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]
| 62
|
| Interplanetary Turbulence [H]
| 27
|
| Turbulence
| 26
|
| Space Plasmas [H]
| 15
|
| Sun: Heliosphere [H]
| 14
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 14
|
| Waves
| 12
|
| Plasmas
| 11
|
| Physics - Space Physics [H]
| 11
|
| Magnetohydrodynamics [S]
| 11
|
| Alfven Waves
| 10
|
| Solar Magnetic Reconnection
| 10
|
| Magnetic Fields
| 9
|
| Sun: Corona [S]
| 8
|
| Sun: Coronal Mass Ejections
| 7
|
| Magnetic Reconnection
| 7
|
| Planetary Magnetospheres
| 5
|
| Sun: Chromosphere [S]
| 5
|
| Methods: Numerical
| 5
|
| Sun: Transition Region [S]
| 5
|
| Acceleration Of Particles
| 4
|
| Interplanetary Magnetic Fields [H]
| 4
|
| Slow Solar Wind [H]
| 4
|
| Shock Waves
| 4
|
| Sun: UV Radiation [S]
| 4
|
| Planetary Bow Shocks
| 3
|
| Solar Coronal Heating [S]
| 3
|
| Sunspots [S]
| 3
|
| Planets And Satellites: Magnetic Fields
| 3
|
| Sun: Magnetic Fields
| 3
|
| Sun: Oscillations [S]
| 3
|
| Sun: Atmosphere [S]
| 2
|
| Techniques: Spectroscopic
| 2
|
| Sun: Active Regions
| 2
|
| Sun: Photosphere [S]
| 2
|
| Solar Physics [S]
| 2
|
| Solar-planetary Interactions
| 2
|
| Interplanetary Shocks [H]
| 2
|
| Alfvén Waves
| 2
|
| Solar Activity
| 2
|
| Line: Profiles
| 2
|
| Physics - Plasma Physics [H]
| 2
|
| Mercury (planet)
| 2
|
| Fast Solar Wind
| 2
|
| Sun: Filaments [S]
| 2
|
| Magnetohydrodynamical Simulations
| 2
|
| Interplanetary Physics [H]
| 1
|
| Interplanetary Medium [H]
| 1
|
| Interplanetary Dust
| 1
|
| Interplanetary Discontinuities
| 1
|
| Interchange Reconnection
| 1
|
| In Situ Measurements
| 1
|
| High-speed Electron Flow
| 1
|
| Geomagnetic Activity
| 1
|
| Energy Dissipation
| 1
|
| Electron Acceleration
| 1
|
| Earth's Magnetotail
| 1
|
| Earth
| 1
|
| Deep Space Mission
| 1
|
| Coronal Magnetic Field
| 1
|
| Convolutional Neural Network
| 1
|
| Computational Methods
| 1
|
| Comet Tails
| 1
|
| Collisionless Shock
| 1
|
| Asteroids
| 1
|
| Venusian Induced Magnetosphere
| 1
|
| Thermal-electric Conversion
| 1
|
| Thermal Protection System
| 1
|
| The Sun [S]
| 1
|
| Tangential Discontinuity
| 1
|
| Supergranulation
| 1
|
| Sun: Turbulence
| 1
|
| Sun: Solar Wind [H]
| 1
|
| Sun: Particle Emission
| 1
|
| Sun: Low Coronal Signatures
| 1
|
| Sun: Heating
| 1
|
| Sun: Granulation [S]
| 1
|
| Sun: Coronal Mass Ejection: CMEs
| 1
|
| Sun: Coronal
| 1
|
| Sun: Activity
| 1
|
| Sun: Abundances
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar Wind Speed
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Particle Emission
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Dynamo
| 1
|
| Solar Cycle
| 1
|
| Solar Coronal Transients
| 1
|
| Solar Coronal Loops [S]
| 1
|
| Solar Coronal Holes [S]
| 1
|
| Solar Activities
| 1
|
| Small Flux Rope
| 1
|
| Shocks
| 1
|
| Rolling Back Magnetic Field Lines
| 1
|
| Red Equatorial Aurora
| 1
|
| Quiet Sun
| 1
|
| Potential Field Source Surface
| 1
|
| Plasma Physics
| 1
|
| Plasma Astrophysics
| 1
|
| Planets And Satellites: Terrestrial Planets
| 1
|
| Planets And Satellites: Physical Evolution
| 1
|
| Planetary Science
| 1
|
| Planetary Boundary Layers
| 1
|
| Pickup Ions
| 1
|
| Parallel Electric Field
| 1
|
| Mms
| 1
|
| Mhd Turbulence
| 1
|
| Mhd Simulation
| 1
|
| Maunder Minimum
| 1
|
| Mars
| 1
|
| Whistler Wave
| 1
|