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: Corona [S]
| 9
|
| Sun: Oscillations [S]
| 9
|
| The Sun [S]
| 7
|
| Sun: Flares [S]
| 6
|
| Sun: Magnetic Fields
| 6
|
| Sun: Atmosphere [S]
| 6
|
| Magnetohydrodynamics [S]
| 5
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 5
|
| Solar And Stellar Astrophysics
| 4
|
| Sun: UV Radiation [S]
| 3
|
| Stars: Oscillations
| 3
|
| Waves
| 3
|
| Sun: Activity
| 2
|
| Space Weather
| 2
|
| Solar Instruments
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 2
|
| Solar Coronal Waves [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
|
| Turbulence
| 1
|
| Stars: Flare
| 1
|
| Stars: Activity
| 1
|
| Historical Observations
| 1
|
| Solar X-ray Flares [S]
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Geomagnetic Storms
| 1
|
| Gamma Rays [S]
| 1
|
| Solar Extreme Event
| 1
|
| Electron Cyclotron
| 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
|
| Auroral Radiation
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: X-rays [S]
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Active Region
| 1
|
| Time Series Analysis
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Stellar Oscillations
| 1
|
| Stellar Flares
| 1
|
| Stellar Coronal Loops
| 1
|
| Stars: Magnetic Field
| 1
|