RELATIONSHIP between CHROMOSPHERIC EVAPORATION and MAGNETIC FIELD TOPOLOGY in AN M-CLASS SOLAR FLARE

Keyphrases

• Advanced Technology Solar Telescope 33%
• Arcade 33%
• Blue Shift 100%
• Chromosphere 33%
• Chromospheric Evaporation 100%
• Energy Release 33%
• Flux Rope 33%
• High-resolution Observations 33%
• Imaging Spectrometer 66%
• Interface Region 33%
• Local Magnetic Field 33%
• Low-lying 33%
• Magnetic Field Topology 66%
• Magnetic Polarity 33%
• Multi-wavelength Observations 33%
• Polarity Inversion 66%
• Quasi-separatrix Layer 33%
• Ribbon 33%
• Solar Dynamics Observatory 33%
• Solar Flares 100%
• Spatial Distribution 33%
• Spatially Resolved 33%
• Vector Magnetograms 33%
• Visible Imaging 33%

Physics

• Energetics 33%
• Helioseismology 33%
• High Resolution 33%
• Magnetic Field 66%
• Solar Flare 100%
• Solar Telescopes 33%
• Spatial Distribution 33%
• Spectrographs 33%

Earth and Planetary Sciences

• Helioseismology 33%
• Magnetic Signature 33%
• Solar Flare 100%
• Spatial Distribution 33%
• Spectrographs 33%