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]
| 45
|
| Sun: Magnetic Fields
| 32
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 23
|
| Sun: Chromosphere [S]
| 17
|
| Sun: Activity
| 16
|
| Sun: Filaments [S]
| 13
|
| Sun: Coronal Mass Ejections
| 13
|
| Sun: Photosphere [S]
| 11
|
| Solar Active Region Magnetic Fields [S]
| 10
|
| Solar Activity
| 9
|
| Magnetohydrodynamics [S]
| 8
|
| Solar Magnetic Reconnection
| 8
|
| Sun: X-rays [S]
| 7
|
| Solar Physics [S]
| 7
|
| Magnetohydrodynamical Simulations
| 7
|
| Solar Wind [H]
| 7
|
| Sun: Atmosphere [S]
| 6
|
| Sun: Active Regions
| 6
|
| Sun: Corona [S]
| 6
|
| Convolutional Neural Networks
| 5
|
| Solar Filament Eruptions
| 5
|
| Magnetic Fields
| 4
|
| Sunspots [S]
| 4
|
| Solar Radio Emission
| 4
|
| Solar Energetic Particles [H]
| 4
|
| Quiet Sun
| 4
|
| Interplanetary Magnetic Fields [H]
| 3
|
| The Sun [S]
| 3
|
| Gamma Rays [S]
| 3
|
| Sun: Radio Radiation [S]
| 3
|
| Sun: UV Radiation [S]
| 2
|
| Solar Magnetic Flux Emergence
| 2
|
| Magnetic Reconnection
| 2
|
| Solar Coronal Transients
| 2
|
| Methods: Data Analysis
| 2
|
| Methods: Numerical
| 2
|
| Sun: Particle Emission
| 2
|
| Solar Flare Spectra
| 2
|
| Neural Networks
| 2
|
| Non-thermal Radiation Sources
| 2
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 2
|
| Active Solar Chromosphere
| 2
|
| Astronomy Data Analysis
| 2
|
| Jets
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Interplanetary Physics [H]
| 2
|
| Solar Coronal Holes [S]
| 2
|
| 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
|
| 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
|
| 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
|
| Initiation And Propagation Flares
| 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
|
| Astronomy Databases
| 1
|
| Astronomy Data Visualization
| 1
|
| Artificial Intelligence
| 1
|
| Active Regions
| 1
|
| Acceleration Of Particles
| 1
|
| 14j60
| 1
|