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]
| 38
|
| Sun: Corona [S]
| 21
|
| Solar Wind [H]
| 20
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 19
|
| Sun: Coronal Mass Ejections
| 16
|
| Methods: Numerical
| 11
|
| Physics - Space Physics [H]
| 10
|
| Interplanetary Medium [H]
| 7
|
| Magnetohydrodynamical Simulations
| 6
|
| Waves
| 4
|
| Physics - Plasma Physics [H]
| 4
|
| Space Weather
| 3
|
| Magnetic Fields
| 3
|
| Magnetohydrodynamic Waves
| 3
|
| Sun: Solar Wind [H]
| 3
|
| Solar Cycle
| 3
|
| Sun: Magnetic Fields
| 3
|
| 52.35.bj
| 3
|
| Sun: Atmosphere [S]
| 3
|
| Tokamaks Spherical Tokamaks
| 2
|
| Sun: Magnetic Topology
| 2
|
| Sun: Interior [S]
| 2
|
| Sun: Heliosphere [H]
| 2
|
| Solar Coronal Waves [S]
| 2
|
| Solar Coronal Heating [S]
| 2
|
| Plasma Dynamics And Flow
| 2
|
| Physics - Computational Physics
| 2
|
| Magnetohydrodynamics And Plasmas
| 2
|
| Astrophysics
| 2
|
| Alfven Waves
| 2
|
| 95.30.qd
| 2
|
| 52.55.fa
| 2
|
| 52.30.cv
| 2
|
| 52.30.-q
| 2
|
| 47.65.+a
| 2
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Solar Coronal Lines
| 1
|
| 52.70.-m
| 1
|
| Solar Active Regions [S]
| 1
|
| Slow Solar Wind [H]
| 1
|
| Shock Waves
| 1
|
| Scientific Computing
| 1
|
| Relativity
| 1
|
| Radiative Transfer [S]
| 1
|
| Quiet Sun
| 1
|
| Polarization Field.
| 1
|
| Alfvén Waves
| 1
|
| Plasma Diagnostic Techniques And Instrumentation
| 1
|
| Planet Hosting Stars
| 1
|
| Sun: Models
| 1
|
| Sun: Observations
| 1
|
| Physics - Fluid Dynamics
| 1
|
| 52.35.-g
| 1
|
| Monte Carlo Methods
| 1
|
| Sun: Photosphere [S]
| 1
|
| Waves Oscillations And Instabilities In Plasmas And Intense Beams
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Structures
| 1
|
| Sun: Surface Magnetism [S]
| 1
|
| Magnetogram
| 1
|
| Sun: Transition Region [S]
| 1
|
| Line: Profiles
| 1
|
| Jeans Instability
| 1
|
| Ism: Jets And Outflows
| 1
|
| Ionization
| 1
|
| Interplanetary Turbulence [H]
| 1
|
| Interplanetary Physics [H]
| 1
|
| Sun: Uv Radiation [S]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Inhomogeneous Plasma
| 1
|
| Hydrodynamics
| 1
|
| Hydrodynamical Simulations
| 1
|
| High Resolution Spectroscopy
| 1
|
| G Dwarf Stars
| 1
|
| Flux Emergence.
| 1
|
| Flux Emergence
| 1
|
| Extreme Ultraviolet Astronomy
| 1
|
| Exoplanets
| 1
|
| Distributed Computing
| 1
|
| Cosmic Rays
| 1
|
| Computational Mhd
| 1
|
| Cme Propagation
| 1
|
| Techniques: Spectroscopic
| 1
|
| Stellar Winds
| 1
|
| Stellar Coronae
| 1
|
| Spectrophotometry
| 1
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 1
|
| Space Plasmas [H]
| 1
|
| Space Plasma Physics
| 1
|
| Solar Wind Cme Initiation
| 1
|
| Sun: E
| 1
|
| Solar Transition Region
| 1
|
| Solar Spectral Irradiance
| 1
|
| Solar Flares And Cmes
| 1
|
| Sun: Magnetohydrodynamics
| 1
|