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Astrophysical Journal Letters, ISSN 2041-8205, 01/2014, Volume 780, Issue 1, pp. 1 - 7
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2018, Volume 618, p. A176
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2016, Volume 596, p. A41
Context. Suprathermal tails are a common feature of solar wind electron velocity distributions, and are expected in the solar corona. From the corona,... 
Sun: transition region | Plasmas | Methods: numerical | WIND | plasmas | CORONA | methods: numerical | SUN | ACCELERATION | WAVES | KAPPA DISTRIBUTIONS | ASTRONOMY & ASTROPHYSICS | GENERATION | HEAT-FLOW | HALO | Coronas | Electron velocity distribution | Local thermodynamic equilibrium | Ionization | Boundary conditions | Mathematical models | Electron distribution | Electron energy
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A17
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 11/2017, Volume 607, p. A80
Context. We study the physics of erupting prominences in the core of coronal mass ejections (CMEs) and present a continuation of a previous analysis. Aims. We... 
Line: formation | Radiative transfer | Sun: UV radiation | Techniques: spectroscopic | Sun: coronal mass ejections (CMEs) | RATE COEFFICIENTS | radiative transfer | SOHO OBSERVATIONS | IONS | UV radiation | HYDROGEN | line: formation | ELECTRON-IMPACT-EXCITATION | ASTRONOMY & ASTROPHYSICS | techniques: spectroscopic Sun | EQUILIBRIUM | EMISSION
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 531, p. A122
Aims. The solar transition region satisfies the conditions for appearance of the non-thermal.-distribution. We aim to prove the occurrence of the non-thermal... 
Sun: UV-radiation | Sun: transition region | RATIOS | CORONA | MAXWELLIAN ELECTRON-DISTRIBUTION | EMISSION-LINES | FOKKER-PLANCK | ENERGY DISTRIBUTIONS | DENSITY | OXYGEN | ATOMIC DATABASE | ASTRONOMY & ASTROPHYSICS | IONIZATION EQUILIBRIUM
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2018, Volume 864, Issue 1
We analyze the spectra of high-temperature Fe XXIV lines observed by the Hinode/Extreme-Ultraviolet Imaging Spectrometer (EIS) during the impulsive phase of... 
Sun: flares | Sun: activity | Sun: UV radiation | line: profiles | techniques: spectroscopic | radiation mechanisms: nonthermal | SPECTROMETER | FIELD | RESOLUTION | CORONA | X-RAY-SPECTRA | FAST SOLAR-WIND | REGION | PLASMA | ASTRONOMY & ASTROPHYSICS | EMISSION | RHESSI | Physics - Solar and Stellar Astrophysics
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2018, Volume 610, p. A67
Context. Transition region (TR) spectra typically show the Si IV 1402.8 angstrom line to be enhanced by a factor of 5 or more compared to the neighboring O IV... 
Sun: UV radiation | Radiation mechanisms: Non-thermal | Sun: Transition region | radiation mechanisms non-thermal | EXCITATION | Sun UV radiation | CORONAL LOOPS | RADIATION | FOKKER-PLANCK | FLARE | ASTRONOMY & ASTROPHYSICS | EXTREME-ULTRAVIOLET | SOLAR | EQUILIBRIUM | DENSITY DIAGNOSTICS | EMISSION | Sun transition region | Physics - Solar and Stellar Astrophysics
Journal Article