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]
| 17
|
| Sun: Spectrum
| 7
|
| Sun: X-rays [S]
| 5
|
| Sun: Filaments [S]
| 5
|
| Sun: X-ray Bursts
| 4
|
| Sun: Oscillations [S]
| 3
|
| Gamma Rays [S]
| 3
|
| Sun: Corona [S]
| 3
|
| Sun: Solar Flares
| 2
|
| Solar Activity
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Sun: Chromosphere [S]
| 2
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 2
|
| Sun: Activity
| 2
|
| Techniques: Image Processing
| 2
|
| Sun: X-ray
| 2
|
| Sun: Geomagnetic Disturbances
| 1
|
| Sun: Failed Eruption
| 1
|
| Sun: Energetic Particles
| 1
|
| Sun: Dynamics
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Active Regions
| 1
|
| Solar Particle Emission
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Filament Eruptions
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Coronal Waves [S]
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar And Stellar Astrophysics
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Solar Active Region Filaments
| 1
|
| Quiescent Solar Prominence
| 1
|
| Plasma Physics
| 1
|
| Methods: Data Analysis
| 1
|
| Magnetohydrodynamics [S]
| 1
|
| Magnetic Fields
| 1
|
| Instabilities [H]
| 1
|
| Gamma-rays
| 1
|
| Techniques: X-ray Imaging
| 1
|
| Techniques: Simulation
| 1
|
| Sun: X-ray Stereoscopic Observations
| 1
|
| Sun: X-ray Emission
| 1
|
| Sun: Radio Radiation [S]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Observational Signatures
| 1
|
| Sun: Magnetosphere
| 1
|
| Sun: Magnetic Reconnection
| 1
|
| Sun: Magnetic Fields
| 1
|
| Sun: Machine Learning
| 1
|
| Sun: Instrumentation And Data Management
| 1
|
| Sun: Instrumental Effects
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: Hard X-ray Imaging
| 1
|
| Sun: Hard
| 1
|
| The Sun [S]
| 1
|