributions of the magnetic field strength and prominence plasma (temperature, pr...
Aims. We analyze distributions of the magnetic field strength and prominence plasma (temperature, pr...
Aims. We use 3D non-linear force-free magnetic field modeling of prominence/filament magnetic fields...
Aims. The aim of this work is to analyse the multi-instrument observations of the June 22, 2010 prom...
High-resolution Ha images of solar filaments show a variety of dark fine-structure fibrils, most of ...
Abstract Magnetic fields suspend the relatively cool material of solar prominences in an otherwise h...
P.H. acknowledges the support from grant 209/12/0906 of the Grant Agency of the Czech Republic. S.G....
International audienceContext. Direct magnetic field measurements in solar prominences occur infrequ...
International audienceObservations and models of solar prominences are reviewed. We focus on non-eru...
Aims. We present a novel approximate radiative transfer method developed to visualize 3D w...
In this paper we construct theoretical models for vertical prominence threads which are in magnetohy...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
We investigate the properties of a "solar tornado" observed on 2014 July 15, and aim to link the beh...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
We use the new three-dimensional (3D) whole-prominence fine structure model to study the evolution o...
Aims. We analyze distributions of the magnetic field strength and prominence plasma (temperature, pr...
Aims. We analyze distributions of the magnetic field strength and prominence plasma (temperature, pr...
Aims. We use 3D non-linear force-free magnetic field modeling of prominence/filament magnetic fields...
Aims. The aim of this work is to analyse the multi-instrument observations of the June 22, 2010 prom...
High-resolution Ha images of solar filaments show a variety of dark fine-structure fibrils, most of ...
Abstract Magnetic fields suspend the relatively cool material of solar prominences in an otherwise h...
P.H. acknowledges the support from grant 209/12/0906 of the Grant Agency of the Czech Republic. S.G....
International audienceContext. Direct magnetic field measurements in solar prominences occur infrequ...
International audienceObservations and models of solar prominences are reviewed. We focus on non-eru...
Aims. We present a novel approximate radiative transfer method developed to visualize 3D w...
In this paper we construct theoretical models for vertical prominence threads which are in magnetohy...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
We investigate the properties of a "solar tornado" observed on 2014 July 15, and aim to link the beh...