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
|
|---|
| Sun: Corona [S]
| 40
|
| Magnetohydrodynamics [S]
| 25
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 25
|
| Sun: Magnetic Fields
| 19
|
| Sun: Coronal Mass Ejections
| 18
|
| Solar Wind [H]
| 18
|
| Sun: Uv Radiation [S]
| 9
|
| Solar Physics [S]
| 6
|
| Sun: Activity
| 6
|
| Physics - Space Physics [H]
| 6
|
| Sun: Solar Wind [H]
| 5
|
| Corona [S]
| 5
|
| Electric And Magnetic Fields Solar Magnetism
| 5
|
| Sun: Heliosphere [H]
| 5
|
| 96.60.hv
| 5
|
| Astrophysics
| 5
|
| Sun: Flares [S]
| 5
|
| Turbulence
| 4
|
| Sun: Filaments [S]
| 4
|
| Photosphere [S]
| 4
|
| Gamma Rays [S]
| 3
|
| Magnetohydrodynamical Simulations
| 3
|
| Waves
| 3
|
| Magnetohydrodynamics And Plasmas
| 3
|
| Sun: Magnetic Topology
| 3
|
| 95.30.qd
| 3
|
| Magnetic Fields
| 3
|
| Solar Magnetism
| 3
|
| Sun: Atmosphere [S]
| 3
|
| Sun: X-rays [S]
| 3
|
| Sun: Transition Region [S]
| 2
|
| Solar Magnetic Flux Emergence
| 2
|
| Plasma Turbulence
| 2
|
| Plasma Alfven Waves
| 2
|
| Particle Emission Solar Wind [H]
| 2
|
| Methods: Numerical
| 2
|
| Magnetohydrodynamic Waves
| 2
|
| Interplanetary Medium [H]
| 2
|
| Instabilities [H]
| 2
|
| Hydrodynamics
| 2
|
| Astrophysical Plasma
| 2
|
| 96.60.vg
| 2
|
| 96.60.pb
| 2
|
| 96.60.p-
| 2
|
| 96.60.mz
| 2
|
| 52.35.bj
| 2
|
| 52.30.-q
| 2
|
| Plasma Dynamics And Flow
| 2
|
| Potential Field
| 1
|
| Plasma Temperature
| 1
|
| Plasma Properties
| 1
|
| 52.25.-b
| 1
|
| Plasma Density
| 1
|
| Plasma Astrophysics
| 1
|
| 52.25.fi
| 1
|
| Sources Of Solar Wind
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Fluid Dynamics
| 1
|
| Physics - Classical Physics
| 1
|
| Space Weather
| 1
|
| Topology
| 1
|
| Numerical Solutions
| 1
|
| Nonlinear Phenomena: Waves Wave Propagation And Other Interactions
| 1
|
| Nonlinear Equations
| 1
|
| Mhd Model
| 1
|
| 96.50.ci
| 1
|
| Methods: Data Analysis
| 1
|
| Mathematical Geophysics: Numerical Solutions
| 1
|
| Spectrometers
| 1
|
| Spectroscopy
| 1
|
| Streamer
| 1
|
| 96.50.bh
| 1
|
| Magnetohydrodynamic And Fluid Equation
| 1
|
| Sun: Fundamental Parameters
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field
| 1
|
| Magnetic Clouds
| 1
|
| Macroinstabilities
| 1
|
| Lines Of Force
| 1
|
| Kink Bands
| 1
|
| Ionization
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 1
|
| Interplanetary Physics: Interplanetary Shocks
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Physics: Ejecta
| 1
|
| Transport Properties
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| 95.30.lz
| 1
|
| 94.05.lk
| 1
|
| Sun: Particle Emission
| 1
|
| Fractional Charge States
| 1
|
| Flare
| 1
|
| Field Line
| 1
|
| Faraday Rotation
| 1
|
| Exploration
| 1
|
| Evolution
| 1
|
| Sun: Photosphere [S]
| 1
|
| Driver Gases
| 1
|
| Current Sheet
| 1
|
| Corotating Interaction Regions
| 1
|
| Coronal Mass Injections
| 1
|
| Coronal Magnetic Field
| 1
|
| Coronal Loops
| 1
|
| Sun: Prominences
| 1
|
| Chemical Abundances
| 1
|
| Sunspots [S]
| 1
|
| The Sun [S]
| 1
|
| 52.65.kj
| 1
|
| Astrophysical Fluid Dynamics
| 1
|
| And Magnetic Clouds
| 1
|
| And Astronomy: Magnetic Fields
| 1
|
| And Astronomy: Coronal Mass Ejections
| 1
|
| And Astronomy: Coronal Holes
| 1
|
| And Astronomy
| 1
|
| Alfven Waves
| 1
|
| Acceleration Of Particles
| 1
|
| 52.35.ra
| 1
|
| 96.60.ph
| 1
|
| Solar Storm
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Middle Corona
| 1
|
| Solar Wind Plasma [H]
| 1
|
| 52.35.py
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Corona: Plasma
| 1
|
| Solar Corona: Magnetohydrodynamics
| 1
|
| Solar Activity
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Recombination
| 1
|
| Radiation
| 1
|
| Quiet Solar Corona
| 1
|
| 52.35.mw
| 1
|