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: Coronal Mass Ejections
| 75
|
| Solar Wind [H]
| 36
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 36
|
| Physics - Space Physics [H]
| 27
|
| Sun: Heliosphere [H]
| 25
|
| Space Weather
| 15
|
| Solar-terrestrial Relations
| 12
|
| Sun: Corona [S]
| 10
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 8
|
| Astrophysics - Earth And Planetary Astrophysics
| 8
|
| Solar─terrestrial Relations
| 7
|
| Sun: Solar Wind [H]
| 7
|
| Sun: Flares [S]
| 6
|
| Space Physics
| 6
|
| Magnetohydrodynamics [S]
| 6
|
| Solar And Stellar Astrophysics
| 5
|
| Sun: Physics - Space Physics
| 5
|
| Sun: Coronal Mass Ejection
| 5
|
| Solar Physics [S]
| 4
|
| Heliophysics
| 4
|
| Sun: Interplanetary Coronal Mass Ejection
| 4
|
| Shock Waves
| 4
|
| Sun: Space Weather
| 4
|
| Sun: Filaments [S]
| 4
|
| Solar Coronal Holes [S]
| 3
|
| Flux Ropes
| 3
|
| Driver Gases
| 3
|
| Ensemble Modeling
| 3
|
| Interplanetary Magnetic Field
| 3
|
| Sun: Magnetic Cloud
| 3
|
| Dynamical Evolution
| 3
|
| Heliospheric Imaging
| 3
|
| Interplanetary Physics: Ejecta
| 3
|
| Space Weather Prediction
| 3
|
| Sun: Interplanetary
| 3
|
| And Magnetic Clouds
| 3
|
| Sun: Magnetic Fields
| 3
|
| Sun: Flux Rope
| 3
|
| Drag-based Model
| 3
|
| Sun: Low Coronal Signatures
| 2
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 2
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 2
|
| Interplanetary Physics [H]
| 2
|
| Interplanetary Medium [H]
| 2
|
| Interplanetary Magnetic Fields [H]
| 2
|
| Sun: Interplanetary Coronal Mass Ejections
| 2
|
| Inner Heliosphere
| 2
|
| Planets And Satellites: Atmospheres
| 2
|
| Sun: Evolution
| 2
|
| Sun: Photosphere [S]
| 2
|
| Space Weather Forecasting
| 2
|
| Sun: Ecliptic Plane
| 2
|
| Geomagnetic Storms
| 2
|
| Galactic Cosmic Rays
| 2
|
| Forecasting
| 2
|
| Sun: Dynamics
| 2
|
| Sun: Disturbances
| 2
|
| Sun: Initiation And Propagation
| 2
|
| Solar Storm
| 2
|
| Sun: Radio Radiation [S]
| 2
|
| Ejecta
| 2
|
| Earth And Planetary Astrophysics
| 2
|
| Methods: Analytical
| 2
|
| Sun: Solar Phys
| 2
|
| Mars
| 2
|
| Solar Energetic Particles [H]
| 2
|
| Sun: Icmes
| 2
|
| Catalogs
| 2
|
| Sun: Arrival Time
| 2
|
| The Sun [S]
| 2
|
| Stereo
| 2
|
| Interplanetary Turbulence [H]
| 2
|
| Sdo Workshop
| 1
|
| Sdo 3
| 1
|
| Sdo
| 1
|
| Scattering
| 1
|
| Radially Aligned Spacecraft
| 1
|
| Quasi-perpendicular Bow Shock
| 1
|
| Prediction
| 1
|
| Plasmas
| 1
|
| Plasma Instability
| 1
|
| Plasma Alfven Waves
| 1
|
| Planets And Satellites: Physical Evolution
| 1
|
| Planet-star Interactions
| 1
|
| Physics - Plasma Physics [H]
| 1
|
| Physics - Geophysics
| 1
|
| Physics - Computational Physics
| 1
|
| Pattern Recognition
| 1
|
| Operational
| 1
|
| Off Sun-earth Line Observations
| 1
|
| Neural Networks
| 1
|
| Nasa/maven
| 1
|
| Multi-viewpoint Observations
| 1
|
| Msl/rad
| 1
|
| Models
| 1
|
| Mission Concept
| 1
|
| Mirror Modes
| 1
|
| Mhd Models
| 1
|
| Methods: Statistical
| 1
|
| Methods: Observational
| 1
|
| Methods: Numerical
| 1
|
| Maven Mission
| 1
|
| Mathematical Expression
| 1
|
| Magnetosheath
| 1
|
| Magnetometer Data
| 1
|
| Magnetometer
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Flux Ropes
| 1
|
| Magnetic Fields
| 1
|
| Magnetic Field
| 1
|
| Magnetic Cloud
| 1
|
| Magnetic Cleanliness
| 1
|
| Magnetic Bright Points
| 1
|
| Machine Learning
| 1
|
| Lws/sdo-3/soho-26/gong-2011 Workshop
| 1
|
| Lstm
| 1
|
| Lagrange 5 Point
| 1
|
| Interplanetary Space
| 1
|
| Interplanetary Shocks [H]
| 1
|
| Interplanetary Physics: Solar Wind Plasma [H]
| 1
|
| Interplanetary Coronal Mass Ejections
| 1
|
| Instrumentation And Methods For Astrophysics
| 1
|
| Instabilities [H]
| 1
|
| Icmes
| 1
|
| Icme
| 1
|
| Hydrodynamics
| 1
|
| Huxt
| 1
|
| Hinode/sot
| 1
|
| High Energy Astrophysical Phenomena
| 1
|
| Heliospheric Physics
| 1
|
| Heliospheric Imagers
| 1
|
| Heliophysics System Observatory
| 1
|
| Geometric Modeling
| 1
|
| Geomagnetically Induced Currents
| 1
|
| Forward Modeling
| 1
|
| Forecasts
| 1
|
| Forbush Secrease
| 1
|
| Forbush Effect
| 1
|
| Forbush Decreases
| 1
|
| Flux Rope Modeling
| 1
|
| Flux Rope
| 1
|
| Filament Plasma
| 1
|
| Elevohi
| 1
|
| Earth-impacting CMEs
| 1
|
| Early Warning
| 1
|
| Dst Index
| 1
|
| Data Analysis
| 1
|
| Cosmic Rays
| 1
|
| Corotating Streams
| 1
|
| Corona [S]
| 1
|
| Computer Science - Machine Learning
| 1
|
| Community Initiative
| 1
|
| Comets: Individual: 67p/churyumov-gerasimenko
| 1
|
| Comets: General
| 1
|
| CME-solar Wind Interaction
| 1
|
| CME Prediction
| 1
|
| CME
| 1
|
| Bow Shock
| 1
|
| Automatic Detection
| 1
|
| Atmospheric And Oceanic Physics
| 1
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 1
|
| Astrophysics
| 1
|
| Astrophysical Plasma
| 1
|
| Arrive Time Prediction
| 1
|
| Vigil
| 1
|
| Validation
| 1
|
| Uncertainty
| 1
|
| Techniques: Image Processing
| 1
|
| Sun: Velocity Histogram
| 1
|
| Sun: Velocity Fields
| 1
|
| Sun: Sun: Coronal Mass Ejections (cmes)
| 1
|
| Sun: Sun: Corona
| 1
|
| Sun: Stereo Spacecraft
| 1
|
| Sun: Stereo
| 1
|
| Sun: Solar Cycle
| 1
|
| Sun: Small Solar Wind Flux Ropes
| 1
|
| Sun: Slow Solar Wind
| 1
|
| Sun: Radially Aligned Spacecraft
| 1
|
| Sun: Propagation Direction
| 1
|
| Sun: Propagation Angle
| 1
|
| Sun: Prominences
| 1
|
| Sun: Methods
| 1
|
| Sun: Magnetohydrodynamics
| 1
|
| Sun: Magnetic Field Line Twist
| 1
|
| Sun: Magnetic Clouds
| 1
|
| Sun: Kink Wave
| 1
|
| Sun: Kinematics
| 1
|
| Sun: Inner Heliosphere
| 1
|
| Sun: In-situ Data
| 1
|
| Sun: Impulsive Phase
| 1
|
| Sun: High Active Region
| 1
|
| Sun: Helmet Streamer
| 1
|
| Sun: Heliospheric Imagers
| 1
|
| Sun: Heliospheric Imager
| 1
|
| Sun: Heliocentric Distance
| 1
|
| Sun: Granular Velocity
| 1
|
| Sun: Grad-shafranov Reconstruction
| 1
|
| Sun: Galactic
| 1
|
| Sun: Flux Ropes
| 1
|
| Sun: Flare
| 1
|
| Sun: Electron Temperature
| 1
|
| 4315)
| 1
|
| Sun: Corotating Interaction Region
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Carrington Rotation
| 1
|
| Sun: Bright Point
| 1
|
| Sun: Analytical Models
| 1
|
| Sun: Advance Composition Explorer
| 1
|
| Sun: Activity
| 1
|
| Sub-storm
| 1
|
| Stealth CMEs
| 1
|
| Stars: Late-type
| 1
|
| Stars: Flare
| 1
|
| Spacecraft Constellation
| 1
|
| Space Weather: Solar Effects
| 1
|
| Space Weather: Models
| 1
|
| Space Weather: Magnetic Storms (2788)
| 1
|
| Space Weather: Forecasting (2722)
| 1
|
| Space Weather: Forecasting (1922
| 1
|
| Space Weather Monitor
| 1
|
| Space Weather Forecasts
| 1
|
| Space Plasma Physics: Transport Processes
| 1
|
| Solar Wind Modeling
| 1
|
| Solar Wind Measurements
| 1
|
| Solar System
| 1
|
| Solar Rotation
| 1
|
| Solar Magnetism
| 1
|
| Solar Magnetic Flux Emergence
| 1
|
| Solar Extreme Ultraviolet Emission [S]
| 1
|
| Solar Dynamic Observatory
| 1
|
| Solar Cosmic Ray Particles
| 1
|
| Solar Coronal Heating [S]
| 1
|
| Solar Activity
| 1
|
| Small Solar Wind Transients In 2007-2009
| 1
|
| Slow Solar Wind [H]
| 1
|
| Sdo-3
| 1
|
| Analytical Empirical Models
| 1
|
| Active Solar Corona
| 1
|
| Acceleration Of Particles
| 1
|
| Sun: Cosmic Rays
| 1
|