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: Oscillations [S]
| 9
|
| Sun: Corona [S]
| 9
|
| The Sun [S]
| 7
|
| Sun: Flares [S]
| 7
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 7
|
| Sun: Magnetic Fields
| 6
|
| Sun: Atmosphere [S]
| 6
|
| Magnetohydrodynamics [S]
| 5
|
| Solar And Stellar Astrophysics
| 4
|
| Stars: Oscillations
| 3
|
| Sun: UV Radiation [S]
| 3
|
| Waves
| 3
|
| Solar Coronal Waves [S]
| 3
|
| Sun: Activity
| 2
|
| Stellar Oscillations
| 2
|
| Stellar Flares
| 2
|
| Space Weather
| 2
|
| Solar Instruments
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Methods: Numerical
| 2
|
| Maser Instability
| 2
|
| Magnetic Reconnection
| 2
|
| Loss-cone
| 2
|
| Convolutional Neural Networks
| 2
|
| Astronomy Data Analysis
| 2
|
| Techniques: Image Processing
| 2
|
| Stars: Flare
| 1
|
| Geomagnetic Storms
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Gamma Rays [S]
| 1
|
| Electron Cyclotron
| 1
|
| Solar Extreme Event
| 1
|
| Turbulence
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Seismology
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Upper-hybrid
| 1
|
| Ribbon Flares
| 1
|
| Oscillations
| 1
|
| Neural Networks
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Deep Learning
| 1
|
| Methods: Data Analysis
| 1
|
| Maximum Growth
| 1
|
| Corona [S]
| 1
|
| Weakly Relativistic
| 1
|
| Z Mode
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun: X-rays [S]
| 1
|
| Active Region
| 1
|
| Auroral Radiation
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Historical Observations
| 1
|
| Stellar Coronal Loops
| 1
|
| Time Series Analysis
| 1
|
| Stars: Magnetic Field
| 1
|
| Stars: Activity
| 1
|