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: Magnetic Fields
| 13
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 12
|
| Sunspots [S]
| 11
|
| Sun: Filaments [S]
| 11
|
| Solar Magnetic Reconnection
| 9
|
| Sun: Flares [S]
| 8
|
| Sun: Photosphere [S]
| 7
|
| Solar Activity
| 7
|
| Sun: Coronal Mass Ejections
| 5
|
| Solar Filament Eruptions
| 5
|
| Sun: Activity
| 5
|
| Solar Atmosphere
| 4
|
| Solar Active Regions [S]
| 4
|
| Solar Active Region Magnetic Fields [S]
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Magnetic Fields
| 3
|
| Solar Coronal Transients
| 2
|
| Sun: Corona [S]
| 2
|
| Magnetohydrodynamics [S]
| 2
|
| Magnetic Reconnection
| 2
|
| Solar Magnetic Flux Emergence
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Sunspot Groups
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Evolution
| 1
|
| Solar Physics [S]
| 1
|
| Solar Observatories
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Evolution
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Chromospheric Heating
| 1
|
| Solar Active Region Velocity Fields
| 1
|
| Solar Active Region Filaments
| 1
|
| Quiet Solar Corona
| 1
|
| Penumbra
| 1
|
| Oscillations
| 1
|
| Methods: Numerical
| 1
|
| Jets
| 1
|
| Chromosphere
| 1
|
| Active Solar Chromosphere
| 1
|