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]
| 20
|
| Interplanetary Turbulence [H]
| 9
|
| Sun: Corona [S]
| 6
|
| Solar Magnetic Reconnection
| 5
|
| Magnetohydrodynamics [S]
| 5
|
| Alfvén Waves
| 3
|
| Interplanetary Magnetic Fields [H]
| 3
|
| Space Plasmas [H]
| 3
|
| Alfven Waves
| 3
|
| Plasma Physics
| 3
|
| Planetary Magnetospheres
| 3
|
| Sun: Heliosphere [H]
| 3
|
| Solar Coronal Holes [S]
| 2
|
| Planetary Bow Shocks
| 2
|
| Sun: Coronal Mass Ejections
| 2
|
| Sun: Magnetic Fields
| 2
|
| Fast Solar Wind
| 2
|
| Interplanetary Physics [H]
| 2
|
| Interplanetary Dust
| 1
|
| Gamma-ray Astronomy
| 1
|
| Deep Space Probes
| 1
|
| Cosmic Rays
| 1
|
| Cosmic Ray Astronomy
| 1
|
| Convolutional Neural Network
| 1
|
| Comet Tails
| 1
|
| Asteroids
| 1
|
| Very Long Baseline Interferometry
| 1
|
| Supergranulation
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Atmosphere [S]
| 1
|
| Sun: Activity
| 1
|
| Sun: Active Regions
| 1
|
| Solar Wind Speed
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Potential Field Source Surface
| 1
|
| Plasma Astrophysics
| 1
|
| Pic Simulation
| 1
|
| Magnetohydrodynamical Simulations
| 1
|
| Magnetic Reconnection
| 1
|
| Kinetic Instability
| 1
|
| Ion Acoustic Waves
| 1
|
| Interstellar Plasma
| 1
|
| Interplanetary Discontinuities
| 1
|