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
|
|---|
| Magnetohydrodynamics [S]
| 8
|
| Sun: Corona [S]
| 7
|
| Sun: Magnetic Fields
| 6
|
| The Sun [S]
| 4
|
| Solar Coronal Heating [S]
| 4
|
| Solar Physics [S]
| 4
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 3
|
| Turbulence
| 3
|
| Solar Coronal Loops [S]
| 3
|
| Solar Coronal Waves [S]
| 2
|
| Sun: UV Radiation [S]
| 2
|
| Quiet Solar Corona
| 2
|
| Active Solar Corona
| 2
|
| Alfven Waves
| 2
|
| Ism: Atoms
| 1
|
| Ionization
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Gamma-rays
| 1
|
| Galactic Cosmic Rays
| 1
|
| Flares
| 1
|
| Extragalactic Magnetic Fields
| 1
|
| Coronal Mass Ejections─interplanetary Shocks
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics - High Energy Astrophysical Phenomena [S]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Coronal Mass Ejections
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Active Regions
| 1
|
| Starburst Galaxies
| 1
|
| Solar Wind [H]
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Granulation
| 1
|
| Solar Coronal Lines
| 1
|
| Slow Solar Wind [H]
| 1
|
| Polarimetry
| 1
|
| Methods: Numerical
| 1
|
| Ism: Magnetic Fields
| 1
|
| Ism: Clouds
| 1
|
| Waves
| 1
|