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