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: Coronal Mass Ejections
| 7
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 6
|
| Magnetohydrodynamics [S]
| 5
|
| Methods: Numerical
| 4
|
| Sun: Corona [S]
| 3
|
| Physics - Space Physics [H]
| 3
|
| Solar Wind [H]
| 2
|
| Sun: Flares [S]
| 2
|
| Sun: Filaments [S]
| 2
|
| Methods: Observational
| 2
|
| Sun: Chromosphere [S]
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Sun: Active
| 1
|
| Space Weather
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Potential Field Source Surface
| 1
|
| Methods: Data Analysis
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetograms
| 1
|
| Magnetic Storms
| 1
|
| Magnetic Reconnection
| 1
|
| Low-coronal Signatures
| 1
|
| 00-01
| 1
|
| Sun: UV Radiation [S]
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Sun: Modelling
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Oscillations [S]
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Heating
| 1
|
| Sun: Dynamics
| 1
|
| 99-00
| 1
|
| Wang-sheeley-arge
| 1
|