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: Particle Emission
| 13
|
| Interplanetary Medium [H]
| 13
|
| Sun: Coronal Mass Ejections
| 11
|
| Sun: Flares [S]
| 10
|
| Astrophysics
| 9
|
| Shock Waves
| 8
|
| Solar Wind [H]
| 6
|
| International Sun Earth Explorer 3
| 5
|
| Interplanetary Magnetic Fields [H]
| 5
|
| Shock Wave Propagation
| 5
|
| Solar Physics [S]
| 4
|
| Particle Acceleration
| 4
|
| Acceleration Of Particles
| 4
|
| Galactic Clusters
| 4
|
| Mass Distribution
| 3
|
| Solar Energetic Particles [H]
| 3
|
| Magnetohydrodynamics [S]
| 3
|
| Energetic Particles
| 3
|
| Astronomical Photometry
| 3
|
| Chemical Evolution
| 3
|
| Flare
| 2
|
| Physics - Space Physics [H]
| 2
|
| Evolutionary Model
| 2
|
| Particle Flux Density
| 2
|
| Galactic Evolution
| 2
|
| Magnetic Storms
| 2
|
| Space Weather
| 2
|
| Anisotropic Media
| 2
|
| Sun: Solar-terrestrial Relations
| 2
|
| Interplanetary Plasma: Shock Waves
| 2
|
| Interplanetary Plasma: Particle Propagation
| 2
|
| Solar Terrestrial Interactions
| 2
|
| Sun: Magnetic Fields
| 2
|
| Computerized Simulation
| 2
|
| Cluster Dynamic
| 2
|
| Solar Planetary Interactions
| 2
|
| Numerical Code
| 2
|
| Interplanetary Physics: Energetic Particles (7514)
| 2
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 2
|
| Proton Flux Density
| 2
|
| Solar Activity
| 2
|
| Solar Protons
| 2
|
| Protons
| 2
|
| Radiation
| 2
|
| Anisotropy
| 2
|
| Photochemical Reactions
| 2
|
| Flares
| 2
|
| Sep
| 2
|
| Propagation Model
| 1
|
| Projects
| 1
|
| Prediction Analysis Techniques
| 1
|
| Planetary Sciences: Solar System Objects: Mars
| 1
|
| Plages
| 1
|
| Particle Trajectories
| 1
|
| Particle Intensity
| 1
|
| Particle Event
| 1
|
| Particle Energy
| 1
|
| Particle Accelerators
| 1
|
| Observational Characteristic
| 1
|
| Numerical Modeling
| 1
|
| Nowcasting
| 1
|
| Natural Hazards: Space Weather (2101
| 1
|
| Monte Carlo Simulation
| 1
|
| Monte Carlo Methods
| 1
|
| Monte Carlo Method
| 1
|
| Methods: Numerical
| 1
|
| Metallicity
| 1
|
| Medium
| 1
|
| Mass Spectrometers
| 1
|
| Mars
| 1
|
| Magnetospheric Physics: Solar Wind/magnetosphere Interactions
| 1
|
| Magnetohydrodynamic Waves
| 1
|
| Magnetic Fields
| 1
|
| Magnetic Field
| 1
|
| Machine Learning Methods
| 1
|
| Iron Line
| 1
|
| Iron
| 1
|
| Interplanetary Space
| 1
|
| Interplanetary Shock
| 1
|
| Interplanetary Propagation
| 1
|
| Interplanetary Plasma: Solar Activity
| 1
|
| Interplanetary Plasma: Energetic Particles
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (4305
| 1
|
| Interplanetary
| 1
|
| Injection Rate
| 1
|
| Initial Mass
| 1
|
| Hubble Space Telescope
| 1
|
| Heliocentric Distance
| 1
|
| H Alpha Line
| 1
|
| Gravitational Lensing
| 1
|
| Gravitational Lenses
| 1
|
| Gravitational Fields
| 1
|
| Galaxy Evolution
| 1
|
| Galaxy Cluster
| 1
|
| Galaxies: Evolution
| 1
|
| Galaxies: Clusters: Individual: Abell 2218
| 1
|
| Galactic Wind
| 1
|
| Galactic Bulge
| 1
|
| Forecasting
| 1
|
| Filaments
| 1
|
| Faculae
| 1
|
| Equations Of Motion
| 1
|
| Energy Spectrum
| 1
|
| Energy Spectra
| 1
|
| Energy Range
| 1
|
| Energetic Particle
| 1
|
| Directional Evolution
| 1
|
| Data Reduction
| 1
|
| Cosmology: Observations
| 1
|
| Cosmic Gases
| 1
|
| Charged Particles
| 1
|
| Asymmetry
| 1
|
| Astronomical Spectroscopy
| 1
|
| Astronomical Models
| 1
|
| Applications Of Monte Carlo Methods
| 1
|
| Active Region
| 1
|
| 02.70.uu
| 1
|
| Wave-particle Interactions
| 1
|
| Upstream Region
| 1
|
| Time Dependence
| 1
|
| Theoretical Prediction
| 1
|
| Sun: Radio
| 1
|
| Sun: Interplanetary Transport
| 1
|
| Sun: Heliosphere [H]
| 1
|
| Sun: Filaments [S]
| 1
|
| Sun: Faculae [S]
| 1
|
| Sun: Activity
| 1
|
| Stellar Luminosity
| 1
|
| Statistical Modeling
| 1
|
| Spectrographs
| 1
|
| Spatial Distribution
| 1
|
| Spacecraft/atmosphere Interactions
| 1
|
| Spacecraft
| 1
|
| Space Radiation Environment
| 1
|
| Space Plasma Physics: Charged Particle Motion And Acceleration
| 1
|
| Solar X-rays
| 1
|
| Solar Wind–magnetosphere–ionosphere–atmosphere Coupling
| 1
|
| Solar Wind Structures
| 1
|
| Solar Variability
| 1
|
| Solar Radio Emission
| 1
|
| Solar Longitude
| 1
|
| Solar Energetic Particle Environment
| 1
|
| Solar Disc
| 1
|
| Solar Cosmic Rays: Space Research
| 1
|
| Solar Cosmic Rays: Interplanetary Space
| 1
|
| Solar Cosmic Rays: Geomagnetic Field
| 1
|
| Solar Corpuscular Radiation
| 1
|
| Solar Activity Effects
| 1
|
| Slow Propagation
| 1
|
| Shocks
| 1
|
| Shock Fronts
| 1
|
| Shock Front
| 1
|
| Sepem Application Server
| 1
|
| Sep Events
| 1
|
| Scientific Modeling
| 1
|
| Satellites
| 1
|
| Satellite-borne Instruments
| 1
|
| Red Shift
| 1
|
| Random Distribution
| 1
|
| Radio Signatures
| 1
|
| Radio Emissions (dynamic)
| 1
|
| Radiation Belts
| 1
|
| Proton Event
| 1
|
| Proton Energy
| 1
|
| 96.50.pw
| 1
|
| 96.50.bh
| 1
|
| 94.05.hk
| 1
|
| 7900)
| 1
|
| 7513)
| 1
|
| X Ray Astronomy
| 1
|