I introduce techniques to derive the major properties of prominences based on NLTE modelling. The main results of one- and two-dimensional models of the prominences and their fine-structures are presented. Modelling the radiative transfer processes out of local thermodynamic equilibrium allows one to retrieve the prominence plasma parameters (temperature, density, pressure, ionisation degree) as well as the prominence’s mass
Aims. The aim of this work is to analyse the multi-instrument observations of the June 22, 2010 prom...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
Aims. We use 3D non-linear force-free magnetic field modeling of prominence/filament magnetic fields...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
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...
This review paper outlines background information and covers recent advances made via the analysis o...
International audienceThis review paper outlines background information and covers recent advances m...
International audienceContext. With more than four years of IRIS observations, and in order to avoid...
Prominence eruptions are one of the most spectacular manifestations of our Sun's activity. Yet there...
This paper presents several magnetohydrostatic equilibrium models for prominences with fibril-like f...
Aims.We outline the construction of prominence – corona transition region models based upon the obse...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
In this work we study the hydrogen, helium and calcium spectra emitted by a one-dimensional prominen...
We studied the physical conditions of an erupting prominence observed in the core of a coronal mass ...
Aims. The aim of this work is to analyse the multi-instrument observations of the June 22, 2010 prom...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
Aims. We use 3D non-linear force-free magnetic field modeling of prominence/filament magnetic fields...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
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...
This review paper outlines background information and covers recent advances made via the analysis o...
International audienceThis review paper outlines background information and covers recent advances m...
International audienceContext. With more than four years of IRIS observations, and in order to avoid...
Prominence eruptions are one of the most spectacular manifestations of our Sun's activity. Yet there...
This paper presents several magnetohydrostatic equilibrium models for prominences with fibril-like f...
Aims.We outline the construction of prominence – corona transition region models based upon the obse...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
In this work we study the hydrogen, helium and calcium spectra emitted by a one-dimensional prominen...
We studied the physical conditions of an erupting prominence observed in the core of a coronal mass ...
Aims. The aim of this work is to analyse the multi-instrument observations of the June 22, 2010 prom...
We present the first 3D whole-prominence fine structure model. The model combines a 3D magnetic fiel...
Aims. We use 3D non-linear force-free magnetic field modeling of prominence/filament magnetic fields...