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: Magnetic Fields
| 43
|
| Sun: Corona [S]
| 32
|
| Sun: Flares [S]
| 22
|
| Sun: Coronal Mass Ejections
| 18
|
| Sun: Active Regions
| 18
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 13
|
| Sun: Photosphere [S]
| 8
|
| Sun: Magnetic Reconnection
| 8
|
| Sun: Flare
| 7
|
| Sun: Astrophysics - Solar And Stellar Astrophysics
| 7
|
| Sun: Activity
| 6
|
| Sun: Relation To Magnetic Field
| 6
|
| Magnetic Fields
| 6
|
| Sun: Solar Wind [H]
| 6
|
| Magnetohydrodynamics [S]
| 6
|
| Sun: X-rays [S]
| 5
|
| Gamma Rays [S]
| 5
|
| Sun: Helicity
| 5
|
| Sun: Dynamics
| 5
|
| Sun: Magnetic
| 5
|
| Sun: Coronal Mass Ejection
| 5
|
| Astrophysics
| 4
|
| Solar Physics [S]
| 4
|
| Solar Wind [H]
| 4
|
| Sun: Solar Phys
| 4
|
| Sun: Radio Radiation [S]
| 4
|
| Sun: UV Radiation [S]
| 3
|
| Sun: Low Coronal Signatures
| 3
|
| Sun: Chromosphere [S]
| 3
|
| Sun: Atmosphere [S]
| 3
|
| Sun: Association With Flares
| 3
|
| Sun: Models
| 3
|
| Sun: Structures
| 3
|
| Driver Gases
| 3
|
| Sun: Radio Bursts
| 3
|
| Sun: Active Region
| 3
|
| Sun: Magnetic Topology
| 3
|
| Sun: Solar Magnetic Field
| 3
|
| Sun: Heliosphere [H]
| 2
|
| Sun: Magnetic Field Reconnection
| 2
|
| Sun: Observational Signatures
| 2
|
| Sunspots [S]
| 2
|
| Sun: Michelson Doppler Imager
| 2
|
| Interplanetary Physics: Interplanetary Magnetic Fields [H]
| 2
|
| Sun: Interplanetary
| 2
|
| Interplanetary Physics: Ejecta
| 2
|
| Sun: Interior [S]
| 2
|
| Sun: Photospheric Magnetic Field
| 2
|
| Sun: Filaments [S]
| 2
|
| Sun: Waves
| 2
|
| Sun: Velocity Field
| 2
|
| Sun: Astrophysics
| 2
|
| Sun: Magnetic Flux
| 2
|
| And Magnetic Clouds
| 2
|
| Sun: Solar Flares
| 2
|
| Sun: Microwave
| 2
|
| Sun: X-ray Bursts
| 2
|
| Sun: Active
| 2
|
| Sun: Solar Flare
| 2
|
| Sun: Magnetic Extrapolations
| 2
|
| Magnetospheric Physics: Solar Wind/magnetosphere Interactions
| 2
|
| Methods: Data Analysis
| 2
|
| Sun: Magnetic Field
| 2
|
| Sun: Coronal Hole
| 2
|
| Methods: Statistical
| 2
|
| Sun: Magnetic Cloud
| 2
|
| Sun: Coronal Mass Ejections: Interplanetary
| 2
|
| Magnetic Flux
| 2
|
| Sun: Coronal Mass Ejections: Low Coronal Signatures
| 2
|
| Sun: Magnetic Field Configurations
| 2
|
| Sun: Frequency Drift
| 1
|
| Sun: Free Magnetic Energy
| 1
|
| Sun: Force-free Magnetic Fields
| 1
|
| Sun: Flux Tube
| 1
|
| Sun: Flux Transport
| 1
|
| Sun: Flux Emergence
| 1
|
| Sun: Field Line
| 1
|
| Sun: Field Aligned Currents
| 1
|
| Sun: Evolution
| 1
|
| Sun: Drift Rate
| 1
|
| Sun: Disturbances
| 1
|
| Sun: Coronal Mass Ejection: Interplanetary
| 1
|
| Sun: Coronal Magnetic Field
| 1
|
| Sun: Coronal Loop
| 1
|
| Sun: Coronal Holes
| 1
|
| Sun: Coronal
| 1
|
| Sun: Corona: Models
| 1
|
| Sun: Corona E
| 1
|
| Sun: Corona Active
| 1
|
| Sun: Constant Amplitude
| 1
|
| Sun: Coherence
| 1
|
| Sun: Brightness Distribution
| 1
|
| Sun: Bright Point
| 1
|
| Sun: Atomic
| 1
|
| Sun: Atmospheric Motions
| 1
|
| Sun: Aso-s Mission
| 1
|
| Sun: Argentina
| 1
|
| Sun: Active Research Area
| 1
|
| Sun: Active Regions: Structure
| 1
|
| Sun: Active Regions: Magnetic Fields
| 1
|
| Sun: Active Region Upflow
| 1
|
| Sun: Abundances
| 1
|
| Stellar Spectra
| 1
|
| Stellar Evolution
| 1
|
| Stellar Atmospheres
| 1
|
| Space Weather: Solar Effects
| 1
|
| Space Weather: Magnetic Storms (2788)
| 1
|
| Space Weather: General Or Miscellaneous
| 1
|
| Space Weather: Forecasting (2722)
| 1
|
| Space Weather
| 1
|
| Solar-terrestrial Relations
| 1
|
| Solar X-ray And Gamma-ray Emission
| 1
|
| Solar Ultraviolet Emission [S]
| 1
|
| Solar Magnetism
| 1
|
| Solar Magnetic Field
| 1
|
| Solar Energetic Particles [H]
| 1
|
| Solar Activity
| 1
|
| Solar Active-region Magnetic Fields
| 1
|
| Slow Solar Wind [H]
| 1
|
| Reconnection
| 1
|
| Radial Velocity
| 1
|
| Precipitating
| 1
|
| Physics - Space Physics [H]
| 1
|
| Natural Hazards: Space Weather (2101
| 1
|
| Methods: Numerical
| 1
|
| Methods: Miscellaneous
| 1
|
| Magnetospheric Physics: Storms And Substorms
| 1
|
| Magnetospheric Physics: Ring Current
| 1
|
| Magnetospheric Physics: Energetic Particles
| 1
|
| Magnetospheric Physics: Current Systems (2409)
| 1
|
| Magnetic Signatures
| 1
|
| Magnetic Reconnection
| 1
|
| Magnetic Field Reconnection
| 1
|
| Magnetic Field Effects
| 1
|
| Magnetic Field
| 1
|
| Magnetic Clouds
| 1
|
| Lines Of Force
| 1
|
| Interplanetary Physics: Solar Wind Sources
| 1
|
| Interplanetary Physics: Energetic Particles (7514)
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (7513)
| 1
|
| Interplanetary Physics: Coronal Mass Ejections (4305
| 1
|
| Interplanetary Medium [H]
| 1
|
| Interplanetary Magnetic Fields [H]
| 1
|
| Instrumentation: Spectrographs
| 1
|
| Instrumentation: High Angular Resolution
| 1
|
| Free Energy
| 1
|
| Flares
| 1
|
| Energy Transfer
| 1
|
| Energy Conversion
| 1
|
| Ejecta
| 1
|
| Cospar/ilws Road Map Panel
| 1
|
| Coronal Loops
| 1
|
| Corona [S]
| 1
|
| Bipolar Sunspot Groups
| 1
|
| Binary Stars
| 1
|
| B Stars
| 1
|
| Astrophysics - Earth And Planetary Astrophysics
| 1
|
| Astronomical Catalogues
| 1
|
| Three Dimensional Models
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Sun: X-ray: Gamma Rays
| 1
|
| Sun: X-ray
| 1
|
| Sun: X Ray Spectroscopy
| 1
|
| Sun: Velocity Fields
| 1
|
| Sun: Transition Region [S]
| 1
|
| Sun: Trace Image
| 1
|
| Sun: Topology
| 1
|
| Sun: Topological Structure
| 1
|
| Sun: Sun: Magnetic Fields
| 1
|
| Sun: Sun: Flares
| 1
|
| Sun: Sun: Filament Eruptions
| 1
|
| Sun: Subsurface Flows
| 1
|
| Sun: Structure
| 1
|
| Sun: Stellar Models
| 1
|
| Sun: Spectral Line
| 1
|
| Sun: Space Weather
| 1
|
| Sun: Solar Wind: Disturbances
| 1
|
| Sun: Solar Synoptic Maps
| 1
|
| Sun: Solar Maximum Mission
| 1
|
| Sun: Solar Corona
| 1
|
| Sun: Solar Activity Cycle
| 1
|
| Sun: Slow Solar Wind Contribution
| 1
|
| Sun: Shear Velocity
| 1
|
| Sun: Remote-sensing
| 1
|
| Sun: Relevant Information
| 1
|
| Sun: Region Loop
| 1
|
| Sun: Reconnection Process
| 1
|
| Sun: Radio Emission
| 1
|
| Sun: Radio Burst
| 1
|
| Sun: Quiet Sun
| 1
|
| Sun: Propagation
| 1
|
| Sun: Prominences
| 1
|
| Sun: Polar Coronal Hole
| 1
|
| Sun: Plasma Flow
| 1
|
| Sun: Physical Sciences
| 1
|
| Sun: Output Layer
| 1
|
| Sun: Origins
| 1
|
| Sun: Observations
| 1
|
| Sun: Null Point
| 1
|
| Sun: Neural Network
| 1
|
| Sun: Monotonic Function
| 1
|
| Sun: Michelson Doppler Imager Magnetogram
| 1
|
| Sun: Mathematical Models
| 1
|
| Sun: Magnetic Region
| 1
|
| Sun: Magnetic Reconnection: Observational Signatures
| 1
|
| Sun: Magnetic Polis
| 1
|
| Sun: Magnetic Polarity
| 1
|
| Sun: Magnetic Inversion Line
| 1
|
| Sun: Magnetic Fields: Interplanetary
| 1
|
| Sun: Magnetic Field: Photosphere
| 1
|
| Sun: Magnetic Field: Interplanetary
| 1
|
| Sun: Magnetic Field Line
| 1
|
| Sun: Magnetic Energy Storage
| 1
|
| Sun: Magnetic Energy
| 1
|
| Sun: Longitudinal Magnetic Field
| 1
|
| Sun: Latitudinal Distribution
| 1
|
| Sun: Interplanetary Ejecta
| 1
|
| Sun: Initiation And Propagation
| 1
|
| Sun: Infrared
| 1
|
| Sun: Imaging Spectrometers
| 1
|
| Sun: High Temperature Plasmas
| 1
|
| Sun: Hide Layer
| 1
|
| Sun: Helioseismology [S]
| 1
|
| Sun: Heliocentric Distance
| 1
|
| Sun: Helicity: Magnetic
| 1
|
| Sun: Heating
| 1
|
| Sun: Geomagnetic Storm
| 1
|
| Sun: General
| 1
|
| Active Solar Chromosphere
| 1
|
| 7513)
| 1
|