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
|
|---|
| Solar Wind [H]
| 19
|
| Interplanetary Turbulence [H]
| 8
|
| Sun: Corona [S]
| 5
|
| Solar Magnetic Reconnection
| 5
|
| Alfven Waves
| 3
|
| Planetary Magnetospheres
| 3
|
| Space Plasmas [H]
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Magnetohydrodynamics [S]
| 3
|
| Alfvén Waves
| 3
|
| Solar Coronal Holes [S]
| 2
|
| Plasma Physics
| 2
|
| Planetary Bow Shocks
| 2
|
| Interplanetary Physics [H]
| 2
|
| Fast Solar Wind
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Solar Coronal Heating [S]
| 1
|
| Potential Field Source Surface
| 1
|
| Convolutional Neural Network
| 1
|
| Plasma Astrophysics
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Comet Tails
| 1
|
| Pic Simulation
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Reconnection
| 1
|
| Kinetic Instability
| 1
|
| Ion Acoustic Waves
| 1
|
| Interstellar Plasma
| 1
|
| Sun: Magnetic Fields
| 1
|
| Asteroids
| 1
|
| Supergranulation
| 1
|
| Interplanetary Dust
| 1
|
| Interplanetary Discontinuities
| 1
|
| Very Long Baseline Interferometry
| 1
|
| Solar Wind Speed
| 1
|
| Sun: Active Regions
| 1
|
| Sun: Activity
| 1
|
| Solar Coronal Transients
| 1
|
| Deep Space Probes
| 1
|
| Slow Solar Wind [H]
| 1
|