The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Sun: Flares [S]
| 46
|
| Sun: Magnetic Fields
| 32
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 23
|
| Sun: Chromosphere [S]
| 17
|
| Sun: Activity
| 16
|
| Sun: Filaments [S]
| 14
|
| Sun: Coronal Mass Ejections
| 13
|
| Solar Active Region Magnetic Fields [S]
| 12
|
| Sun: Photosphere [S]
| 11
|
| Solar Activity
| 10
|
| Magnetohydrodynamics [S]
| 10
|
| Magnetohydrodynamical Simulations
| 9
|
| Solar Magnetic Reconnection
| 8
|
| Sun: X-rays [S]
| 8
|
| Solar Physics [S]
| 8
|
| Solar Wind [H]
| 7
|
| Sun: Corona [S]
| 7
|
| Solar Filament Eruptions
| 6
|
| Sun: Active Regions
| 6
|
| Sun: Atmosphere [S]
| 6
|
| Convolutional Neural Networks
| 5
|
| Quiet Sun
| 4
|
| Sunspots [S]
| 4
|
| Magnetic Fields
| 4
|
| Solar Radio Emission
| 4
|
| Solar Energetic Particles [H]
| 4
|
| Non-thermal Radiation Sources
| 3
|
| The Sun [S]
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Sun: Radio Radiation [S]
| 3
|
| Solar Coronal Holes [S]
| 3
|
| Gamma Rays [S]
| 3
|
| Interplanetary Physics [H]
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Solar Flare Spectra
| 2
|
| Jets
| 2
|
| Magnetic Reconnection
| 2
|
| Methods: Data Analysis
| 2
|
| Methods: Numerical
| 2
|
| Neural Networks
| 2
|
| Sun: UV Radiation [S]
| 2
|
| Solar Coronal Transients
| 2
|
| Astronomy Data Analysis
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Active Solar Chromosphere
| 2
|
| Sun: Particle Emission
| 2
|
| Solar Magnetic Flux Emergence
| 2
|
| Astronomy Databases
| 1
|
| Astronomy Data Visualization
| 1
|
| Artificial Intelligence
| 1
|
| Alfven Waves
| 1
|
| Active Solar Corona
| 1
|
| Transient Detection
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Solar Photosphere
| 1
|
| Sun: Rotation [S]
| 1
|
| Sun: Neural Networks
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Evolution
| 1
|
| Sun: Data Analysis
| 1
|
| Sun: Computer Science - Machine Learning
| 1
|
| Structure Coronal Mass Ejections
| 1
|
| Spectroscopy
| 1
|
| Space Weather
| 1
|
| Solar-terrestrial Interactions
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar Transition Region
| 1
|
| Solar Surface
| 1
|
| Solar Radio Flares
| 1
|
| Solar Particle Emission
| 1
|
| Solar Granulation
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Evolution
| 1
|
| Solar Active Region Filaments
| 1
|
| Shock Waves
| 1
|
| Random Forests
| 1
|
| Radiation Mechanisms: Non-thermal
| 1
|
| Plasma Diagnostics
| 1
|
| Plasma Control
| 1
|
| Nuclear Fusion
| 1
|
| Models Magnetohydrodynamics
| 1
|
| Methods: Observational
| 1
|
| Magnetic Fields Active Regions
| 1
|
| Machine Learning
| 1
|
| Line: Profiles
| 1
|
| 14j60
| 1
|
| Heliophysics
| 1
|
| Ground-based Astronomy
| 1
|
| Galaxies: Magnetic Fields
| 1
|
| Flares
| 1
|
| Dynamics Flares
| 1
|
| Delta Sunspots
| 1
|
| Data-driven Plasma Science
| 1
|
| Coronal Mass Ejections─interplanetary Shocks
| 1
|
| Coronal Mass Ejections: CMEs
| 1
|
| Computer Science - Machine Learning
| 1
|
| Computational Methods
| 1
|
| Active Regions
| 1
|
| Acceleration Of Particles
| 1
|
| Initiation And Propagation Flares
| 1
|