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
|
| Magnetohydrodynamics [S]
| 10
|
| Interplanetary Turbulence [H]
| 9
|
| Physics - Space Physics [H]
| 8
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 8
|
| Turbulence
| 6
|
| Methods: Numerical
| 5
|
| Sun: Corona [S]
| 5
|
| Magnetohydrodynamical Simulations
| 4
|
| Magnetic Reconnection
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Sun: Coronal Mass Ejections
| 3
|
| Waves
| 3
|
| Physics - Plasma Physics [H]
| 3
|
| Astrophysics - Earth And Planetary Astrophysics
| 2
|
| Astrophysics
| 2
|
| Solar Physics [S]
| 2
|
| Interplanetary Physics [H]
| 2
|
| Solar Magnetic Reconnection
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Fast Solar Wind
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Slow Solar Wind [H]
| 2
|
| Magnetic Fields
| 2
|
| Time-dependent
| 1
|
| Theory
| 1
|
| Space Plasmas [H]
| 1
|
| Space Plasma Physics: Mathematical And Numerical Techniques (0500
| 1
|
| Solar Wind Simulation
| 1
|
| Solar Minimum
| 1
|
| Solar Coronal Mass Ejection Shocks
| 1
|
| Solar Atmosphere
| 1
|
| Shock Waves
| 1
|
| Polar Field
| 1
|
| Numerical Simulation
| 1
|
| Numerical Mhd Method
| 1
|
| Mhd Model
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Dust
| 1
|
| Daily-updated Data As Input
| 1
|
| 3200)
| 1
|
| Computational Geophysics: Modeling (1952
| 1
|
| Comet Tails
| 1
|
| Asteroids
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Corona
| 1
|
| Alfvén
| 1
|
| Alfven Waves
| 1
|
| 4316)
| 1
|
| Computational Methods
| 1
|