Non-thermal broadening of IRIS Fe XXI line caused by turbulent plasma flows in the magnetic reconnection region during solar eruptions

Keyphrases

• Magnetic Reconnection 100%
• Reconnection 100%
• Solar Eruptions 100%
• Plasma Flow 100%
• Imaging Spectrometer 100%
• Interface Region 100%
• Turbulent Plasma 100%
• Thermal Broadening 100%
• Current Sheet 50%
• High Temperature 50%
• Highly Dynamic 50%
• Thermal Velocity 50%
• Solar Flares 25%
• Energy Release 25%
• Magnetohydrodynamic Model 25%
• Magnetohydrodynamic Simulation 25%
• Plasma Temperature 25%
• Plasma Density 25%
• Three-dimensional (3D) 25%
• Spectral Lines 25%
• Plasma Properties 25%
• Emission Lines 25%
• Velocity Range 25%
• Plasma Velocity 25%
• Line Map 25%
• Synthetic Profiles 25%
• UV Spectrometer 25%
• Primary Diagnostics 25%

Physics

• Spectrographs 100%
• Solar Prominence 100%
• Magnetohydrodynamic Flow 100%
• Current Sheet 66%
• Thermal Velocity 66%
• Solar Flare 33%
• Magnetohydrodynamics 33%
• Magnetohydrodynamic Simulation 33%
• Plasma Density 33%
• Spacecraft 33%
• Line Spectra 33%
• Plasma Property 33%

Earth and Planetary Sciences

• Spectrographs 100%
• Solar Prominence 100%
• Magnetohydrodynamic Flow 100%
• Current Sheet 66%
• Emissions 66%
• Solar Flare 33%
• Magnetohydrodynamic Simulation 33%
• Plasma Density 33%
• Spacecraft 33%
• Magnetohydrodynamics 33%
• Line Spectra 33%