Context. With more than four years of IRIS observations, and in order to avoid building customized diagnostics for each observation, it is useful to derive some simple relations between spectra and physical quantities. This is even more useful for the k and h lines of Mg I
The solar prominence radiation spectrum has been simulated in close H and K lines of ionized calcium...
The Chromospheric Lyman Alpha Spectropolarimeter (CLASP) observed the Sun in H i Lyα during a suborb...
The bulk of the radiative output of a solar flare is emitted from the chromosphere, which produces e...
International audienceContext. With more than four years of IRIS observations, and in order to avoid...
Context: Observations of the Mg II h and k lines in solar prominences with IRIS reveal a wide range...
Aims. We investigate a new method to for obtaining the plasma parameters of solar prominences observ...
Context. A flux emergence in the active region AR 111850 was observed on September 24, 201...
International audienceContext. A flux emergence in the active region AR 111850 was observed on Septe...
Date of Acceptance: 08/01/2015Mg ii h and k and Hα spectra in a dynamical prominence have been obtai...
We continued our investigation of the plasma characteristics of a quiescent prominence that occurred...
Context. Empirical relations between major UV and extreme UV spectral lines are one of the inputs fo...
Context. The interpretation of high-resolution spectropolarimetric observations of solar prominences...
International audienceAims. In this paper we focus on the possible observational signatures of the p...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
The Mg II h&k lines are the prime chromospheric diagnostics of NASA’s Interface Region Imaging S...
The solar prominence radiation spectrum has been simulated in close H and K lines of ionized calcium...
The Chromospheric Lyman Alpha Spectropolarimeter (CLASP) observed the Sun in H i Lyα during a suborb...
The bulk of the radiative output of a solar flare is emitted from the chromosphere, which produces e...
International audienceContext. With more than four years of IRIS observations, and in order to avoid...
Context: Observations of the Mg II h and k lines in solar prominences with IRIS reveal a wide range...
Aims. We investigate a new method to for obtaining the plasma parameters of solar prominences observ...
Context. A flux emergence in the active region AR 111850 was observed on September 24, 201...
International audienceContext. A flux emergence in the active region AR 111850 was observed on Septe...
Date of Acceptance: 08/01/2015Mg ii h and k and Hα spectra in a dynamical prominence have been obtai...
We continued our investigation of the plasma characteristics of a quiescent prominence that occurred...
Context. Empirical relations between major UV and extreme UV spectral lines are one of the inputs fo...
Context. The interpretation of high-resolution spectropolarimetric observations of solar prominences...
International audienceAims. In this paper we focus on the possible observational signatures of the p...
I introduce techniques to derive the major properties of prominences based on NLTE modelling. The ma...
The Mg II h&k lines are the prime chromospheric diagnostics of NASA’s Interface Region Imaging S...
The solar prominence radiation spectrum has been simulated in close H and K lines of ionized calcium...
The Chromospheric Lyman Alpha Spectropolarimeter (CLASP) observed the Sun in H i Lyα during a suborb...
The bulk of the radiative output of a solar flare is emitted from the chromosphere, which produces e...
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